Search Publications

Working models for the gravitational field of Phobos
DOI: 10.1007/s11433-011-4606-4 Bibcode: 2012SCPMA..55..358S

Shi, Xian; Willner, Konrad; Oberst, Jürgen +2 more

Models for the gravitational field of Mars moon Phobos were developed using the latest shape model and assuming homogeneous density distribution. Three methods were applied in our study. Comparisons were made between these methods and all were shown to yield consistent results. Notably, the most accurate shape model of Phobos to date, complete up …

2012 Science China Physics, Mechanics, and Astronomy
MEx 18
H α counterparts of X-ray bright points in the solar atmosphere
DOI: 10.1007/s11433-012-4694-9 Bibcode: 2012SCPMA..55..907Z

Zhang, Ping; Fang, Cheng; Zhang, QingMin

X-ray bright points (XBPs) are small-scale brightenings in the solar corona. Their counterparts in the lower atmosphere, however, are poorly investigated. In this paper, we study the counterparts of XBPs in the upper chromosphere where the Hα line center is formed. The XBPs were observed by the X-ray Telescope (XRT) aboard the Hinode spacecraft du…

2012 Science China Physics, Mechanics, and Astronomy
Hinode 7
Martian ionogram scaling by the Object Tracking Method
DOI: 10.1007/s11433-012-4639-3 Bibcode: 2012SCPMA..55..540W

Ping, JinSong; Wang, MingYuan

The Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) onboard the Mars Express (MEX) spacecraft started to collect data of the Martian topside ionosphere from May, 2005. By now a large amount of ionograms has been obtained. It is important to extract vertical ionospheric information effectively from the ionograms for further stud…

2012 Science China Physics, Mechanics, and Astronomy
MEx 3