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Autre Publication Scientifique From the Outer Heliosphere to the Local Bubble, Space Sciences Series of ISSI Année : 2009

The Solar Wind Charge-eXchange Contribution to the Local Soft X-ray Background

Résumé

The major sources of the Soft X-ray Background (SXRB), besides distinct structures as supernovae and superbubbles (e.g. Loop I), are: (i) an absorbed extragalactic emission following a power law, (ii) an absorbed thermal component (∼2×106 K) from the galactic disk and halo, (iii) an unabsorbed thermal component, supposedly at 106 K, attributed to the Local Bubble and (iv) the very recently identified unabsorbed Solar Wind Charge-eXchange (SWCX) emission from the heliosphere and the geocorona.

Dates et versions

hal-04113795 , version 1 (01-06-2023)

Identifiants

Citer

Dimitra Koutroumpa, Rosine Lallement, Vasili Kharchenko, Alex Dalgarno. The Solar Wind Charge-eXchange Contribution to the Local Soft X-ray Background. 2009, pp.217. ⟨10.1007/978-1-4419-0247-4_17⟩. ⟨hal-04113795⟩
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