Results 101 to 110 of about 475 (211)

In Situ Measurements of Thermal Ion Temperature in the Martian Ionosphere. [PDF]

J Geophys Res Space Phys, 2021
Hanley KG, McFadden JP, Mitchell DL, Fowler CM, Stone SW, Yelle RV, Mayyasi M, Ergun RE, Andersson L, Benna M, Elrod MK, Jakosky BM.   +11 more
europepmc   +1 more source

Thermal Variability in the Martian Upper Atmosphere within the Crustal Magnetic Field Region Induced by Gravity Wave Dissipation Due to Ion-drag Effect

The Astronomical Journal
Mars Atmosphere and Volatile Evolution detected a significant temperature increase of approximately 20–40 K in the upper atmosphere within the strong crustal magnetic field (CF) region during two deep dip campaigns.
Xing Wang, Xiaojun Xu, Jun Cui, Siqi Yi, Hao Gu, Zilu Zhou, Hengyan Man, Lei Luo, Peishan He, Pu Yang   +9 more
doaj   +1 more source

In Search of Subsurface Oceans Within the Uranian Moons. [PDF]

J Geophys Res Planets, 2021
Cochrane CJ, Vance SD, Nordheim TA, Styczinski MJ, Masters A, Regoli LH.   +5 more
europepmc   +1 more source

Revealing the CME Impact on the Martian Nightside Ionosphere Based on MAVEN and Tianwen-1 Observations

The Astrophysical Journal
Due to the absence of an Earth-like dipole magnetic field, the impact of coronal mass ejections (CMEs) on the Martian nightside ionosphere differs from that on Earth and is still not well understood.
Longhui Liu, Xinzhi Qiu, Yiqun Yu, Wudi Luo, Xin Wang, Jinbin Cao, Cunhui Li, YuMing Wang, TieLong Zhang   +8 more
doaj   +1 more source

A perturbation method for evaluating the magnetic field induced from an arbitrary, asymmetric ocean world analytically. [PDF]

Icarus, 2022
Styczinski MJ, Vance SD, Harnett EM, Cochrane CJ.   +3 more
europepmc   +1 more source

Carbon Ion Fluxes at Mars: First Results of Tailward Flows From MAVEN-STATIC. [PDF]

J Geophys Res Space Phys, 2022
Pickett NB, McFadden JP, Fowler CM, Hanley KG, Benna M.   +4 more
europepmc   +1 more source

Chaos gated tunneling drives molecular reactivity in astrophysical environments

Discover Space
Accurate modeling of ion-molecule reaction networks is essential for understanding the chemical evolution of planetary ionospheres, particularly for giant planets where proton-transfer chains drive atmospheric composition.
Saptarshi G. Dastider, K. Prashant, P. Shruti, C. Sudheesh, Jobin Cyriac   +4 more
doaj   +1 more source

Atmospheric Distribution and Escape of Odd Nitrogen on Mars

The Astronomical Journal
The total nitrogen budget in the Martian upper atmosphere is significantly contributed by the presence of odd nitrogen, mainly in the form of NO and ground-state or excited-state N.
Hao Gu, Xiaoshu Wu, Jun Cui, Xu Huang, Wenlong Li, Jinjin Zhao, Lei Li   +6 more
doaj   +1 more source

Magnetopause ripples going against the flow form azimuthally stationary surface waves. [PDF]

Nat Commun, 2021
Archer MO, Hartinger MD, Plaschke F, Southwood DJ, Rastaetter L.   +4 more
europepmc   +1 more source

Multi-Fluid MHD Simulations of Europa's Plasma Interaction: Effects of Variation in Europa's Atmosphere. [PDF]

J Geophys Res Space Phys, 2022
Harris CDK, Jia X, Slavin JA.
europepmc   +1 more source