In Situ Measurements of Thermal Ion Temperature in the Martian Ionosphere. [PDF]
Hanley KG +11 more
europepmc +1 more source
C+ 133.5 nm Emission Mechanisms on Mars Revealed by the MAVEN Observations
C ^+ emission is generated by electron impact, dissociative ionization, photoionization, and resonant scattering with carbon-related atoms, molecules, and ions in the Martian ionosphere and thermosphere. The contribution of each mechanism to the emission,
Shotaro Sakai +15 more
doaj +1 more source
Joint Observation of a Rotational Discontinuity by Tianwen‐1 and MAVEN at Mars
The solar wind plays a crucial role in the evolution of planets in the solar system, particularly Mars. Mars has no global intrinsic magnetic field, leading the solar wind to interact directly with the Martian ionosphere and atmosphere.
Z. Z. Guo +8 more
doaj +1 more source
Recent progress in understanding magnetic reconnection in the Martian space environment
Magnetic reconnection, a ubiquitous plasma process in the universe, serves as a key mechanism for explosive energy release in various astrophysical phenomena.
Xiaojun Xu +6 more
doaj +1 more source
Spatial Scales of Electron Density Fluctuations in the Martian Ionosphere
In recent Martian ionospheric studies, the spatial scales of electron density irregularities have been computed using magnetic field measurements by treating these fluctuations as electromagnetic.
Chougule Prathmesh +2 more
doaj +1 more source
Detection of magnetospheric ion drift patterns at Mars. [PDF]
Zhang C +22 more
europepmc +1 more source
Upstream IMF Influence on Closed Magnetic Field Orientation on Mars
Closed magnetic fields play an important role in plasma transport and atmospheric escape from the Martian dayside ionosphere. Leveraging in‐situ magnetic field data from the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission, we conduct a statistical
JunFeng Qin +5 more
doaj +1 more source
Mars' plasma system. Scientific potential of coordinated multipoint missions: "The next generation". [PDF]
Sánchez-Cano B +29 more
europepmc +1 more source
Sporadic E-like Topside Layer Driven by Wind Shear in the Martian Ionosphere
Ionospheric plasma density disturbances significantly affect radio wave propagation, impacting communication and planetary exploration. At Earth, sporadic E layers (Es) are commonly observed. They are characterized by thin, high-density plasma structures
Rong Tian +10 more
doaj +1 more source
Atmospheric Distribution and Escape of Odd Nitrogen on Mars
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 +6 more
doaj +1 more source

