Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.0755l&link_type=abstract
American Astronomical Society, HEAD meeting #9, #7.55; Bulletin of the American Astronomical Society, Vol. 38, p.358
Astronomy and Astrophysics
Astronomy
Scientific paper
We study the EUV/soft X-ray emission generated by charge transfer between solar wind heavy ions and interstellar H and He neutral atoms in the inner Heliosphere. We present heliospheric maps for stationary solar wind, depending on solar cycle phase, solar wind anisotropies and composition, line of sight direction and observer position. A series of time-dependant simulations of the X-ray intensities variations due to temporary solar wind enhancements are compared with XMM Newton recorded spectra at different intervals in the period 2000-2003. Results show that the heliospheric component can explain a large fraction of (if not all) the line intensity below 1.3 keV, strongly attenuating the need for soft X-ray emission from the Local Interstellar Bubble.
Acero Fabio
Ballet Jean
Dalgarno Alexander
Kharchenko Vasili
Koutroumpa Dimitra
No associations
LandOfFree
Temporal Variations of Charge-Exchange induced Heliospheric X-rays: Constraints on the Local Interstellar X-ray Background does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Temporal Variations of Charge-Exchange induced Heliospheric X-rays: Constraints on the Local Interstellar X-ray Background, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Temporal Variations of Charge-Exchange induced Heliospheric X-rays: Constraints on the Local Interstellar X-ray Background will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-777190