The emirates Mars mission
HES Amiri, D Brain, O Sharaf, P Withnell… - Space Science …, 2022 - Springer
Abstract 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 …
and is the first interplanetary spacecraft mission undertaken by the United Arab Emirates …
Emirates Mars mission characterization of Mars atmosphere dynamics and processes
H Almatroushi, H AlMazmi, N AlMheiri… - Space Science …, 2021 - Springer
Abstract The Emirates Mars Mission (EMM)–Hope Probe–was developed to understand
Mars atmospheric circulation, dynamics, and processes through characterization of the Mars …
Mars atmospheric circulation, dynamics, and processes through characterization of the Mars …
Martian water loss to space enhanced by regional dust storms
Mars has lost most of its initial water to space as atomic hydrogen and oxygen. Spacecraft
measurements have determined that present-day hydrogen escape undergoes large …
measurements have determined that present-day hydrogen escape undergoes large …
Loss of the Martian atmosphere to space: Present-day loss rates determined from MAVEN observations and integrated loss through time
Observations of the Mars upper atmosphere made from the Mars Atmosphere and Volatile
Evolution (MAVEN) spacecraft have been used to determine the loss rates of gas from the …
Evolution (MAVEN) spacecraft have been used to determine the loss rates of gas from the …
Atmospheric escape processes and planetary atmospheric evolution
The habitability of the surface of any planet is determined by a complex evolution of its
interior, surface, and atmosphere. The electromagnetic and particle radiation of stars drive …
interior, surface, and atmosphere. The electromagnetic and particle radiation of stars drive …
The MAVEN EUVM model of solar spectral irradiance variability at Mars: Algorithms and results
Solar extreme ultraviolet (EUV) radiation is a primary energy input to the Mars atmosphere,
causing ionization and driving photochemical processes above approximately 100 km …
causing ionization and driving photochemical processes above approximately 100 km …
Initial results from the MAVEN mission to Mars
BM Jakosky, JM Grebowsky… - Geophysical …, 2015 - Wiley Online Library
Abstract The Mars Atmosphere and Volatile EvolutioN (MAVEN) Mars orbiter has been
gathering information on the Mars upper atmosphere, ionosphere, and solar and solar wind …
gathering information on the Mars upper atmosphere, ionosphere, and solar and solar wind …
Thermal structure of the Martian upper atmosphere from MAVEN NGIMS
Abstract The Neutral Gas and Ion Mass Spectrometer (NGIMS) aboard the NASA Mars
Atmosphere and Volatile EvolutioN (MAVEN) mission measures the structure and variability …
Atmosphere and Volatile EvolutioN (MAVEN) mission measures the structure and variability …
Photochemical escape of oxygen from Mars: First results from MAVEN in situ data
Photochemical escape of atomic oxygen is thought to be one of the dominant channels for
Martian atmospheric loss today and played a potentially major role in climate evolution …
Martian atmospheric loss today and played a potentially major role in climate evolution …
The emirates Mars ultraviolet spectrometer (EMUS) for the EMM mission
GM Holsclaw, J Deighan, H Almatroushi… - Space Science …, 2021 - Springer
Abstract 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 …
01: 58 GST (Gulf Standard Time) and entered orbit around Mars on 9 Feb 2021 at 19: 42 …