THE SOLAR-RADIATION BETWEEN 3300-A AND 12500-A

THE SOLAR-RADIATION BETWEEN 3300-A AND 12500-A
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DOI:
10.1007/bf00173953
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发表时间:
1984-01-01
期刊:
影响因子:
2.8
通讯作者:
LABS, D
LABS, D
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
NECKEL, H;LABS, D

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结果如下合并:(a)我们以前发表的20个宽谱带的盘中心强度的绝对积分;(B)来自最近观测的这些谱带的中心到边缘变化的平均强度与中心强度的比值(λ <6600 λ);(c)根据Pierce和Slaughter的连续波长中心到边缘变化的观测结果得出的平均强度与中心强度的比值(d)J. Brault在Kitt峰获得的盘心和辐照度的高分辨率傅里叶变换光谱;(e)一些进一步的辅助数据,主要用于消除由大地分子谱带线引起的局部扰动,主要结果是提供了积分盘和盘中心的高精度辐射数据,关于线平均辐射和连续谱(在UV中:最高“窗口”强度)。内部精度(“散射”)不应比FTS光谱差,FTS光谱小于0.2%(平均误差);局部系统偏差不应超过0.5%。在其他地方已经证明了不存在显著的系统误差-中性或波长依赖性。
Results are presented, which follow from the merging of: (a) our previously published absolute integrals of the disk-center intensity for 20 Å wide spectral bands; (b) the ratios of mean to central intensity derived from recent observations of the center-to-limb variation of those bands (λ <6600 Å); (c) the ratios of mean to central intensity derived from the observations of the center-to-limb variation at continuum-wavelengths according to Pierce and Slaughter (λ >6600 Å); (d) the high resolution Fourier transform spectra obtained by J. Brault at Kitt Peak for the disk-center and the irradiance; (e) some further auxiliary data, which served mainly to eliminate the local perturbations caused by lines of telluric molecular bands.The main result is the presentation of high precision radiation data for both the integrated disk and the disk-center, concerning the line-averaged radiation and the continuum (in UV: highest ‘window’-intensities) as well.The internal accuracy (the ‘scatter’) should not be worse than that of the FTS spectra, which is less than 0.2% (mean error); local systematic deviations exceeding 0.5% are not to be expected. The absence of a significant systematic error - neutral or wavelength-dependent - has been proven already elsewhere.