z-logo
open-access-imgOpen Access
The Sun as an X‐Ray Star. IV. The Contribution of Different Regions of the Corona to Its X‐Ray Spectrum
Author(s) -
S. Orlando,
G. Pérès,
F. Reale
Publication year - 2001
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/322333
Subject(s) - physics , astrophysics , rosat , luminosity , corona (planetary geology) , spectral line , stars , astronomy , brightness , light curve , flux (metallurgy) , solar radius , coronal mass ejection , plasma , galaxy , solar wind , quantum mechanics , astrobiology , venus , materials science , metallurgy

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom