Astrospheres and Solar-like Stellar Winds

Stellar analogs for the solar wind have proven to be frustratingly difficult to detect directly. However, these stellar winds can be studied indirectly by observing the interaction regions carved out by the collisions between these winds and the interstellar medium (ISM). These interaction regions a...

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Main Author: Wood Brian E.
Format: Article
Language:English
Published: Springer 2004-07-01
Series:Living Reviews in Solar Physics
Subjects:
Online Access:http://www.livingreviews.org/lrsp-2004-2
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author Wood Brian E.
author_facet Wood Brian E.
author_sort Wood Brian E.
collection DOAJ
description Stellar analogs for the solar wind have proven to be frustratingly difficult to detect directly. However, these stellar winds can be studied indirectly by observing the interaction regions carved out by the collisions between these winds and the interstellar medium (ISM). These interaction regions are called "astrospheres", analogous to the "heliosphere" surrounding the Sun. The heliosphere and astrospheres contain a population of hydrogen heated by charge exchange processes that can produce enough H I Ly alpha absorption to be detectable in UV spectra of nearby stars from the Hubble Space Telescope (HST). The amount of astrospheric absorption is a diagnostic for the strength of the stellar wind, so these observations have provided the first measurements of solar-like stellar winds. Results from these stellar wind studies and their implications for our understanding of the solar wind are reviewed here. Of particular interest are results concerning the past history of the solar wind and its impact on planetary atmospheres.
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spelling doaj.art-06b31925f97e4d7a9a4608352482e5fb2023-09-03T05:59:04ZengSpringerLiving Reviews in Solar Physics1614-49612004-07-0112Astrospheres and Solar-like Stellar WindsWood Brian E.Stellar analogs for the solar wind have proven to be frustratingly difficult to detect directly. However, these stellar winds can be studied indirectly by observing the interaction regions carved out by the collisions between these winds and the interstellar medium (ISM). These interaction regions are called "astrospheres", analogous to the "heliosphere" surrounding the Sun. The heliosphere and astrospheres contain a population of hydrogen heated by charge exchange processes that can produce enough H I Ly alpha absorption to be detectable in UV spectra of nearby stars from the Hubble Space Telescope (HST). The amount of astrospheric absorption is a diagnostic for the strength of the stellar wind, so these observations have provided the first measurements of solar-like stellar winds. Results from these stellar wind studies and their implications for our understanding of the solar wind are reviewed here. Of particular interest are results concerning the past history of the solar wind and its impact on planetary atmospheres.http://www.livingreviews.org/lrsp-2004-2Solar windStellar windsHeliosphereAstrosphere
spellingShingle Wood Brian E.
Astrospheres and Solar-like Stellar Winds
Living Reviews in Solar Physics
Solar wind
Stellar winds
Heliosphere
Astrosphere
title Astrospheres and Solar-like Stellar Winds
title_full Astrospheres and Solar-like Stellar Winds
title_fullStr Astrospheres and Solar-like Stellar Winds
title_full_unstemmed Astrospheres and Solar-like Stellar Winds
title_short Astrospheres and Solar-like Stellar Winds
title_sort astrospheres and solar like stellar winds
topic Solar wind
Stellar winds
Heliosphere
Astrosphere
url http://www.livingreviews.org/lrsp-2004-2
work_keys_str_mv AT woodbriane astrospheresandsolarlikestellarwinds