The solar wind in time
| Author | |
|---|---|
| Abstract |
We describe our method for measuring mass loss rates of F–M main sequence stars with high-resolution Lyman-α line profiles. Our diagnostic is the extra absorption on the blue side the interstellar hydrogen absorption produced by neutral hydrogen gas in the hydrogen walls of stars. For stars with low X-ray fluxes, the correlation of observed mass loss rate with X-ray surface flux and age predicts the solar wind mass flux between 700 Myr and the present. |
| Year of Conference |
2011
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| Volume |
7
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| Start Page or Article ID |
286-290
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| Date Published |
2011-01
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| Publisher |
Cambridge University Press
|
| DOI |
10.1017/S174392131200498X
|
| Download citation | |
| Publication Status | |
| JILA PI | |
| JILA Topics | |
Conference Proceedings
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