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10.12942/lrsp-2004-2 http://scihub22266oqcxt.onion/10.12942/lrsp-2004-2 C4841182!4841182!27194955     free     free     free       Living+Rev+Sol+Phys 2004 ; 1 (ä): ä Nephropedia Template TP {{tp|p=27194955|t=2004. Astrospheres and Solar-like Stellar Winds |pdf=|usr=}}{{27194955}} gab.com Text Astrospheres and Solar-like Stellar Winds JO: Living Rev Sol Phys http://www.kidney.de/pget.php?&tw=1&pmid=27194955 #FOAvip 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? 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. Twit Text FOAVip Astrospheres and Solar-like Stellar Winds ????Living Rev Sol Phys http://www.kidney.de/pget.php?&tw=1&pmid=27194955 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=27194955 #FOAvip English Wikipedia <ref>{{Cite pmid|27194955}}</ref> Astrospheres and Solar-like Stellar Winds #MMPMID27194955 Wood BE Living Rev Sol Phys 2004[]; 1 (ä): ä PMID27194955show ga 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? 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. äAstrospheres and Solar-like Stellar Winds (epmc).pdf DeepDyve Pubget Overpricing