73 citations · 163 across the 7 of their papers we have counts for
7 papers
Interplanetary Coronal Mass Ejections and Stream Interaction Regions observed by Tianwen-1 and Maven at Mars
Yutian Chi, Chenglong Shen, Long Cheng +22
Tianwen-1 spacecraft (Wan et al. 2020) is China's first Mars exploration mission. The Mars Orbiter Magnetometer (MOMAG) is a scientific instrument aboard the Tianwen-1 mission that…
In-flight Calibration of the Magnetometer on the Mars Orbiter of Tianwen-1
Zhuxuan Zou, Yuming Wang, Tielong Zhang +17
Mars Orbiter Magnetometer (MOMAG) is one of seven science payloads onboard Tianwen-1's orbiter. Unlike most of the satellites, Tianwen-1's orbiter is not magnetically cleaned, and…
The Mars Orbiter Magnetometer of Tianwen-1: In-flight Performance and First Science Results
Yuming Wang, Tielong Zhang, Guoqiang Wang +17
Mars Orbiter MAGnetometer (MOMAG) is a scientifc instrument onboard the orbiter of China's first mission for Mars -- Tianwen-1. It started to routinely measure the magnetic field f…
Spatially high-resolved solar-wind-induced magnetic field on Venus
Maosheng He, Joachim Vogt, Eduard Dubinin +2
The current work investigates the Venusian solar-wind-induced magnetosphere at a high spatial resolution using all Venus Express (VEX) magnetic observations through an unbiased sta…
Understanding the twist distribution inside magnetic flux ropes by anatomizing an interplanetary magnetic cloud
Yuming Wang, Chenglong Shen, Rui Liu +6
Magnetic flux rope (MFR) is the core structure of the greatest eruptions, i.e., the coronal mass ejections (CMEs), on the Sun, and magnetic clouds are post-eruption MFRs in interpl…
Solar wind turbulence at 0.72 AU and solar minimum
Eliza Teodorescu, Marius Echim, Costel Munteanu +3
We investigate Venus Express (VEX) observations of magnetic field fluctuations performed systematically in the solar wind at 0.72 Astronomical Units (AU), between 2007 and 2009, du…
Morphological evolution of a 3D CME cloud reconstructed from three viewpoints
L. Feng, B. Inhester, Y. Wei +3
The propagation properties of coronal mass ejections (CMEs) are crucial to predict its geomagnetic effect. A newly developed three dimensional (3D) mask fitting reconstruction meth…