A new approach for deriving the solar irradiance from nonflaring solar upper atmosphere plasmas at 2 × 104 ≤ T ≤ 2 × 107 K

We propose a new approach for deriving the solar irradiance due to the emission by solar upper atmosphere plasmas at 2 × 104 ≤ T ≤ 2 × 107 K for wavelengths shorter than 800 Å. Our approach is based on a new understanding of the properties of the solar upper atmosphere; specifically, the discovery t...

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Veröffentlicht in:	Journal of Geophysical Research. B. Solid Earth 2010-03, Vol.115 (A3), p.n/a
Hauptverfasser:	Feldman, U., Brown, C. M., Seely, J. F., Dammasch, I. E., Landi, E., Doschek, G. A., Colgan, J., Abdallah Jr, J., Fontes, C. J., Sherrill, M. E.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Astrophysics Atmosphere Emission Emission measurements Geophysics Irradiance Physics Plasmas Recording Spectrometers Sun Upper atmosphere Wavelengths
Online-Zugang:	Volltext
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