UV solar irradiance in observations and the NRLSSI and SATIRE‐S models
UV solar irradiance in observations and the NRLSSI and SATIRE‐S models
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观测中的紫外线太阳辐照度以及 NRLSSI 和 SATIRE-S 模型
DOI：
10.1002/2015ja021277
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发表时间：
2015
期刊：
影响因子：
--
通讯作者：
J. Morrill
中科院分区：
文献类型：
--
作者：
K. L. Yeo;W. Ball;N. Krivova;S. Solanki;Y. Unruh;J. Morrill
自1978年以来，通过一系列空间飞行任务对太阳总辐照度和紫外光谱太阳辐照度进行了监测。与此同时，还开发了一些模型，旨在通过将变化与太阳磁活动联系起来，复制太阳辐照度。海军研究实验室太阳光谱辐照度（NRLSSI）和卫星时代光谱和总辐照度重建（SATIRE-S）模型提供了目前可用的卫星观测期间最全面的总和光谱太阳辐照度重建。在太阳周期变化的波长依赖性方面，各种测量和模型之间存在持续的争议，这对我们理解紫外线太阳辐照度变化对平流层的影响产生了影响。我们回顾了卫星观测期间紫外太阳辐照度变化的测量和建模。SATIRE-S重建与光谱太阳辐照度观测一致，它们是可靠的。它还得到了一个独立的，经验重建紫外光谱太阳辐照度的基础上高层大气研究卫星/太阳紫外光谱辐照度监测测量从早期的研究。NRLSSI在300和400 nm之间产生的较弱的太阳周期变化在任何现有记录中都不明显。我们表明，虽然用于构建NRLSSI的方法主要是健全的，重建的太阳周期变率是不确定性的影响，它借鉴了SSI观测的推导。根据我们的研究结果，我们建议在两个模型之间进行选择时，使用SATIRE-S进行气候研究。
Total solar irradiance and UV spectral solar irradiance has been monitored since 1978 through a succession of space missions. This is accompanied by the development of models aimed at replicating solar irradiance by relating the variability to solar magnetic activity. The Naval Research Laboratory Solar Spectral Irradiance (NRLSSI) and Spectral And Total Irradiance REconstruction for the Satellite era (SATIRE‐S) models provide the most comprehensive reconstructions of total and spectral solar irradiance over the period of satellite observation currently available. There is persistent controversy between the various measurements and models in terms of the wavelength dependence of the variation over the solar cycle, with repercussions on our understanding of the influence of UV solar irradiance variability on the stratosphere. We review the measurement and modeling of UV solar irradiance variability over the period of satellite observation. The SATIRE‐S reconstruction is consistent with spectral solar irradiance observations where they are reliable. It is also supported by an independent, empirical reconstruction of UV spectral solar irradiance based on Upper Atmosphere Research Satellite/Solar Ultraviolet Spectral Irradiance Monitor measurements from an earlier study. The weaker solar cycle variability produced by NRLSSI between 300 and 400 nm is not evident in any available record. We show that although the method employed to construct NRLSSI is principally sound, reconstructed solar cycle variability is detrimentally affected by the uncertainty in the SSI observations it draws upon in the derivation. Based on our findings, we recommend, when choosing between the two models, the use of SATIRE‐S for climate studies.
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使用贝叶斯推理评估太阳光谱辐照度与平流层臭氧之间的关系
影响因子：
3.3
作者：
Ball W
通讯作者：
Ball W
影响因子：
5.2
作者：
S. Oberländer;U. Langematz;K. Matthes;M. Kunze;A. Kubin;J. Harder;N. Krivova;S. Solanki;J. Pagaran;M. Weber
通讯作者：
S. Oberländer;U. Langematz;K. Matthes;M. Kunze;A. Kubin;J. Harder;N. Krivova;S. Solanki;J. Pagaran;M. Weber
影响因子：
6.5
作者：
Ball, W. T.;Unruh, Y. C.;Jaffe, A. H.
通讯作者：
Jaffe, A. H.
影响因子：
6.3
作者：
Ermolli, I.;Matthes, K.;Woods, T. N.
通讯作者：
Woods, T. N.