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Wadsworth JDF, Joiner S, Linehan JM, Jack K, Al-Doujaily H, Costa H, Ingold T, Taema M, Zhang F, Sandberg MK, Brandner S, Tran L, Vikøren T, Våge J, Madslien K, Ytrehus B, Benestad SL, Asante EA, Collinge J. Humanized Transgenic Mice Are Resistant to Chronic Wasting Disease Prions From Norwegian Reindeer and Moose. J Infect Dis 2022; 226:933-937. [PMID: 33502474 PMCID: PMC9470110 DOI: 10.1093/infdis/jiab033] [Citation(s) in RCA: 11] [Impact Index Per Article: 5.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/01/2020] [Accepted: 01/19/2021] [Indexed: 01/08/2023] Open
Abstract
Chronic wasting disease (CWD) is the transmissible spongiform encephalopathy or prion disease affecting cervids. In 2016, the first cases of CWD were reported in Europe in Norwegian wild reindeer and moose. The origin and zoonotic potential of these new prion isolates remain unknown. In this study to investigate zoonotic potential we inoculated brain tissue from CWD-infected Norwegian reindeer and moose into transgenic mice overexpressing human prion protein. After prolonged postinoculation survival periods no evidence for prion transmission was seen, suggesting that the zoonotic potential of these isolates is low.
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Affiliation(s)
- Jonathan D F Wadsworth
- Medical Research Council Prion Unit at University College London, University College London Institute of Prion Diseases, London, United Kingdom
| | - Susan Joiner
- Medical Research Council Prion Unit at University College London, University College London Institute of Prion Diseases, London, United Kingdom
| | - Jacqueline M Linehan
- Medical Research Council Prion Unit at University College London, University College London Institute of Prion Diseases, London, United Kingdom
| | - Kezia Jack
- Medical Research Council Prion Unit at University College London, University College London Institute of Prion Diseases, London, United Kingdom
| | - Huda Al-Doujaily
- Medical Research Council Prion Unit at University College London, University College London Institute of Prion Diseases, London, United Kingdom
| | - Helena Costa
- Medical Research Council Prion Unit at University College London, University College London Institute of Prion Diseases, London, United Kingdom
| | - Thea Ingold
- Medical Research Council Prion Unit at University College London, University College London Institute of Prion Diseases, London, United Kingdom
| | - Maged Taema
- Medical Research Council Prion Unit at University College London, University College London Institute of Prion Diseases, London, United Kingdom
| | - Fuquan Zhang
- Medical Research Council Prion Unit at University College London, University College London Institute of Prion Diseases, London, United Kingdom
| | - Malin K Sandberg
- Medical Research Council Prion Unit at University College London, University College London Institute of Prion Diseases, London, United Kingdom
| | - Sebastian Brandner
- Medical Research Council Prion Unit at University College London, University College London Institute of Prion Diseases, London, United Kingdom
- Department of Neurodegenerative Disease, University College London Queen Square Institute of Neurology and Division of Neuropathology, National Hospital for Neurology and Neurosurgery, University College London National Health Service Foundation Trust, London, United Kingdom
| | - Linh Tran
- Norwegian Veterinary Institute, Oslo, Norway
| | | | - Jørn Våge
- Norwegian Veterinary Institute, Oslo, Norway
| | | | | | | | - Emmanuel A Asante
- Medical Research Council Prion Unit at University College London, University College London Institute of Prion Diseases, London, United Kingdom
| | - John Collinge
- Medical Research Council Prion Unit at University College London, University College London Institute of Prion Diseases, London, United Kingdom
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Ingold T, Mätzler C, Kämpfer N, Heimo A. Aerosol optical depth measurements by means of a Sun photometer network in Switzerland. ACTA ACUST UNITED AC 2001. [DOI: 10.1029/2000jd000088] [Citation(s) in RCA: 18] [Impact Index Per Article: 0.8] [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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Schmid B, Michalsky JJ, Slater DW, Barnard JC, Halthore RN, Liljegren JC, Holben BN, Eck TF, Livingston JM, Russell PB, Ingold T, Slutsker I. Comparison of columnar water-vapor measurements from solar transmittance methods. Appl Opt 2001; 40:1886-1896. [PMID: 18357188 DOI: 10.1364/ao.40.001886] [Citation(s) in RCA: 29] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/26/2023]
Abstract
In the fall of 1997 the Atmospheric Radiation Measurement program conducted a study of water-vapor-abundance-measurement at its southern Great Plains site. The large number of instruments included four solar radiometers to measure the columnar water vapor (CWV) by measuring solar transmittance in the 0.94-mum water-vapor absorption band. At first, no attempt was made to standardize our procedures to the same radiative transfer model and its underlying water-vapor spectroscopy. In the second round of comparison we used the same line-by-line code (which includes recently corrected H(2)O spectroscopy) to retrieve CWV from all four solar radiometers, thus decreasing the mean CWV by 8-13%. The remaining spread of 8% is an indication of the other-than-model uncertainties involved in the retrieval.
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Ingold T, Mätzler C, Wehrli C, Heimo A, Kämpfer N, Philipona R. Ozone column density determination from direct irradiance measurements in the ultraviolet performed by a four-channel precision filter radiometer. Appl Opt 2001; 40:1989-2003. [PMID: 18357202 DOI: 10.1364/ao.40.001989] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/26/2023]
Abstract
Ultraviolet light was measured at four channels (305, 311, 318, and 332 nm) with a precision filter radiometer (UV-PFR) at Arosa, Switzerland (46.78 degrees , 9.68 degrees , 1850 m above sea level), within the instrument trial phase of a cooperative venture of the Swiss Meteorological Institute (MeteoSwiss) and the Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center. We retrieved ozone-column density data from these direct relative irradiance measurements by adapting the Dobson standard method for all possible single-difference wavelength pairs and one double-difference pair (305/311 and 305/318) under conditions of cloud-free sky and of thin clouds (cloud optical depth <2.5 at 500 nm). All UV-PFR retrievals exhibited excellent agreement with those of collocated Dobson and Brewer spectrophotometers for data obtained during two months in 1999. Combining the results of the error analysis and the findings of the validation, we propose to retrieve ozone-column density by using the 305/311 single difference pair and the double-difference pair. Furthermore, combining both retrievals by building the ratio of ozone-column density yields information that is relevant to data quality control. Estimates of the 305/311 pair agree with measurements by the Dobson and Brewer instruments within 1% for both the mean and the standard deviation of the differences. For the double pair these values are in a range up to 1.6%. However, this pair is less sensitive to model errors. The retrieval performance is also consistent with satellite-based data from the Earth Probe Total Ozone Mapping Spectrometer (EP-TOMS) and the Global Ozone Monitoring Experiment instrument (GOME).
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Ingold T, Schmid B, Mätzler C, Demoulin P, Kämpfer N. Modeled and empirical approaches for retrieving columnar water vapor from solar transmittance measurements in the 0.72, 0.82, and 0.94 μm absorption bands. ACTA ACUST UNITED AC 2000. [DOI: 10.1029/2000jd900392] [Citation(s) in RCA: 40] [Impact Index Per Article: 1.7] [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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Schmid B, Spyak PR, Biggar SF, Wehrli C, Sekler J, Ingold T, Mätzler C, Kämpfer N. Evaluation of the Applicability of Solar and Lamp Radiometric Calibrations of a Precision Sun Photometer Operating Between 300 and 1025 nm. Appl Opt 1998; 37:3923-3941. [PMID: 18273360 DOI: 10.1364/ao.37.003923] [Citation(s) in RCA: 23] [Impact Index Per Article: 0.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/25/2023]
Abstract
Over a period of 3 years a precision Sun photometer (SPM) operating between 300 and 1025 nm was calibrated four times at three different high-mountain sites in Switzerland, Germany, and the United States by means of the Langley-plot technique. We found that for atmospheric window wavelengths the total error (2varsigma-statistical plus systematic errors) of the calibration constants V(0) (lambda), the SPM voltage in the absence of any attenuating atmosphere, can be kept below 1.6% in the UV-A and blue, 0.9% in the mid-visible, and 0.6% in the near-infrared spectral region. For SPM channels within strong water-vapor or ozone absorption bands a modified Langley-plot technique was used to determine V(0) (lambda) with a lower accuracy. Within the same period of time, we calibrated the SPM five times using irradiance standard lamps in the optical labs of the Physikalisch-Meteorologisches Observatorium Davos and World Radiation Center, Switzerland, and of the Remote Sensing Group of the Optical Sciences Center, University of Arizona, Tucson, Arizona. The lab calibration method requires knowledge of the extraterrestrial spectral irradiance. When we refer the standard lamp results to the World Radiation Center extraterrestrial solar irradiance spectrum, they agree with the Langley results within 2% at 6 of 13 SPM wavelengths. The largest disagreement (4.4%) is found for the channel centered at 610 nm. The results of these intercomparisons change significantly when the lamp results are referred to two different extraterrestrial solar irradiance spectra that have become recently available.
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