A high-resolution atlas of the infrared spectrum of the Sun and the Earth atmosphere from space. Volume 3: Key to identification of solar features
A high-resolution atlas of the infrared spectrum of the Sun and the Earth atmosphere from space. Volume 3: Key to identification of solar features
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发表时间：
1992-08
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通讯作者：
M. Geller
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作者：
M. Geller
1985 年 4 月 29 日至 5 月 2 日期间，大气痕量分子光谱 (ATMOS) 实验作为挑战者号航天飞机上 Spacelab-3 (SL-3) 有效载荷的一部分进行运行。该仪器是一台傅里叶变换光谱仪，从 360 公里的高度记录了 2000 多个红外太阳光谱。尽管大部分光谱是通过地球大气层边缘获取的，以便更好地了解其成分，但数百个“高太阳”光谱完全不受大地吸收。这些从太空记录的高太阳光谱是目前唯一不受地球大气成分吸收的太阳高分辨率红外光谱。本系列的第 1 卷和第 2 卷提供了这些光谱的汇编，以适合快速查看参考目的的格式排列，并且是来自太空的太阳和地球大气层的连续高分辨率红外光谱的第一个记录。在构成本卷主体的识别表中，每个八个波数块都有一个单独的标题，并对应于本系列第一卷中两个面板的一页。此外，来自 ATMOS 的 622-630 cm(exp -1)、630-638 cm(exp -1) 和 638-646 cm(exp -1) 三个独立的数据块（由于信噪比低而被排除在第 1 卷之外）由于对几个 OH 和 NH 跃迁的确定识别而被包括在内。在表的第一列中，给出了校正频率。第二列标识分子种类。第三列和第四列代表指定的转换。第五列给出了分子线的深度（以毫米为单位）。此列中还包含一个符号，用于指示该线是混合线还是位于另一条线的肩部。如果该行无法识别，最后一列会重复问号。
During the period April 29 through May 2, 1985, the Atmospheric Trace Molecule Spectroscopy (ATMOS) experiment was operated as part of the Spacelab-3 (SL-3) payload on the shuttle Challenger. The instrument, a Fourier transform spectrometer, recorded over 2000 infrared solar spectra from an altitude of 360 km. Although the majority of the spectra were taken through the limb of the Earth's atmosphere in order to better understand its composition, several hundred of the 'high-sun' spectra were completely free from telluric absorption. These high-sun spectra recorded from space are, at the present time, the only high-resolution infrared spectra ever taken of the Sun free from absorptions due to constituents in the Earth's atmosphere. Volumes 1 and 2 of this series provide a compilation of these spectra arranged in a format suitable for quick-look reference purposes and are the first record of the continuous high-resolution infrared spectrum of the Sun and the Earth's atmosphere from space. In the Table of Identifications, which constitutes the main body of this volume, each block of eight wavenumbers is given a separate heading and corresponds to a page of two panels in Volume 1 of this series. In addition, three separate blocks of data available from ATMOS from 622-630 cm(exp -1), 630-638 cm(exp -1) and 638-646 cm(exp -1), excluded from Volume 1 because of the low signal-to-noise ratio, have been included due to the certain identification of several OH and NH transitions. In the first column of the table, the corrected frequency is given. The second column identifies the molecular species. The third and fourth columns represent the assigned transition. The fifth column gives the depth of the molecular line in millimeters. Also included in this column is a notation to indicate whether the line is a blend or lies on the shoulder(s) of another line(s). The final column repeats a question mark if the line is unidentified.