Jets downstream of collisionless shocks
The magnetosheath flow may take the form of large amplitude, yet spatially localized,
transient increases in dynamic pressure, known as “magnetosheath jets” or “plasmoids” …
transient increases in dynamic pressure, known as “magnetosheath jets” or “plasmoids” …
Observations and impacts of the 10 September 2017 solar events at Mars: An overview and synthesis of the initial results
On 10 September 2017, some of the strongest solar activity occurred in association with
active region 12673 (AR2673), including an X‐class solar flare and a fast coronal mass …
active region 12673 (AR2673), including an X‐class solar flare and a fast coronal mass …
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 …
Seasonal variability of the hydrogen exosphere of Mars
JS Halekas - Journal of Geophysical Research: Planets, 2017 - Wiley Online Library
Abstract The Mars Atmosphere and Volatile EvolutioN (MAVEN) mission measures both the
upstream solar wind and collisional products from energetic neutral hydrogen atoms that …
upstream solar wind and collisional products from energetic neutral hydrogen atoms that …
CME evolution in the structured heliosphere and effects at Earth and Mars during solar minimum
The activity of the Sun alternates between a solar minimum and a solar maximum, the former
corresponding to a period of “quieter” status of the heliosphere. During solar minimum, it is …
corresponding to a period of “quieter” status of the heliosphere. During solar minimum, it is …
Statistical properties of solar wind upstream of Mars: MAVEN observations
Using the data sets of Mars Atmosphere and Volatile EvolutioN and OMNI for the period
2014 October 10–2020 February 14 and the heliocentric distance of 1–1.66 au, we …
2014 October 10–2020 February 14 and the heliocentric distance of 1–1.66 au, we …
The twisted configuration of the Martian magnetotail: MAVEN observations
Measurements provided by the Mars Atmosphere and Volatile EvolutioN (MAVEN)
spacecraft are analyzed to investigate the Martian magnetotail configuration as a function of …
spacecraft are analyzed to investigate the Martian magnetotail configuration as a function of …
Three‐dimensional configuration of induced magnetic fields around Mars
Using over 6 years of magnetic field data (October 2014–December 2020) collected by the
Mars Atmosphere and Volatile EvolutioN, we conduct a statistical study on the three …
Mars Atmosphere and Volatile EvolutioN, we conduct a statistical study on the three …
Flows, fields, and forces in the Mars‐solar wind interaction
We utilize suprathermal ion and magnetic field measurements from the Mars Atmosphere
and Volatile EvolutioN (MAVEN) mission, organized by the upstream magnetic field, to …
and Volatile EvolutioN (MAVEN) mission, organized by the upstream magnetic field, to …
A technique to infer magnetic topology at Mars and its application to the terminator region
Magnetic topology is important for understanding the Martian plasma environment, including
particle precipitation, energy transport, cold ion escape, and wave‐particle interaction. In this …
particle precipitation, energy transport, cold ion escape, and wave‐particle interaction. In this …