Observational, reference and model data on solar EUV, from measurements on AE-E
Observational, reference and model data on solar EUV, from measurements on AE-E
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DOI：
10.1029/gl008i011p01147
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发表时间：
1981-11
影响因子：
5.2
通讯作者：
H. Hinteregger;K. Fukui;B. Gilson
中科院分区：
文献类型：
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作者：
H. Hinteregger;K. Fukui;B. Gilson
在当前太阳黑子第21周的整个发展过程中，由AE - E卫星上的极紫外光谱仪（EUVS）实验所观测到的波长低于185纳米的太阳辐照度信息，对许多关于行星热层和电离层的研究都很重要。更先进的研究项目所需要的完整性和光谱细节方面的严格观测信息通常是缺乏的。因此，还有必要结合对适当参考光谱的详尽汇编来开发计算机模型。由于各种原因，我们很难选择合适的有效出版形式。我们认识到在科学期刊上完整重现我们的各种观测、参考和模型数据清单是不切实际的，于是我们开始了一种或多或少非正式的程序，即及时向少数特别感兴趣的同事发布信息。通过这封信，我们希望至少能缓解这一程序中一些不尽人意的方面。
Information on solar irradiance at wavelengths below 185 nm, observed by the EUVS experiment on the AE-E satellite over the entire development of the present sunspot cycle 21, is important to many investigations of planetary thermospheres and ionospheres. Strictly observational information is generally lacking in both the completeness and the spectral detail required by the more advanced study programs. Therefore, it has been necessary also to develop computer models in connection with fully detailed compilations of an appropriate reference spectrum. Our selection of appropriate forms of effective publication has been difficult for various reasons. Recognizing that full reproduction of our various lists of observational, reference, and model data in scientific journals would be impracticable, we started a more or less informal procedure of timely release of information to a limited number of particularly interested colleagues. With the present letter, we hope to mitigate at least some of the dissatisfactory aspects of this procedure.