The Emirates Mars Mission

The Emirates Mars Mission (EMM) was launched to Mars in the summer of 2020, and is the first interplanetary spacecraft mission undertaken by the United Arab Emirates (UAE). The mission has multiple programmatic and scientific objectives, including the return of scientifically useful information about Mars. Three science instruments on the mission's Hope Probe will make global remote sensing measurements of the Martian atmosphere from a large low-inclination orbit that will advance our understanding of atmospheric variability on daily and seasonal timescales, as well as vertical atmospheric transport and escape. The mission was conceived and developed rapidly starting in 2014, and had aggressive schedule and cost constraints that drove the design and implementation of a new spacecraft bus. A team of Emirati and American engineers worked across two continents to complete a fully functional and tested spacecraft and bring it to the launchpad in the middle of a global pandemic. EMM is being operated from the UAE and the United States (U.S.), and will make its data freely available.

The Space Physics Environment Data Analysis System (SPEDAS)

With the advent of the Heliophysics/Geospace System Observatory (H/GSO), a complement of multi-spacecraft missions and ground-based observatories to study the space environment, data retrieval, analysis, and visualization of space physics data can be daunting. The Space Physics Environment Data Analysis System (SPEDAS), a grass-roots software development platform (www.spedas.org), is now officially supported by NASA Heliophysics as part of its data environment infrastructure. It serves more than a dozen space missions and ground observatories and can integrate the full complement of past and upcoming space physics missions with minimal resources, following clear, simple, and well-proven guidelines. Free, modular and configurable to the needs of individual missions, it works in both command-line (ideal for experienced users) and Graphical User Interface (GUI) mode (reducing the learning curve for first-time users). Both options have "crib-sheets," user-command sequences in ASCII format that can facilitate record-and-repeat actions, especially for complex operations and plotting. Crib-sheets enhance scientific interactions, as users can move rapidly and accurately from exchanges of technical information on data processing to efficient discussions regarding data interpretation and science. SPEDAS can readily query and ingest all International Solar Terrestrial Physics (ISTP)-compatible products from the Space Physics Data Facility (SPDF), enabling access to a vast collection of historic and current mission data. The planned incorporation of Heliophysics Application Programmer's Interface (HAPI) standards will facilitate data ingestion from distributed datasets that adhere to these standards. Although SPEDAS is currently Interactive Data Language (IDL)-based (and interfaces to Java-based tools such as Autoplot), efforts are under-way to expand it further to work with python (first as an interface tool and potentially even receiving an under-the-hood replacement). We review the SPEDAS development history, goals, and current implementation. We explain its "modes of use" with examples geared for users and outline its technical implementation and requirements with software developers in mind. We also describe SPEDAS personnel and software management, interfaces with other organizations, resources and support structure available to the community, and future development plans.

ELECTRONIC SUPPLEMENTARY MATERIAL

The online version of this article (10.1007/s11214-018-0576-4) contains supplementary material, which is available to authorized users.

MAVEN observations of the response of Mars to an interplanetary coronal mass ejection

Coupling between the lower and upper atmosphere, combined with loss of gas from the upper atmosphere to space, likely contributed to the thin, cold, dry atmosphere of modern Mars. To help understand ongoing ion loss to space, the Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft made comprehensive measurements of the Mars upper atmosphere, ionosphere, and interactions with the Sun and solar wind during an interplanetary coronal mass ejection impact in March 2015. Responses include changes in the bow shock and magnetosheath, formation of widespread diffuse aurora, and enhancement of pick-up ions. Observations and models both show an enhancement in escape rate of ions to space during the event. Ion loss during solar events early in Mars history may have been a major contributor to the long-term evolution of the Mars atmosphere.

Early MAVEN Deep Dip campaign reveals thermosphere and ionosphere variability

The Mars Atmosphere and Volatile Evolution (MAVEN) mission, during the second of its Deep Dip campaigns, made comprehensive measurements of martian thermosphere and ionosphere composition, structure, and variability at altitudes down to ~130 kilometers in the subsolar region. This altitude range contains the diffusively separated upper atmosphere just above the well-mixed atmosphere, the layer of peak extreme ultraviolet heating and primary reservoir for atmospheric escape. In situ measurements of the upper atmosphere reveal previously unmeasured populations of neutral and charged particles, the homopause altitude at approximately 130 kilometers, and an unexpected level of variability both on an orbit-to-orbit basis and within individual orbits. These observations help constrain volatile escape processes controlled by thermosphere and ionosphere structure and variability.

Interactions of Escherichia coli endonuclease IV and exonuclease III with abasic sites in DNA

Duplex oligodeoxynucleotides with synthetic analogs of abasic sites were used to study the specificity of the abasic endonucleases of Escherichia coli. The apparent Km values of exonuclease III for the tetrahydrofuranyl, propanyl, and deoxyribosyl substrates varied only somewhat (20-140 nM) in either Mg2+ or Ca2+ and were similar to those for endonuclease IV. In Mg2+, exonuclease III had a turnover number 4-13-fold higher than measured for endonuclease IV (ranging 5.6-18 min-1), but was lowered in Ca2+ to values similar to those for endonuclease IV. The rate of cleavage of tetrahydrofuranyl (F) substrate by both enzymes was unaffected by the base in the opposite strand or its replacement by a tetrahydrofuranyl moiety. A C:C mismatch on the 5' but not the 3' side of F strongly inhibited cleavage by exonuclease III in Ca2+, while mismatches on both sides were required to diminish endonuclease IV cleavage significantly. A phosphorothioate ester linked 5' to the tetrahydrofuranyl moiety inhibited both enzymes, with the Rp stereoisomer most effective. Endonuclease IV bound stably to duplex substrates containing the Rp phosphorothioate in the presence of poly(dI-dC). Although the apurinic/apyrimidinic-cleaving activities of endonuclease IV and exonuclease III have some common features they also differ in their specific interactions with DNA containing abasic sites.

Intracellular localization of the Apn1 DNA repair enzyme of Saccharomyces cerevisiae. Nuclear transport signals and biological role

The Apn1 DNA repair enzyme of Saccharomyces cerevisiae acts on abasic sites and oxygen radical damages. Apn1 is homologous to the repair endonuclease IV of Escherichia coli, but the yeast protein is approximately 80 residues longer at the C terminus. The Apn1 C terminus is rich in basic amino acids and includes two lysine/arginine clusters related to the nuclear transport signals of some other proteins. We show here by indirect immunofluorescence that Apn1 is localized to the yeast nucleus. Mutant Apn1 proteins were engineered with progressive deletions inward from the C terminus. Elimination of just the last 12 residues from Apn1 (to yield Apn355) did not alter the stability in yeast cells or the in vitro activity of the enzyme. Greater truncation of Apn1 produced proteins of apparently lower (Apn334) or much lower (Apn315 and Apn293) in vivo stability. Both Apn355 and Apn334 failed to concentrate in the yeast nucleus and remained in the cytoplasm. These delocalized derivatives also failed to restore wild-type resistance to oxidative or alkylating agents in a delta apn1 strain. Apn355 and Apn334 complemented repair-deficient E. coli as effectively as did wild-type Apn1. Resistance to these DNA-damaging agents in yeast was restored if Apn355 and Apn334 (but not Apn315 or Apn293) were overproduced approximately 20-fold, which suggests either weak active transport or passive diffusion of these derivatives into the nucleus. Replacement of the C-terminal 12 residues of Apn1 with the nuclear targeting sequence of SV40 T-antigen did not restore effective function or nuclear localization in yeast.

Trophic regulation of nodose ganglion cell development: evidence for an expanded role of nerve growth factor during embryogenesis in the rat

Peripheral sensory neurons are derived from two distinct embryonic tissues, the neural crest and epibranchial placodes. Studies in the chick suggest that embryonic lineage and trophic dependence are interrelated, such that many crest-derived cells depend on NGF for survival during development, whereas placodal derivates, including nodose ganglion neurons, do not (30). It remains controversial, however, whether or not a similar dichotomy exists in mammalian species, in which trophic requirements during early development of placodal ganglia have not been defined. To approach this issue, the present study examined the effects of nerve growth factor (NGF) on neuronal survival in embryonic rat nodose ganglion cultures. Treatment of E13.5-14.5 nodose explants with 20 ng/ml NGF resulted in a four-fold increase in neuronal survival that was blocked by anti-NGF antiserum. Increased neuronal survival and neurite outgrowth were also observed in neuron-enriched dissociated cell cultures; these effects were seen within 12 h of plating, indicating that NGF-responsive neurons or neuroblasts were already present in the ganglion at the time of explantation. This was further supported by immunocytochemical staining of nodose cell bodies in situ with the monoclonal antibody 192-IgG against the NGF receptor (12). These findings indicate that NGF may be important in regulating nodose development during early gangliogenesis in mammals and suggest that NGF plays a more widespread role in peripheral nervous system ontogeny than previously recognized.