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Persson M, Aizawa S, André N, Barabash S, Saito Y, Harada Y, Heyner D, Orsini S, Fedorov A, Mazelle C, Futaana Y, Hadid LZ, Volwerk M, Collinson G, Sanchez-Cano B, Barthe A, Penou E, Yokota S, Génot V, Sauvaud JA, Delcourt D, Fraenz M, Modolo R, Milillo A, Auster HU, Richter I, Mieth JZD, Louarn P, Owen CJ, Horbury TS, Asamura K, Matsuda S, Nilsson H, Wieser M, Alberti T, Varsani A, Mangano V, Mura A, Lichtenegger H, Laky G, Jeszenszky H, Masunaga K, Signoles C, Rojo M, Murakami G. BepiColombo mission confirms stagnation region of Venus and reveals its large extent. Nat Commun 2022; 13:7743. [PMID: 36522338 PMCID: PMC9755131 DOI: 10.1038/s41467-022-35061-3] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/08/2022] [Accepted: 11/16/2022] [Indexed: 12/23/2022] Open
Abstract
The second Venus flyby of the BepiColombo mission offer a unique opportunity to make a complete tour of one of the few gas-dynamics dominated interaction regions between the supersonic solar wind and a Solar System object. The spacecraft pass through the full Venusian magnetosheath following the plasma streamlines, and cross the subsolar stagnation region during very stable solar wind conditions as observed upstream by the neighboring Solar Orbiter mission. These rare multipoint synergistic observations and stable conditions experimentally confirm what was previously predicted for the barely-explored stagnation region close to solar minimum. Here, we show that this region has a large extend, up to an altitude of 1900 km, and the estimated low energy transfer near the subsolar point confirm that the atmosphere of Venus, despite being non-magnetized and less conductive due to lower ultraviolet flux at solar minimum, is capable of withstanding the solar wind under low dynamic pressure.
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Affiliation(s)
- M. Persson
- grid.15781.3a0000 0001 0723 035XInstitut de Recherche en Astrophysique et Planétologie, Centre National de la Recherche Scientifique, Centre National d’Etudes Spatiales, Université Paul Sabatier—Toulouse III, Toulouse, France
| | - S. Aizawa
- grid.15781.3a0000 0001 0723 035XInstitut de Recherche en Astrophysique et Planétologie, Centre National de la Recherche Scientifique, Centre National d’Etudes Spatiales, Université Paul Sabatier—Toulouse III, Toulouse, France
| | - N. André
- grid.15781.3a0000 0001 0723 035XInstitut de Recherche en Astrophysique et Planétologie, Centre National de la Recherche Scientifique, Centre National d’Etudes Spatiales, Université Paul Sabatier—Toulouse III, Toulouse, France
| | - S. Barabash
- grid.425140.60000 0001 0706 1867Swedish Institute of Space Physics, Kiruna, Sweden
| | - Y. Saito
- grid.62167.340000 0001 2220 7916Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Kyoto, Japan
| | - Y. Harada
- grid.258799.80000 0004 0372 2033Department of Geophysics, Graduate School of Science, Kyoto University, Kyoto, Japan
| | - D. Heyner
- grid.6738.a0000 0001 1090 0254Institute for Geophysics and Extraterrestrial Physics, Technische Universität Braunschweig, Braunschweig, Germany
| | - S. Orsini
- grid.4293.c0000 0004 1792 8585Institute of Space Astrophysics and Planetology, Istituto Nazionale di Astrofisica, Rome, Italy
| | - A. Fedorov
- grid.15781.3a0000 0001 0723 035XInstitut de Recherche en Astrophysique et Planétologie, Centre National de la Recherche Scientifique, Centre National d’Etudes Spatiales, Université Paul Sabatier—Toulouse III, Toulouse, France
| | - C. Mazelle
- grid.15781.3a0000 0001 0723 035XInstitut de Recherche en Astrophysique et Planétologie, Centre National de la Recherche Scientifique, Centre National d’Etudes Spatiales, Université Paul Sabatier—Toulouse III, Toulouse, France
| | - Y. Futaana
- grid.425140.60000 0001 0706 1867Swedish Institute of Space Physics, Kiruna, Sweden
| | - L. Z. Hadid
- grid.508893.fLaboratoire de Physique des Plasmas (LPP), Centre National de la Recherche Scientifique, Observatoire de Paris, Sorbonne Université, Université Paris Saclay, École Polytechnique, Institut Polytechnique de Paris, Paris, France
| | - M. Volwerk
- grid.4299.60000 0001 2169 3852Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - G. Collinson
- grid.133275.10000 0004 0637 6666National Aeronautic and Space Administration, Goddard Space Flight Center, Greenbelt, MD USA
| | - B. Sanchez-Cano
- grid.9918.90000 0004 1936 8411School of Physics and Astronomy, University of Leicester, Leicester, UK
| | - A. Barthe
- grid.15781.3a0000 0001 0723 035XInstitut de Recherche en Astrophysique et Planétologie, Centre National de la Recherche Scientifique, Centre National d’Etudes Spatiales, Université Paul Sabatier—Toulouse III, Toulouse, France
| | - E. Penou
- grid.15781.3a0000 0001 0723 035XInstitut de Recherche en Astrophysique et Planétologie, Centre National de la Recherche Scientifique, Centre National d’Etudes Spatiales, Université Paul Sabatier—Toulouse III, Toulouse, France
| | - S. Yokota
- grid.136593.b0000 0004 0373 3971Department of Earth and Space Science, Graduate School of Science, Osaka University, Osaka, Japan
| | - V. Génot
- grid.15781.3a0000 0001 0723 035XInstitut de Recherche en Astrophysique et Planétologie, Centre National de la Recherche Scientifique, Centre National d’Etudes Spatiales, Université Paul Sabatier—Toulouse III, Toulouse, France
| | - J. A. Sauvaud
- grid.15781.3a0000 0001 0723 035XInstitut de Recherche en Astrophysique et Planétologie, Centre National de la Recherche Scientifique, Centre National d’Etudes Spatiales, Université Paul Sabatier—Toulouse III, Toulouse, France
| | - D. Delcourt
- grid.508893.fLaboratoire de Physique des Plasmas (LPP), Centre National de la Recherche Scientifique, Observatoire de Paris, Sorbonne Université, Université Paris Saclay, École Polytechnique, Institut Polytechnique de Paris, Paris, France
| | - M. Fraenz
- grid.435826.e0000 0001 2284 9011Max-Planck-Institute for Solar System Research, Göttingen, Germany
| | - R. Modolo
- Laboratoire Atmosphères, Milieux, Observations Spatiales, Institut Pierre Simon Laplace, Université Versailles Saint Quentin en Yvelines, Université Paris-Saclay, Université Pierre Marie Curie, Centre National de la Recherche Scientifique, Guyancourt, France
| | - A. Milillo
- grid.4293.c0000 0004 1792 8585Institute of Space Astrophysics and Planetology, Istituto Nazionale di Astrofisica, Rome, Italy
| | - H.-U. Auster
- grid.6738.a0000 0001 1090 0254Institute for Geophysics and Extraterrestrial Physics, Technische Universität Braunschweig, Braunschweig, Germany
| | - I. Richter
- grid.6738.a0000 0001 1090 0254Institute for Geophysics and Extraterrestrial Physics, Technische Universität Braunschweig, Braunschweig, Germany
| | - J. Z. D. Mieth
- grid.6738.a0000 0001 1090 0254Institute for Geophysics and Extraterrestrial Physics, Technische Universität Braunschweig, Braunschweig, Germany
| | - P. Louarn
- grid.15781.3a0000 0001 0723 035XInstitut de Recherche en Astrophysique et Planétologie, Centre National de la Recherche Scientifique, Centre National d’Etudes Spatiales, Université Paul Sabatier—Toulouse III, Toulouse, France
| | - C. J. Owen
- grid.83440.3b0000000121901201Mullard Space Science Laboratory, University College London, Holmbury St. Mary, UK
| | - T. S. Horbury
- grid.7445.20000 0001 2113 8111Imperial College London, South Kensington Campus, London, UK
| | - K. Asamura
- grid.62167.340000 0001 2220 7916Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Kyoto, Japan
| | - S. Matsuda
- grid.9707.90000 0001 2308 3329Graduate School of Natural Science and Technology, Kanazawa University, Kanazawa, Japan
| | - H. Nilsson
- grid.425140.60000 0001 0706 1867Swedish Institute of Space Physics, Kiruna, Sweden
| | - M. Wieser
- grid.425140.60000 0001 0706 1867Swedish Institute of Space Physics, Kiruna, Sweden
| | - T. Alberti
- grid.4293.c0000 0004 1792 8585Institute of Space Astrophysics and Planetology, Istituto Nazionale di Astrofisica, Rome, Italy
| | - A. Varsani
- grid.4299.60000 0001 2169 3852Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - V. Mangano
- grid.4293.c0000 0004 1792 8585Institute of Space Astrophysics and Planetology, Istituto Nazionale di Astrofisica, Rome, Italy
| | - A. Mura
- grid.4293.c0000 0004 1792 8585Institute of Space Astrophysics and Planetology, Istituto Nazionale di Astrofisica, Rome, Italy
| | - H. Lichtenegger
- grid.4299.60000 0001 2169 3852Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - G. Laky
- grid.4299.60000 0001 2169 3852Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - H. Jeszenszky
- grid.4299.60000 0001 2169 3852Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - K. Masunaga
- grid.62167.340000 0001 2220 7916Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Kyoto, Japan
| | - C. Signoles
- grid.15781.3a0000 0001 0723 035XInstitut de Recherche en Astrophysique et Planétologie, Centre National de la Recherche Scientifique, Centre National d’Etudes Spatiales, Université Paul Sabatier—Toulouse III, Toulouse, France
| | - M. Rojo
- grid.15781.3a0000 0001 0723 035XInstitut de Recherche en Astrophysique et Planétologie, Centre National de la Recherche Scientifique, Centre National d’Etudes Spatiales, Université Paul Sabatier—Toulouse III, Toulouse, France
| | - G. Murakami
- grid.62167.340000 0001 2220 7916Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Kyoto, Japan
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2
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Orsini S, Milillo A, Lichtenegger H, Varsani A, Barabash S, Livi S, De Angelis E, Alberti T, Laky G, Nilsson H, Phillips M, Aronica A, Kallio E, Wurz P, Olivieri A, Plainaki C, Slavin JA, Dandouras I, Raines JM, Benkhoff J, Zender J, Berthelier JJ, Dosa M, Ho GC, Killen RM, McKenna-Lawlor S, Torkar K, Vaisberg O, Allegrini F, Daglis IA, Dong C, Escoubet CP, Fatemi S, Fränz M, Ivanovski S, Krupp N, Lammer H, Leblanc F, Mangano V, Mura A, Rispoli R, Sarantos M, Smith HT, Wieser M, Camozzi F, Di Lellis AM, Fremuth G, Giner F, Gurnee R, Hayes J, Jeszenszky H, Trantham B, Balaz J, Baumjohann W, Cantatore M, Delcourt D, Delva M, Desai M, Fischer H, Galli A, Grande M, Holmström M, Horvath I, Hsieh KC, Jarvinen R, Johnson RE, Kazakov A, Kecskemety K, Krüger H, Kürbisch C, Leblanc F, Leichtfried M, Mangraviti E, Massetti S, Moissenko D, Moroni M, Noschese R, Nuccilli F, Paschalidis N, Ryno J, Seki K, Shestakov A, Shuvalov S, Sordini R, Stenbeck F, Svensson J, Szalai S, Szego K, Toublanc D, Vertolli N, Wallner R, Vorburger A. Inner southern magnetosphere observation of Mercury via SERENA ion sensors in BepiColombo mission. Nat Commun 2022; 13:7390. [PMID: 36450728 PMCID: PMC9712576 DOI: 10.1038/s41467-022-34988-x] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/24/2022] [Accepted: 11/14/2022] [Indexed: 12/03/2022] Open
Abstract
Mercury's southern inner magnetosphere is an unexplored region as it was not observed by earlier space missions. In October 2021, BepiColombo mission has passed through this region during its first Mercury flyby. Here, we describe the observations of SERENA ion sensors nearby and inside Mercury's magnetosphere. An intermittent high-energy signal, possibly due to an interplanetary magnetic flux rope, has been observed downstream Mercury, together with low energy solar wind. Low energy ions, possibly due to satellite outgassing, were detected outside the magnetosphere. The dayside magnetopause and bow-shock crossing were much closer to the planet than expected, signature of a highly eroded magnetosphere. Different ion populations have been observed inside the magnetosphere, like low latitude boundary layer at magnetopause inbound and partial ring current at dawn close to the planet. These observations are important for understanding the weak magnetosphere behavior so close to the Sun, revealing details never reached before.
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Affiliation(s)
- S Orsini
- Institute of Space Astrophysics and Planetology, INAF, Roma, Italy.
| | - A Milillo
- Institute of Space Astrophysics and Planetology, INAF, Roma, Italy
| | - H Lichtenegger
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - A Varsani
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - S Barabash
- Swedish Institute of Space Physics, Kiruna, Sweden
| | - S Livi
- Southwest Research Institute, San Antonio, TX, USA
- University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, USA
| | - E De Angelis
- Institute of Space Astrophysics and Planetology, INAF, Roma, Italy
| | - T Alberti
- Institute of Space Astrophysics and Planetology, INAF, Roma, Italy
| | - G Laky
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - H Nilsson
- Swedish Institute of Space Physics, Kiruna, Sweden
| | - M Phillips
- Southwest Research Institute, San Antonio, TX, USA
| | - A Aronica
- Institute of Space Astrophysics and Planetology, INAF, Roma, Italy
| | - E Kallio
- Aalto University, Department of Electronics and Nanoengineering, School of Electrical Engineering, Helsinki, Finland
| | - P Wurz
- University of Bern, Institute of Physics, Bern, Switzerland
| | | | | | - J A Slavin
- University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, USA
| | - I Dandouras
- Institut de Recherche en Astrophysique et Planétologie, CNRS, CNES, Université de Toulouse, Toulouse, France
| | - J M Raines
- University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, USA
| | | | - J Zender
- ESA-ESTEC, Noordwijk, The Netherlands
| | | | - M Dosa
- Wigner Research Centre for Physics, Budapest, Hungary
| | - G C Ho
- The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, 20723, USA
| | - R M Killen
- NASA/Goddard Space Flight Center, Greenbelt, MD, 20771, USA
| | | | - K Torkar
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - O Vaisberg
- IKI Space Research Institute, Moscow, Russia
| | - F Allegrini
- Southwest Research Institute, San Antonio, TX, USA
- University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, TX, USA
| | - I A Daglis
- National and Kapodistrian University of Athens, Department of Physics, Athens, Greece
- Hellenic Space Center, Athens, Greece
| | - C Dong
- Princeton Plasma Physics Laboratory and Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA
| | | | - S Fatemi
- Department of Physics, Umeå University, Umeå, Sweden
| | - M Fränz
- Max-Planck-Institut für Sonnensystemforschung, MPS, 37077, Göttingen, Germany
| | - S Ivanovski
- Astronomincal Observatory, INAF, Trieste, Italy
| | - N Krupp
- Max-Planck-Institut für Sonnensystemforschung, MPS, 37077, Göttingen, Germany
| | - H Lammer
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | | | - V Mangano
- Institute of Space Astrophysics and Planetology, INAF, Roma, Italy
| | - A Mura
- Institute of Space Astrophysics and Planetology, INAF, Roma, Italy
| | - R Rispoli
- Institute of Space Astrophysics and Planetology, INAF, Roma, Italy
| | - M Sarantos
- NASA/Goddard Space Flight Center, Greenbelt, MD, 20771, USA
| | - H T Smith
- The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, 20723, USA
| | - M Wieser
- Swedish Institute of Space Physics, Kiruna, Sweden
| | | | | | - G Fremuth
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - F Giner
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - R Gurnee
- Laboratory for Atmospheric and Space Physics, Boulder, CO, USA
| | - J Hayes
- The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, 20723, USA
| | - H Jeszenszky
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - B Trantham
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - J Balaz
- Institute of Experimental Physics SAS, Slovak Academy of Sciences, 040 01, Košice, Slovakia
| | - W Baumjohann
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | | | | | - M Delva
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - M Desai
- Southwest Research Institute, San Antonio, TX, USA
| | - H Fischer
- Max-Planck-Institut für Sonnensystemforschung, MPS, 37077, Göttingen, Germany
| | - A Galli
- University of Bern, Institute of Physics, Bern, Switzerland
| | - M Grande
- Aberystwyth University, Aberystwyth, Ceredigion, UK
| | - M Holmström
- Swedish Institute of Space Physics, Kiruna, Sweden
| | - I Horvath
- Wigner Research Centre for Physics, Budapest, Hungary
| | - K C Hsieh
- University of Arizona, Tucson, AZ, USA
| | - R Jarvinen
- Aalto University, Department of Electronics and Nanoengineering, School of Electrical Engineering, Helsinki, Finland
- Finnish Meteorological Institute FMI, Helsinki, Finland
| | - R E Johnson
- University of Virginia, Charlottesville, VA, 22904, USA
| | - A Kazakov
- Institute of Space Astrophysics and Planetology, INAF, Roma, Italy
| | - K Kecskemety
- Wigner Research Centre for Physics, Budapest, Hungary
| | - H Krüger
- Max-Planck-Institut für Sonnensystemforschung, MPS, 37077, Göttingen, Germany
| | - C Kürbisch
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | | | - M Leichtfried
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | | | - S Massetti
- Institute of Space Astrophysics and Planetology, INAF, Roma, Italy
| | - D Moissenko
- IKI Space Research Institute, Moscow, Russia
| | - M Moroni
- Institute of Space Astrophysics and Planetology, INAF, Roma, Italy
| | - R Noschese
- Institute of Space Astrophysics and Planetology, INAF, Roma, Italy
| | - F Nuccilli
- Institute of Space Astrophysics and Planetology, INAF, Roma, Italy
| | - N Paschalidis
- NASA/Goddard Space Flight Center, Greenbelt, MD, 20771, USA
| | - J Ryno
- Finnish Meteorological Institute FMI, Helsinki, Finland
| | - K Seki
- University of Tokyo, Department of Earth and Planetary Science, Graduate School of Science, Tokyo, Japan
| | - A Shestakov
- IKI Space Research Institute, Moscow, Russia
| | - S Shuvalov
- IKI Space Research Institute, Moscow, Russia
| | - R Sordini
- Institute of Space Astrophysics and Planetology, INAF, Roma, Italy
| | - F Stenbeck
- Swedish Institute of Space Physics, Kiruna, Sweden
| | - J Svensson
- Swedish Institute of Space Physics, Kiruna, Sweden
| | - S Szalai
- Wigner Research Centre for Physics, Budapest, Hungary
| | - K Szego
- Wigner Research Centre for Physics, Budapest, Hungary
| | - D Toublanc
- Institut de Recherche en Astrophysique et Planétologie, CNRS, CNES, Université de Toulouse, Toulouse, France
| | - N Vertolli
- Institute of Space Astrophysics and Planetology, INAF, Roma, Italy
| | - R Wallner
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - A Vorburger
- University of Bern, Institute of Physics, Bern, Switzerland
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3
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Orsini S, Livi SA, Lichtenegger H, Barabash S, Milillo A, De Angelis E, Phillips M, Laky G, Wieser M, Olivieri A, Plainaki C, Ho G, Killen RM, Slavin JA, Wurz P, Berthelier JJ, Dandouras I, Kallio E, McKenna-Lawlor S, Szalai S, Torkar K, Vaisberg O, Allegrini F, Daglis IA, Dong C, Escoubet CP, Fatemi S, Fränz M, Ivanovski S, Krupp N, Lammer H, Leblanc F, Mangano V, Mura A, Nilsson H, Raines JM, Rispoli R, Sarantos M, Smith HT, Szego K, Aronica A, Camozzi F, Di Lellis AM, Fremuth G, Giner F, Gurnee R, Hayes J, Jeszenszky H, Tominetti F, Trantham B, Balaz J, Baumjohann W, Brienza D, Bührke U, Bush MD, Cantatore M, Cibella S, Colasanti L, Cremonese G, Cremonesi L, D'Alessandro M, Delcourt D, Delva M, Desai M, Fama M, Ferris M, Fischer H, Gaggero A, Gamborino D, Garnier P, Gibson WC, Goldstein R, Grande M, Grishin V, Haggerty D, Holmström M, Horvath I, Hsieh KC, Jacques A, Johnson RE, Kazakov A, Kecskemety K, Krüger H, Kürbisch C, Lazzarotto F, Leblanc F, Leichtfried M, Leoni R, Loose A, Maschietti D, Massetti S, Mattioli F, Miller G, Moissenko D, Morbidini A, Noschese R, Nuccilli F, Nunez C, Paschalidis N, Persyn S, Piazza D, Oja M, Ryno J, Schmidt W, Scheer JA, Shestakov A, Shuvalov S, Seki K, Selci S, Smith K, Sordini R, Svensson J, Szalai L, Toublanc D, Urdiales C, Varsani A, Vertolli N, Wallner R, Wahlstroem P, Wilson P, Zampieri S. SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo. Space Sci Rev 2021; 217:11. [PMID: 33487762 PMCID: PMC7803725 DOI: 10.1007/s11214-020-00787-3] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 04/02/2020] [Accepted: 12/03/2020] [Indexed: 06/12/2023]
Abstract
The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at Mercury as well as their interactions with solar wind, solar radiation, and interplanetary dust. The particle instrument suite SERENA (Search for Exospheric Refilling and Emitted Natural Abundances) is flying in space on-board the BepiColombo Mercury Planetary Orbiter (MPO) and is the only instrument for ion and neutral particle detection aboard the MPO. It comprises four independent sensors: ELENA for neutral particle flow detection, Strofio for neutral gas detection, PICAM for planetary ions observations, and MIPA, mostly for solar wind ion measurements. SERENA is managed by a System Control Unit located inside the ELENA box. In the present paper the scientific goals of this suite are described, and then the four units are detailed, as well as their major features and calibration results. Finally, the SERENA operational activities are shown during the orbital path around Mercury, with also some reference to the activities planned during the long cruise phase.
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Affiliation(s)
- S Orsini
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | - S A Livi
- Southwest Research Institute, San Antonio, TX USA
- Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI USA
| | - H Lichtenegger
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - S Barabash
- Swedish Institute of Space Physics, Kiruna, Sweden
| | - A Milillo
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | - E De Angelis
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | - M Phillips
- Southwest Research Institute, San Antonio, TX USA
| | - G Laky
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - M Wieser
- Swedish Institute of Space Physics, Kiruna, Sweden
| | | | | | - G Ho
- The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723 USA
| | - R M Killen
- NASA/Goddard Space Flight Center, Greenbelt, MD 20771 USA
| | - J A Slavin
- Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI USA
| | - P Wurz
- Physics Institute, University of Bern, Bern, Switzerland
| | | | - I Dandouras
- Institut de Recherche en Astrophysique et Planétologie, CNRS, CNES, Université de Toulouse, Toulouse, France
| | - E Kallio
- School of Electrical Engineering, Department of Electronics and Nanoengineering, Aalto University, Helsinki, Finland
| | | | - S Szalai
- Wigner Research Centre for Physics, Budapest, Hungary
| | - K Torkar
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - O Vaisberg
- IKI Space Research Institute, Moscow, Russia
| | - F Allegrini
- Southwest Research Institute, San Antonio, TX USA
| | - I A Daglis
- Department of Physics, National and Kapodistrian University of Athens, Athens, Greece
- Hellenic Space Center, Athens, Greece
| | - C Dong
- Department of Astrophysical Sciences and Princeton Plasma Physics Laboratory, Princeton University, Princeton, NJ USA
| | | | - S Fatemi
- Swedish Institute of Space Physics, Kiruna, Sweden
| | - M Fränz
- Max-Planck-Institut für Sonnensystemforschung, MPS, 37077 Göttingen, Germany
| | - S Ivanovski
- Astronomical Observatory, INAF, Trieste, Italy
| | - N Krupp
- Max-Planck-Institut für Sonnensystemforschung, MPS, 37077 Göttingen, Germany
| | - H Lammer
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | | | - V Mangano
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | - A Mura
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | - H Nilsson
- Swedish Institute of Space Physics, Kiruna, Sweden
| | - J M Raines
- Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI USA
| | - R Rispoli
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | - M Sarantos
- NASA/Goddard Space Flight Center, Greenbelt, MD 20771 USA
| | - H T Smith
- The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723 USA
| | - K Szego
- Wigner Research Centre for Physics, Budapest, Hungary
| | - A Aronica
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | | | | | - G Fremuth
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - F Giner
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - R Gurnee
- Laboratory for Atmospheric and Space Physics, Boulder, CO USA
| | - J Hayes
- The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723 USA
| | - H Jeszenszky
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | | | - B Trantham
- Southwest Research Institute, San Antonio, TX USA
| | - J Balaz
- Institute of Experimental Physics SAS, Slovak Academy of Sciences, 040 01 Košice, Slovakia
| | - W Baumjohann
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - D Brienza
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | - U Bührke
- Max-Planck-Institut für Sonnensystemforschung, MPS, 37077 Göttingen, Germany
| | - M D Bush
- Physics Institute, University of Bern, Bern, Switzerland
| | | | - S Cibella
- Istituto di Struttura della Materia (CNR-ISM), 00133 Roma, Italy
| | - L Colasanti
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | - G Cremonese
- Astronomical Observatory, INAF, Padova, Italy
| | | | - M D'Alessandro
- Istituto di Struttura della Materia (CNR-ISM), 00133 Roma, Italy
| | | | - M Delva
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - M Desai
- Southwest Research Institute, San Antonio, TX USA
| | - M Fama
- Comisión Nacional de Energía Atómica, cnea, Centro Atómico Bariloche, Bariloche, Argentina
| | - M Ferris
- Southwest Research Institute, San Antonio, TX USA
| | - H Fischer
- Max-Planck-Institut für Sonnensystemforschung, MPS, 37077 Göttingen, Germany
| | - A Gaggero
- Istituto di Struttura della Materia (CNR-ISM), 00133 Roma, Italy
| | - D Gamborino
- Physics Institute, University of Bern, Bern, Switzerland
| | - P Garnier
- Institut de Recherche en Astrophysique et Planétologie, CNRS, CNES, Université de Toulouse, Toulouse, France
| | - W C Gibson
- Southwest Research Institute, San Antonio, TX USA
| | - R Goldstein
- Southwest Research Institute, San Antonio, TX USA
| | - M Grande
- Aberystwyth University, Aberystwyth, Ceredigion SY23 3FL UK
| | - V Grishin
- IKI Space Research Institute, Moscow, Russia
| | - D Haggerty
- The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723 USA
| | - M Holmström
- Swedish Institute of Space Physics, Kiruna, Sweden
| | - I Horvath
- Wigner Research Centre for Physics, Budapest, Hungary
| | - K-C Hsieh
- University of Arizona, Tucson, AZ USA
| | - A Jacques
- NASA/Goddard Space Flight Center, Greenbelt, MD 20771 USA
| | - R E Johnson
- University of Virginia, Charlottesville, VA 22904 USA
| | - A Kazakov
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | - K Kecskemety
- Wigner Research Centre for Physics, Budapest, Hungary
| | - H Krüger
- Max-Planck-Institut für Sonnensystemforschung, MPS, 37077 Göttingen, Germany
| | - C Kürbisch
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | | | | | - M Leichtfried
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | | | - A Loose
- Max-Planck-Institut für Sonnensystemforschung, MPS, 37077 Göttingen, Germany
| | - D Maschietti
- Istituto Fotonica e Nanotecnologie, CNR-IFN, Roma, Italy
| | - S Massetti
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | | | - G Miller
- Southwest Research Institute, San Antonio, TX USA
| | - D Moissenko
- IKI Space Research Institute, Moscow, Russia
| | - A Morbidini
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | - R Noschese
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | - F Nuccilli
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | - C Nunez
- Southwest Research Institute, San Antonio, TX USA
| | - N Paschalidis
- NASA/Goddard Space Flight Center, Greenbelt, MD 20771 USA
| | - S Persyn
- Southwest Research Institute, San Antonio, TX USA
| | - D Piazza
- Physics Institute, University of Bern, Bern, Switzerland
| | - M Oja
- Swedish Institute of Space Physics, Kiruna, Sweden
| | - J Ryno
- Finnish Meteorological Institute FMI, Helsinki, Finland
| | - W Schmidt
- Finnish Meteorological Institute FMI, Helsinki, Finland
| | | | - A Shestakov
- IKI Space Research Institute, Moscow, Russia
| | - S Shuvalov
- IKI Space Research Institute, Moscow, Russia
| | - K Seki
- Department of Earth and Planetary Science, Graduate School of Science, University of Tokyo, Tokyo, Japan
| | - S Selci
- Istituto di Struttura della Materia (CNR-ISM), 00133 Roma, Italy
| | - K Smith
- Southwest Research Institute, San Antonio, TX USA
| | - R Sordini
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | | | - L Szalai
- Wigner Research Centre for Physics, Budapest, Hungary
| | - D Toublanc
- Institut de Recherche en Astrophysique et Planétologie, CNRS, CNES, Université de Toulouse, Toulouse, France
| | - C Urdiales
- Southwest Research Institute, San Antonio, TX USA
| | - A Varsani
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - N Vertolli
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
| | - R Wallner
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - P Wahlstroem
- Physics Institute, University of Bern, Bern, Switzerland
| | - P Wilson
- Southwest Research Institute, San Antonio, TX USA
| | - S Zampieri
- Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy
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Han H, Hamilton E, Irie H, Isakoff S, Jelovac D, Liem A, Liu MC, Milillo A, Nangia J, Page D, Reeves J, Santa-Maria C, Duncan M, Graham JR, Chen J, Dezube BJ, Spring L. Abstract OT3-03-01: Open-label, single-arm study evaluating the antitumor activity and safety of niraparib as neoadjuvant treatment in patients with localized, HER2-negative, BRCA-mutant breast cancer. Cancer Res 2019. [DOI: 10.1158/1538-7445.sabcs18-ot3-03-01] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
Abstract
Abstract
Background: Neoadjuvant chemotherapy is administered to patients with operable breast cancer to downstage the tumor to allow for less extensive surgery and to provide prognostic information about drug efficacy and risk of disease recurrence. Patients who achieve a pathological complete response (pCR) following neoadjuvant treatment have a more favorable outcome than patients with residual invasive disease. Single-agent poly(ADP-ribose) polymerase (PARP) inhibitors have clinical efficacy in BRCA-mutated breast cancer. Niraparib, a potent and selective PARP1/2 inhibitor, is approved for maintenance treatment of patients with recurrent ovarian cancer and has demonstrated strong antitumor activity in in vivo studies with BRCA1-mutant breast cancer. The objective of this study is to evaluate the antitumor activity of single-agent niraparib in the neoadjuvant treatment of patients with localized, human epidermal growth factor receptor 2 (HER2)-negative, BRCAmut breast cancer.
Trial Design: This is an open-label, single-arm pilot study with a target enrollment of 20 evaluable patients. Eligible patients are those ≥18 years old with histologically-confirmed HER2-negative localized breast cancer and either a BRCA1 or BRCA2 mutation (germline or somatic) and no prior anti-cancer therapies for the current malignancy. Patients will receive 200 mg of oral niraparib once daily for 2 months, after which they may either proceed directly to surgery or receive chemotherapy at the discretion of the physician. The primary endpoint is tumor response rate based on the change in tumor volume as measured by breast MRI after 2 months of treatment with niraparib; a response is defined as ≥30% reduction of tumor volume from baseline. Secondary endpoints include pCR rate, tumor response rate based on the change in tumor volume as measured by breast ultrasound, and safety and tolerability. Data will be summarized in a descriptive nature by frequency distributions (number and percentage of patients) for categorical variables and by the mean, median, and standard deviation for continuous variables. Tumor response rate will be tabulated together with its 95% binomial exact confidence interval.
Funding: TESARO, Inc., Waltham, MA, USA sponsored the study.
Citation Format: Han H, Hamilton E, Irie H, Isakoff S, Jelovac D, Liem A, Liu MC, Milillo A, Nangia J, Page D, Reeves J, Santa-Maria C, Duncan M, Graham JR, Chen J, Dezube BJ, Spring L. Open-label, single-arm study evaluating the antitumor activity and safety of niraparib as neoadjuvant treatment in patients with localized, HER2-negative, BRCA-mutant breast cancer [abstract]. In: Proceedings of the 2018 San Antonio Breast Cancer Symposium; 2018 Dec 4-8; San Antonio, TX. Philadelphia (PA): AACR; Cancer Res 2019;79(4 Suppl):Abstract nr OT3-03-01.
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Affiliation(s)
- H Han
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - E Hamilton
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - H Irie
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - S Isakoff
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - D Jelovac
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - A Liem
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - MC Liu
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - A Milillo
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - J Nangia
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - D Page
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - J Reeves
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - C Santa-Maria
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - M Duncan
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - JR Graham
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - J Chen
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - BJ Dezube
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
| | - L Spring
- Moffitt Cancer Center-McKinley Outpatient Clinic, Tampa, FL; Tennessee Oncology, Nashville, TN; Icahn School of Medicine at Mount Sinai, New York, NY; Massachusetts General Hospital, Boston, MA; Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Baltimore, MD; Pacific Shores Medical Group, Long Beach, CA; Mayo Clinic Rochester, Rochester, MN; Memorial Health Care System, Hollywood, FL; Baylor College of Medicine, Houston, TX; Providence Portland Medical Center, Portland, OR; Florida Cancer Specialists-South, Fort Myers, FL; TESARO, Inc., Waltham, MA
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Castrellon AB, Velez M, Raez LE, Danenberg K, Rabizadeh S, Usher J, Jaimes Y, Hunis B, Bittencourt AC, Milillo A, Blaya M, Habaue C, Danenberg PV. Abstract P2-02-16: Use of cell-free circulating RNA and expression of PD-L1 and HER2 in plasma to monitor and predict clinical response in metastatic breast cancer patients. Cancer Res 2018. [DOI: 10.1158/1538-7445.sabcs17-p2-02-16] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
Abstract
Abstract
Background: In addition to traditional radiology tests, cell-free circulating tumor RNA (cfRNA) extracted from plasma of cancer patients (pts) provides a means of evaluating tumor response, but based on molecular changes in the tumor. Measuring dynamic changes in gene expression and levels of total cfRNA (per ml of plasma) in metastatic patients has shown great potential for evaluating disease status and predicting outcome to anti-tumoral therapy in advance of imaging. Though checkpoint inhibitors have not been assessed widely in breast cancer, TNBC has shown mild responses to pembrozilumab and atezolizumab, with significantly better responses in pts with detectable PD-L1 expression.
Methods: Blood was drawn from pts at approximately 6-week intervals under various therapies and CT scans were performed at approximately 3-month intervals. CfRNA was extracted from the resulting plasma and reverse transcribed with random hexamers to cDNA. Levels of cfRNA were quantitated by RT-qPCR and correlated with pt response (PR/SD/PD), as determined by CT scans. Levels of gene expression in cfRNA (including PD-L1 and HER2) were monitored in pts across blood draws.
Results: A total of 28 breast cancer pts were enrolled in a 1-year clinical study. Of pts, 39% (11/28) were Caucasian and 36% (10/28) Hispanic. 19 pts completed the first two cycles of therapy: 2 pts had PR and showed no change (NC) or decrease (DEC) in levels of cfRNA, 11 pts achieved SD with 8 showing DEC or NC in cfRNA levels, and 6 pts had PD and all underwent increases (INC) in cfRNA levels (median increase: 788 ng/mL plasma) which correlated with progressive disease status. Of pts with SD/PR, 4 showed either an emergence or significant increase in PD-L1 expression across blood draws (3.7-98 ct); of PD pts, 1 showed a significant emergence of PD-L1 expression (12.5 ct) across blood draws. 3/5 of these PD-L1 expressing pts were being treated with an everolimus combination; the emergence or increase of PD-L1 in response to this therapy suggests use of checkpoint inhibitors as an option for these pts. In response to therapy, 3 of 5 pts had PD-L1 cfRNA levels above levels predictive of response to nivolumab in lung cancer pts. In the only pt with hyperexpressed HER2, the disappearance of HER2 cfRNA matched positive response (PR) to treatment with trastuzumab. PD-L1 decreased concomitantly for this pt.
Conclusion: We found a strong correlation between clinical responses and changes in plasma levels of ctRNA in breast cancer (84%). Most of these were documented several weeks before imaging was done. Levels of PD-L1 and HER2 expression in plasma can also be used to monitor pt response to specific therapies. The emergence of PD-L1 expression in response to various therapies in breast cancer may confer sensitivity to checkpoint inhibitor therapy.
Citation Format: Castrellon AB, Velez M, Raez LE, Danenberg K, Rabizadeh S, Usher J, Jaimes Y, Hunis B, Bittencourt AC, Milillo A, Blaya M, Habaue C, Danenberg PV. Use of cell-free circulating RNA and expression of PD-L1 and HER2 in plasma to monitor and predict clinical response in metastatic breast cancer patients [abstract]. In: Proceedings of the 2017 San Antonio Breast Cancer Symposium; 2017 Dec 5-9; San Antonio, TX. Philadelphia (PA): AACR; Cancer Res 2018;78(4 Suppl):Abstract nr P2-02-16.
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Affiliation(s)
- AB Castrellon
- Memorial Cancer Institute, Hollywood, FL; Liquid Genomics, Inc., Culver City, CA; NantOmics, Culver City, CA; Keck School of Medicine of University of Southern California, Los Angeles, CA
| | - M Velez
- Memorial Cancer Institute, Hollywood, FL; Liquid Genomics, Inc., Culver City, CA; NantOmics, Culver City, CA; Keck School of Medicine of University of Southern California, Los Angeles, CA
| | - LE Raez
- Memorial Cancer Institute, Hollywood, FL; Liquid Genomics, Inc., Culver City, CA; NantOmics, Culver City, CA; Keck School of Medicine of University of Southern California, Los Angeles, CA
| | - K Danenberg
- Memorial Cancer Institute, Hollywood, FL; Liquid Genomics, Inc., Culver City, CA; NantOmics, Culver City, CA; Keck School of Medicine of University of Southern California, Los Angeles, CA
| | - S Rabizadeh
- Memorial Cancer Institute, Hollywood, FL; Liquid Genomics, Inc., Culver City, CA; NantOmics, Culver City, CA; Keck School of Medicine of University of Southern California, Los Angeles, CA
| | - J Usher
- Memorial Cancer Institute, Hollywood, FL; Liquid Genomics, Inc., Culver City, CA; NantOmics, Culver City, CA; Keck School of Medicine of University of Southern California, Los Angeles, CA
| | - Y Jaimes
- Memorial Cancer Institute, Hollywood, FL; Liquid Genomics, Inc., Culver City, CA; NantOmics, Culver City, CA; Keck School of Medicine of University of Southern California, Los Angeles, CA
| | - B Hunis
- Memorial Cancer Institute, Hollywood, FL; Liquid Genomics, Inc., Culver City, CA; NantOmics, Culver City, CA; Keck School of Medicine of University of Southern California, Los Angeles, CA
| | - AC Bittencourt
- Memorial Cancer Institute, Hollywood, FL; Liquid Genomics, Inc., Culver City, CA; NantOmics, Culver City, CA; Keck School of Medicine of University of Southern California, Los Angeles, CA
| | - A Milillo
- Memorial Cancer Institute, Hollywood, FL; Liquid Genomics, Inc., Culver City, CA; NantOmics, Culver City, CA; Keck School of Medicine of University of Southern California, Los Angeles, CA
| | - M Blaya
- Memorial Cancer Institute, Hollywood, FL; Liquid Genomics, Inc., Culver City, CA; NantOmics, Culver City, CA; Keck School of Medicine of University of Southern California, Los Angeles, CA
| | - C Habaue
- Memorial Cancer Institute, Hollywood, FL; Liquid Genomics, Inc., Culver City, CA; NantOmics, Culver City, CA; Keck School of Medicine of University of Southern California, Los Angeles, CA
| | - PV Danenberg
- Memorial Cancer Institute, Hollywood, FL; Liquid Genomics, Inc., Culver City, CA; NantOmics, Culver City, CA; Keck School of Medicine of University of Southern California, Los Angeles, CA
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Liverani A, Pezzatini M, Conte S, Mari F, Milillo A, Gasparrini M, Marino G, Catracchia V, -Favi F. A rare case of blunt thoracoabdominal trauma with small bowel perforation from air bags. G Chir 2009; 30:234-236. [PMID: 19505417] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 05/27/2023]
Abstract
Vehicle collisions represent more than 75% of mechanism of blunt abdominal trauma. In spite of the incomparable improvement of car safety devices, recent studies pointed out that the air bags might cause injuries, specially when it is not associated with seatbelt. In fact, some studies pointed out that crash victims using air bags alone have increased injury severity, hospitalisations, thoracoabdominal procedure, and rehabilitation. Some of the most frequently injured organs reported from air bag deployment are the liver (38%), the spleen (23%) and digestive system (17%). Injury of the hollow viscera are far less common. In particular, blunt abdominal trauma resulting in small bowel perforation is an infrequent lesion. These injuries are difficult to diagnose because specific signs are poor and a delay in treatment increases mortality and morbidity of the patients. We describe a case of thoracoabdominal trauma that occurred during a head-on collision after an air bag deployment without seatbelt use.
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Affiliation(s)
- A Liverani
- II School of Medicine, S. Andrea Hospital, Department of Surgery, "Sapienza", University of Rome, Italy
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Liverani A, Conte S, Marino G, Mari FS, Milillo A, Pezzatini M. [Non palpable testis in adult: laparoscopic treatment]. G Chir 2007; 28:344-6. [PMID: 17785051] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 05/17/2023]
Abstract
Cryptorchidism has an incidence of 0.8 - 2%, being undescendent testis nonpalpable in 20% of the cases. The latters have an increased risk of malignant transformation, infertility and epididymal malformation. Surgical treatment of nonpalpable testis is prone to failure compared to the palpable ones. Many diagnostic methods have been described; the most promising is the use of diagnostic laparoscopy which, compared to the imaging modalities, is more reliable to determine the site of the nonpalpable testis.
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Affiliation(s)
- A Liverani
- Universitá degli Studi di Roma La Sapienza, Seconda Facoltá di Medicina e Chirurgia
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Papaspyropoulos V, Midiri G, Tucci G, Milillo A, Montana C, Angelini L. [Surgical education: from teledidactics to virtual training]. G Chir 2007; 28:281-5. [PMID: 17626774] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 05/16/2023]
Abstract
The assessment of efficacy and quality of computer-assisted learning is today under evaluation. The Authors propose to use distant learning in the surgical knowledge teaching. In Italy, thanks to the Ministry of University and Scientific Research, a Master on distant learning in Medicine is now starting in 11 Italian Universities under the coordination of the second Faculty of Medicine of the University of Rome 'La Sapienza'. Thanks to the help of medicine and surgery teachers and informatics and telecommunication engineers, this Master is a first step to form and to license medical and surgical specialists experts in distant learning and videoconferencing telemedicine. Videoconferencing system can support Telementoring. Telementoring isn't an exclusive methodology but it is an additional methodology to tradictional didactic for clinicians and surgeons. It allows personal virtual trainings using computers and telecommunication systems.
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Affiliation(s)
- V Papaspyropoulos
- Università degli Studi di Roma La Sapienza, Il Facoltà di Medicina e Chirurgia, Dipartimento di Chirurgia, Italy
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Salvi PF, Midiri G, Tucci G, Lombardi A, Coppola M, Conte S, Marino G, Milillo A, Montana C, Pezzatini M. [Rhomboid flap in radical surgical treatment of sacrococcygeal fistulas: technical notes]. G Chir 2006; 27:335-8. [PMID: 17064496] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 05/12/2023]
Abstract
The Authors report their experience in surgical management of sacrococcygeal fistulas treated by radical excision and subcutaneous/cutaneous rhomboid flap. This is a simple, safe surgical technique and the patients can be treated in day surgery by spinal anesthesia.
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Affiliation(s)
- P F Salvi
- Università degli Studi di Roma "La Sapienza" II Facoltà di Medicina e Chirurgia Dipartmento di Chirurgia Generale, Italy
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10
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Lundin R, Barabash S, Andersson H, Holmström M, Grigoriev A, Yamauchi M, Sauvaud JA, Fedorov A, Budnik E, Thocaven JJ, Winningham D, Frahm R, Scherrer J, Sharber J, Asamura K, Hayakawa H, Coates A, Linder DR, Curtis C, Hsieh KC, Sandel BR, Grande M, Carter M, Reading DH, Koskinen H, Kallio E, Riihela P, Schmidt W, Säles T, Kozyra J, Krupp N, Woch J, Luhmann J, McKenna-Lawler S, Cerulli-Irelli R, Orsini S, Maggi M, Mura A, Milillo A, Roelof E, Williams D, Livi S, Brandt P, Wurz P, Bochsler P. Solar Wind-Induced Atmospheric Erosion at Mars: First Results from ASPERA-3 on Mars Express. Science 2004; 305:1933-6. [PMID: 15448263 DOI: 10.1126/science.1101860] [Citation(s) in RCA: 183] [Impact Index Per Article: 9.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
The Analyzer of Space Plasma and Energetic Atoms (ASPERA) on board the Mars Express spacecraft found that solar wind plasma and accelerated ionospheric ions may be observed all the way down to the Mars Express pericenter of 270 kilometers above the dayside planetary surface. This is very deep in the ionosphere, implying direct exposure of the martian topside atmosphere to solar wind plasma forcing. The low-altitude penetration of solar wind plasma and the energization of ionospheric plasma may be due to solar wind irregularities or perturbations, to magnetic anomalies at Mars, or both.
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Affiliation(s)
- R. Lundin
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - S. Barabash
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - H. Andersson
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - M. Holmström
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - A. Grigoriev
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - M. Yamauchi
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - J.-A. Sauvaud
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - A. Fedorov
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - E. Budnik
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - J.-J. Thocaven
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - D. Winningham
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - R. Frahm
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - J. Scherrer
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - J. Sharber
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - K. Asamura
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - H. Hayakawa
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - A. Coates
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - D. R. Linder
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - C. Curtis
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - K. C. Hsieh
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - B. R. Sandel
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - M. Grande
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - M. Carter
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - D. H. Reading
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - H. Koskinen
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - E. Kallio
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - P. Riihela
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - W. Schmidt
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - T. Säles
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - J. Kozyra
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - N. Krupp
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - J. Woch
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - J. Luhmann
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - S. McKenna-Lawler
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - R. Cerulli-Irelli
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - S. Orsini
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - M. Maggi
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - A. Mura
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - A. Milillo
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - E. Roelof
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - D. Williams
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - S. Livi
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - P. Brandt
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - P. Wurz
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
| | - P. Bochsler
- Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden
- Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France
- Southwest Research Institute, San Antonio, TX 78228–0510, USA
- Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan
- Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
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Milillo A, Orsini S, Daglis IA, Bellucci G. Low-altitude energetic neutral atoms imaging of the inner magnetosphere: A geometrical method to identify the energetic neutral atoms contributions from different magnetospheric regions. ACTA ACUST UNITED AC 1996. [DOI: 10.1029/96ja01560] [Citation(s) in RCA: 13] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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