Results 91 to 100 of about 68,935 (200)
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
Characterizing the current systems in the Martian ionosphere
When the solar wind encounters the ionosphere of an unmagnetized planet, it induces currents, forming an induced magnetosphere. These currents, along with their associated magnetic fields, play a crucial role in controlling the movement of charged particles, and are essential for understanding the escape of planetary ions.
Jiawei Gao +7 more
+5 more sources
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
Study on the Coupling between the Ionosphere and Thermosphere at Different Heights on Mars
Solar-driven thermal tides are an important factor driving spatiotemporal variations in the Martian upper atmosphere and ionosphere. Based on radio occultation data from the Mars Global Surveyor, this study systematically investigates the longitudinal ...
Yu Lou +3 more
doaj +1 more source
Magnetic flux ropes are twisted magnetic field lines that are commonly observed in space and astrophysical plasmas. At Mars, these structures are especially interesting because the planet does not have a global magnetic field like Earth, but instead has ...
Yuanzheng Wen +17 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
The anisotropy of suprathermal electrons in the Martian ionosphere
Suprathermal electrons are an important population of the Martian ionosphere, either produced by photoionization of atmospheric neutrals or supplied from the Solar Wind (SW). This study is dedicated to an in-depth investigation of the pitch angle distribution of suprathermal electrons at two representative energies, 19−55 eV and 124−356 eV, using the ...
YuTian Cao +5 more
openaire +2 more sources
Solar Flare Spotlights the Martian Ionosphere
A “lucky” linkup between orbiters helped scientists study how the Red Planet’s ionosphere responds to solar events.
openaire +1 more source
Detection of Martian ionosphere
Hong Zou +5 more
openaire +1 more source
Convergent Heavy-ion Plume from the Martian Ionosphere
Ion escape is a key consequence of the solar wind interaction with Mars, yet the three-dimensional structure of the heavy-ion plume, a major escape channel, remains poorly constrained.
Fuhao Qiao +12 more
doaj +1 more source

