Browsing by Author "Fillingim, Matt"

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    Combined Analysis of Hydrogen and Oxygen 102.6 nm Emission at Mars
    Chaffin, Michael S.; Deighan, Justin; Jain, Sonal; Holsclaw, Greg; AlMazmi, Hoor; Chirakkil, Krishnaprasad; Correira, John; England, Scott L.; Evans, J. Scott; Fillingim, Matt; Lillis, Rob; Lootah, Fatma; Raghuram, Susarla; Eparvier, Frank; Thiemann, Ed; Curry, Shannon; AlMatroushi, Hessa (American Geophysical Union, 2022-08)
    Water is lost from the Mars upper atmosphere to space as hydrogen and oxygen, both of which can be observed in scattered ultraviolet sunlight at 102.6 nm. We present Emirates Mars Mission Emirates Mars Ultraviolet Spectrometer (EMM/EMUS) insertion orbit observations of this airglow, resolving the independent altitude contributions of H and O for the first time. We present the first airglow modeling of the complete H and O 102.6 nm system and the first 3D azimuthally symmetric modeling of the O emission, retrieving temperatures and densities typical of northern spring. Our model reproduces the emission well above 200 km, but does not incorporate partial frequency redistribution needed to reproduce the observed O brightness at lower altitudes and on the disk. These results support future EMM/EMUS science orbit retrievals of H loss and the use of 102.6 nm observations to constrain planetary atmospheres across the solar system.
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    Morphology of Extreme and Far Ultraviolet Martian Airglow Emissions Observed by the EMUS Instrument on Board the Emirates Mars Mission
    Jain, Sonal K.; Deighan, Justin; Chaffin, Mike; Holsclaw, Greg; Lillis, Rob; Fillingim, Matt; Evans, J. Scott; Correira, John; AlMatroushi, Hessa; Lootah, Fatma; England, Scott L.; AlMazmi, Hoor; Thiemann, Ed; Chamberlin, Phil; Eparvier, Frank (American Geophysical Union, 2022-10)
    We present the first continuous observations of the extreme and far ultraviolet (EUV and FUV) dayglow emissions measured by Emirates Mars Ultraviolet Spectrometer (EMUS) onboard the Emirates Mars Mission. We found excellent agreement between the previous observations from the Hopkins Ultraviolet Telescope and recent observations by EMUS both in shape and magnitude. We presented the average disk brightness of major EUV and FUV emissions for about 10 months of data from April 2021 to February 2022. The solar activity was mild/minimum during the first half of the period presented in this study, but we noticed significant day-to-day variations in the major dayglow emissions independent of solar activity, indicating possible coupling from the lower atmosphere via waves/tides. The solar activity increased significantly during the second half of the study period. Our analysis showed that all major EUV and FUV emissions are highly correlated with solar forcing as well as seasonal changes.