Morphology Of Euv And Fuv Martian Airglow Emissions Observed By The Emus Instrument On Board The Emirates Mars
Mission.
S. K. Jain, J. Deighan, M. S. Chaffin, G. H. Holsclaw, Laboratory For Atmospheric And Space Sciences,
University Of Colorado, Boulder, Co, United States, (Sonal.Jain@Lasp.Colorado.Edu), R. Lillis, M. Fillingim, Space
Sciences Laboratory, University Of California Berkeley, Berkeley, Ca, United States, J. S. Evans, J. Correira,
Computational Physics Inc., Springfield, Virginia, United States, H. Almatroushi, F. Lootah, Mohammed Bin Rashid
Space Center, Al Khawaneej, United Arab Emirates, S. England, Virginia Polytechnic Institute And State University,
Aerospace And Ocean Engineering, Blacks- Burg, Va, United States, H. Almazmi, Uae Space Agency, Abu Dhabi,
United Arab Emirates, E. M. B. Thiemann, F. Eparvier, P. Chamberlin, Laboratory For Atmospheric And Space
Sciences, University Of Colorado, Boulder, Co, United States.

Introduction
The Spectroscopy Of The Martian Atmosphere In Extreme
And Far-Ultraviolet Wavelengths Has Been Extensively Used
To Study Planetary Atmospheres. The Fuv And Euv
Emissions Provide Information About The Atmospheric
Composition (Both Neutral And Ionized) And Structure
And Can Be Used To Study Energy Deposition, Dynamics,
And Chemistry. The Emirates Mars Mission Ultraviolet
Spectrometer (Emm/Emus) Is The First Instrument Capable Of Simultaneously Observing The Euv And Fuv