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X-ray astronomy of stellar coronae
DOI: 10.1007/s00159-004-0023-2 Bibcode: 2004A&ARv..12...71G

Güdel, Manuel

X-ray emission from stars in the cool half of the Hertzsprung-Russell diagram is generally attributed to the presence of a magnetic corona that contains plasma at temperatures exceeding 1 million K. Coronae are ubiquitous among these stars, yet many fundamental mechanisms operating in their magnetic fields still elude an interpretation through a d…

2004 Astronomy and Astrophysics Review
XMM-Newton 406
Solar radiative output and its variability: evidence and mechanisms
DOI: 10.1007/s00159-004-0024-1 Bibcode: 2004A&ARv..12..273F

Fröhlich, Claus; Lean, Judith

Electromagnetic radiation from the Sun is Earth’s primary energy source. Space-based radiometric measurements in the past two decades have begun to establish the nature, magnitude and origins of its variability. An 11-year cycle with peak-to-peak amplitude of order 0.1 % is now well established in recent total solar irradiance observations, as are…

2004 Astronomy and Astrophysics Review
SOHO 275