Discrete aurora at Mars are characterized as localized, short‐lasting ultraviolet emissions on
the nightside. They are caused by the precipitation of accelerated electron along open …

In December 2022, an extremely low‐density solar wind stream encountered first the Earth
and then Mars, shortly after the radial alignment of the two planets (ie, Mars opposition). As …

Mars lacks a global magnetic field, and instead possesses small-scale crustal magnetic
fields, making its magnetic environment fundamentally different from intrinsic …

The current sheet is crucial in releasing magnetic free energy in cosmic plasmas via fast
magnetic reconnection or wave excitation. This research investigates the characteristics of …

We investigate Mars‐ward planetary ions (O+ and O2+) in the Martian magnetotail that
potentially reduce the amount of esca** ions. The global properties of Mars‐ward flows in …

We examine the newly discovered phenomena of sinuous aurora on the nightside of Mars,
using images of 130.4 and 135.6 nm oxygen emission measured by the Emirates Mars …

Abstract The Mars Atmosphere and Volatile EvolutioN (MAVEN) mission has been orbiting
Mars since 2014 and now has over 10,000 orbits which we use to characterize Mars' …

Knowing the properties of the Martian magnetotail flap** waves is critical to understand
the dynamics of the Martian induced magnetosphere. Based on the measurements by Mars …

When the solar wind interacts with the ionosphere of an unmagnetized planet, it induces
currents that form an induced magnetosphere. These currents and their associated magnetic …

Using measurements from the Mars Atmosphere and Volatile EvolutioN mission, we
investigate the densities of H+ (), O+ (), and O2+ (), respectively, in the Martian magnetotail …