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Here for the first time is a comprehensive and up-to-date survey of the proposed theories of chromospheric and coronal heating in stars; the theories are critically reviewed and compared together with the observational evidence. This is an indispensable source for forthcoming work in such areas as stellar activity, radio and XUV emission, rotation, and mass loss.

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Produktbeschreibung
Here for the first time is a comprehensive and up-to-date survey of the proposed theories of chromospheric and coronal heating in stars; the theories are critically reviewed and compared together with the observational evidence. This is an indispensable source for forthcoming work in such areas as stellar activity, radio and XUV emission, rotation, and mass loss.

Dieser Download kann aus rechtlichen Gründen nur mit Rechnungsadresse in A, B, BG, CY, CZ, D, DK, EW, E, FIN, F, GR, HR, H, IRL, I, LT, L, LR, M, NL, PL, P, R, S, SLO, SK ausgeliefert werden.

Autorenporträt
Here for the first time is a comprehensive and up-to-date survey of the proposed theories of chromospheric and coronal heating in stars; the theories are critically reviewed and compared together with the observational evidence. This is an indispensable source for forthcoming work in such areas as stellar activity, radio and XUV emission, rotation, and mass loss.