摘要: Since the early 1970s we have been developing the extensive computer programsneeded to construct models of the solar atmosphere and to calculate detailed spectra for use in the interpretation of solar observations. This research i... 展开
作者 | Avrett, E. H. | ||
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原报告号 | N9423569 | 总页数 | 10 |
报告类别/文献类型 | NASA / NTIS科技报告 | ||
关键词 | Chromosphere Solar atmosphere Solar spectra Solar physics Stellar models Sun Atomic spectra Computer programs Line spectra Molecular spectra Solar activity |