Results 141 to 150 of about 6,063 (251)

Escape of hydrogen from the exosphere of Mars [PDF]

open access: yes, 2016
After decades of exploration, the martian neutral hydrogen exosphere has remained poorly characterized. The first measurements of this layer by Mariner 6 and 7 revealed it to be optically thick in Lyman α emission, along with a characteristic temperature
Bhattacharyya, Dolon
core  

Lyα Emissions from Titan’s Atmosphere and Exosphere

open access: yesThe Planetary Science Journal
From 2004 to 2017, the Cassini/UVIS instrument observed Titan’s Ly α airglow from Titan’s atmosphere and exosphere, helping to characterize Titan’s H population. Most Ly α observations remain unanalyzed. Using data from the T10 Titan flyby, we analyze Ly
Devin Hoover   +5 more
doaj   +1 more source

MESSENGER Observations of Planetary Ion Enhancements at Mercury's Northern Magnetospheric Cusp During Flux Transfer Event Showers. [PDF]

open access: yesJ Geophys Res Space Phys, 2022
Sun W   +13 more
europepmc   +1 more source

Far-ultraviolet Flares and Variability of the Young M Dwarf AU Mic: A Nondetection of Planet C in Transit at Lyα

open access: yesThe Astronomical Journal
Atmospheric escape’s potential to shape the exoplanet population motivates detailed observations of systems actively undergoing escape. AU Mic is a young and active M dwarf hosting two close-in transiting sub- to Neptune-sized planets. Atmospheric escape
Keighley E. Rockcliffe   +10 more
doaj   +1 more source

Soft X-ray and ENA Imaging of the Earth's Dayside Magnetosphere. [PDF]

open access: yesJ Geophys Res Space Phys, 2021
Connor HK   +18 more
europepmc   +1 more source

Mercury at the Dawn of a New Exploration Phase. [PDF]

open access: yesNat Commun
Del Vecchio E   +2 more
europepmc   +1 more source

Energetic electron irradiations of amorphous and crystalline sulphur-bearing astrochemical ices. [PDF]

open access: yesFront Chem, 2022
Mifsud DV   +12 more
europepmc   +1 more source

Exospheric Temperature of Venus

open access: yesExospheric Temperature of Venus
The local time dependence of the Cytherean exospheric temperature in the instantaneous heating rate model is calculated by solving the heat conduction equation. It is found that the differential heating by the solar ultraviolet radiation produces steep temperature gradients near terminator, mainly due to the low exospheric temperatures at the night ...
openaire  

SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo. [PDF]

open access: yesSpace Sci Rev, 2021
Orsini S   +120 more
europepmc   +1 more source

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