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Showing 1 to 2 of 2 for “"IUVS"”.
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Non-migrating tides in the Martian thermosphere
… Mars. MAVEN’s Imaging Ultraviolet Spectrometer (IUVS) observations of the upper atmosphere reveal variations in density with longitude at altitudes of 130 – 200 km, and can be used to identify non-migrating tides. These observations cover higher latitudes and allow for studying the local time …
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Proton Aurora at Mars: Assessing the Characteristics, Variability, and Driving Mechanisms of a Newly Discovered Phenomenon
… using the Imaging UltraViolet Spectrograph (IUVS) onboard the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft. Martian proton aurora are observed in IUVS data as a prominent enhancement in the intensity of the hydrogen Lyman-alpha (Ly-α) emission (121.6 nm) between ~110-150 km …