搜索结果: 1-6 共查到“空间天文学 PLASMA”相关记录6条 . 查询时间(0.109 秒)
日冕物质抛射(CME)是灾害性空间天气的主要驱动源，如何针对特定的CME事件, 了解其在日冕和行星际空间的传播特性及演化过程，预测近地空间太阳风状态的变化，是空间天气研究领域的重要内容，同时受到国内外学者的广泛关注，近年来，在CME传播特性的观测和数值模拟研究中取得了大量进展。
Suzaku Discovery of Twin Thermal Plasma from the Tornado Nebula
ISM: individual (G357.7− 0.1)—ISM: jets and outfl ows—X-ray:ISM
2011/9/28
The Tornado nebula (G357.7-0.1) is a mysterious radio source with bright "head" and faint "tail" located in the direction of the Galactic center (GC) region. We here report the discovery of two diffus...
We present some methods of X-ray data analysis employed in our laboratory for deducing the physical parameters of flaring plasma. For example, we have used a flare well observed with Polish instrument...
Spectral Measurements of Cyg X-3: A Thermal Source Embedded in Hot Plasma within a Cold Shell
Low mass X-ray binaries X-ray sources Cyg X-3
2009/5/19
The attempts at unified model fitting to explain the spectral
variations in Cyg X-3 suggest equally probable fits with a combination of
an absorbed blackbody and a separately absorbed power law with...
We present some methods of X-ray data analysis employed in
our laboratory for deducing the physical parameters of flaring plasma. For
example, we have used a flare well observed with Polish instrum...
DUST PLASMA ANALOGUE FOR INTERSTELLAR 217.5 nm EXTINCTION
dust extinction-Methods laboratory
2009/1/16
The new ultraviolet (UV) extinction measurements of carbona-
ceous nanoparticles in the range from 140 nm to 260 nm are presented. The plasma
polymerized hydrocarbon nanoparticles were already propo...