The Emirates Mars Ultraviolet Spectrometer (EMUS) for the EMM Mission

被引：0
|
作者：
Gregory M. Holsclaw
Justin Deighan
Hessa Almatroushi
Mike Chaffin
John Correira
J. Scott Evans
Matthew Fillingim
Alan Hoskins
Sonal K. Jain
Robert Lillis
Fatma Hussain Lootah
Jason B. McPhate
Oswald H. W. Siegmund
Regina Soufli
Kush Tyagi
机构：
[1] University of Colorado,Laboratory for Atmospheric and Space Physics
[2] Mohammed Bin Rashid Space Centre,Space Sciences Laboratory
[3] University of California,undefined
[4] Berkeley,undefined
[5] Lawrence Livermore National Laboratory,undefined
[6] Computational Physics Inc.,undefined
来源：
Space Science Reviews | 2021年 / 217卷
关键词：
Mars; Atmosphere; EMM; Hope; Spectrograph; Ultraviolet;
D O I：
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中图分类号：
学科分类号：
摘要：
The Emirates Mars Mission (EMM) Hope probe was launched on 20 July 2020 at 01:58 GST (Gulf Standard Time) and entered orbit around Mars on 9 Feb 2021 at 19:42 GST. The high-altitude orbit (19,970 km periapse, 42,650 km apoapse altitude, 25° inclination) with a 54.5 hour period enables a unique, synoptic, and nearly-continuous monitor of the Mars global climate. The Emirates Mars Ultraviolet Spectrometer (EMUS), one of three remote sensing instruments carried by Hope, is an imaging ultraviolet spectrograph, designed to investigate how conditions throughout the Mars atmosphere affect rates of atmospheric escape, and how key constituents in the exosphere behave temporally and spatially. EMUS will target two broad regions of the Mars upper atmosphere: 1) the thermosphere (100–200 km altitude), observing UV dayglow emissions from hydrogen (102.6, 121.6 nm), oxygen (130.4, 135.6 nm), and carbon monoxide (140–170 nm) and 2) the exosphere (above 200 km altitude), observing bound and escaping hydrogen (121.6 nm) and oxygen (130.4 nm).
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