Identifications of Emission Lines in the EUV Solar Spectrum
نویسندگان
چکیده
منابع مشابه
Retrieving the solar EUV spectrum from a reduced set of spectral lines
The solar EUV irradiance is a key input for thermospheric and ionospheric models. Difficulties in continuously measuring the calibrated spectrum has prompted the use of various surrogate quantities. Although most proxies correlate quite well with the spectral variability, their use for modelling purposes becomes increasingly unsatisfactory. A different and data-driven approach is considered her...
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P. R. Young, G. Del Zanna, H. E. Mason, K. P. Dere, E. Landi, M. Landini, G. A. Doschek, 1STFC Rutherford Appleton Laboratory, Chilton, Didcot, Oxfor 2University College London, Department of Space and Climate Physics, 3DAMTP, Centre for Mathematical Sciences, 4George Mason University, 4400 University Dr., Fairfax 5Artep, Inc at Naval Research Laboratory, 4555 Overlook Ave. S.W., 6Code 7670, Na...
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ژورنال
عنوان ژورنال: International Astronomical Union Colloquium
سال: 1972
ISSN: 0252-9211
DOI: 10.1017/s0252921100089740