MODELLING THE SOLAR UV RADIATION

机译：模拟太阳能紫外线辐射

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We model the solar spectrum with emphasis on the UV range with the spherical non-LTE atmosphere code COSI (COde for Solar Irradiance). Presently, we explicitly treat 31 levels in non-LTE and apply to 17 levels of neutral metals the latest theoretical photoionization cross sections. The atmosphere models are based on the observed temperature and density structures by Fontenla et al. (1999), which include the chromosphere and transition region. We compare synthetic spectra from 2000 to 7500 A in local thermodynamic equilibrium (LTE) with calculations from a Kurucz model, as well as theoretical Balmer line profiles computed in non-LTE with observations.

机译：我们使用球形非LTE大气代码COSI（太阳辐照度COde）对紫外线范围内的太阳光谱进行建模。目前，我们明确处理非LTE中的31种水平，并将最新理论光电离截面应用于17种水平的中性金属。大气模型基于Fontenla等人观察到的温度和密度结构。（1999年），其中包括色球层和过渡区。我们将本地热力学平衡（LTE）中2000至7500 A的合成光谱与Kurucz模型的计算结果进行了比较，并将非LTE中的理论Balmer线轮廓与观察结果进行了比较。

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来源
《International Solar Cycle Studies (ISCS) Symposium 2003; Jun 23-28, 2003; Tatranska Lomnica, Slovak Republic》|2003年|p.289-292|共4页
会议地点 Tatranska Lomnica(SK)
作者
M. Haberreiter; W. Schmutz;
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作者单位

Physikalisch-Meteorologisches Observatorium Davos, Dorfstrasse 33, CH-7260 Davos Dorf, Switzerland;

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会议组织
原文格式 PDF
正文语种 eng
中图分类环境科学基础理论;
关键词
sun: UV irradiance; sun: variability; radiative transfer;

机译：太阳：紫外线辐射；太阳：变化；辐射转移;

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5. A SOLAR RADIATION MODEL AND AN ANALYSIS OF SYNOPTIC SOLAR RADIATION REGIMES IN BRITISH COLUMBIA. [D] . SUCKLING, PHILIP WAYNE. 1977

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MODELLING THE SOLAR UV RADIATION

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