... As an example for an observation of a stellar corona, a simulation of the response of RGS was performed. ... The input spectrum was a two component Mewe-Kaastra plasma, with solar abundance, and temperatures of 0.35 and 2 keV. ...
... The hot phase of the Galactic ISM . Cool gas . Stellar coronae . ... to see whether X-ray data can corroborate the "canonical" value of 1.4 solar masses ... to come from their million degree coronae, which are thin plasmas approximately in ...
... no clear correlation between the EPIC-pn CTE degradation and proton flares solar flares created a series of jumps in the EPIC-MOS cameras CTE EPIC-pn CTE is degrading independently of the solar flares with a nearly constant rate EPIC-MOS Al З EPIC-pn Mn З ...
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Ссылки http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/XMM_KIRSCH_POLLOCK.pdf -- 2643.9 Кб -- 19.06.2006 Похожие документы
... lines observed in a number of stellar coronae with agreement between model and data ... throughout the mission of 3 stellar coronae in first and second order for RGS1 and ...
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Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0030-5-1.pdf -- 977.2 Кб -- 12.11.2008 Похожие документы