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使用多相同辐照度水平(MuSIL)分析技术解耦太阳变化和仪器趋势。

Decoupling Solar Variability and Instrument Trends Using the Multiple Same-Irradiance-Level (MuSIL) Analysis Technique.

作者信息

Woods Thomas N, Eparvier Francis G, Harder Jerald, Snow Martin

机构信息

Laboratory for Atmospheric and Space Physics, University of Colorado, 3665 Discovery Drive, CO 80303 Boulder, USA.

出版信息

Sol Phys. 2018;293(5):76. doi: 10.1007/s11207-018-1294-5. Epub 2018 Apr 23.

Abstract

The solar spectral irradiance (SSI) dataset is a key record for studying and understanding the energetics and radiation balance in Earth's environment. Understanding the long-term variations of the SSI over timescales of the 11-year solar activity cycle and longer is critical for many Sun-Earth research topics. Satellite measurements of the SSI have been made since the 1970s, most of them in the ultraviolet, but recently also in the visible and near-infrared. A limiting factor for the accuracy of previous solar variability results is the uncertainties for the instrument degradation corrections, which need fairly large corrections relative to the amount of solar cycle variability at some wavelengths. The primary objective of this investigation has been to separate out solar cycle variability and any residual uncorrected instrumental trends in the SSI measurements from the (SORCE) mission and the (TIMED) mission. A new technique called the Multiple Same-Irradiance-Level (MuSIL) analysis has been developed, which examines an SSI time series at different levels of solar activity to provide long-term trends in an SSI record, and the most common result is a downward trend that most likely stems from uncorrected instrument degradation. This technique has been applied to each wavelength in the SSI records from SORCE (2003 - present) and TIMED (2002 - present) to provide new solar cycle variability results between 27 nm and 1600 nm with a resolution of about 1 nm at most wavelengths. This technique, which was validated with the highly accurate total solar irradiance (TSI) record, has an estimated relative uncertainty of about 5% of the measured solar cycle variability. The MuSIL results are further validated with the comparison of the new solar cycle variability results from different solar cycles.

摘要

太阳光谱辐照度(SSI)数据集是研究和理解地球环境中的能量学与辐射平衡的关键记录。了解太阳光谱辐照度在11年太阳活动周期及更长时间尺度上的长期变化,对于许多日地研究课题至关重要。自20世纪70年代以来就开始进行太阳光谱辐照度的卫星测量,其中大部分测量集中在紫外线波段,但最近也扩展到了可见光和近红外波段。此前太阳变化结果准确性的一个限制因素是仪器退化校正的不确定性,在某些波长下,相对于太阳周期变化量而言,这种校正需要相当大的幅度。本次调查的主要目标是从太阳辐射和气候实验(SORCE)任务以及热层电离层、中层能量与动力学(TIMED)任务的太阳光谱辐照度测量数据中,分离出太阳周期变化以及任何残留的未校正仪器趋势。一种名为多同辐照度水平(MuSIL)分析的新技术已经被开发出来,该技术通过在不同太阳活动水平下检查太阳光谱辐照度时间序列,以提供太阳光谱辐照度记录中的长期趋势,最常见的结果是一种下降趋势,这很可能源于未校正的仪器退化。该技术已应用于SORCE(2003年至今)和TIMED(2002年至今)太阳光谱辐照度记录中的每个波长,以提供27纳米至1600纳米之间新的太阳周期变化结果,在大多数波长下分辨率约为1纳米。该技术通过高度精确的总太阳辐照度(TSI)记录进行了验证,估计相对不确定性约为所测量太阳周期变化的5%。通过比较不同太阳周期的新太阳周期变化结果,进一步验证了MuSIL结果。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a7d4/6438597/4899bd7b7d6f/11207_2018_1294_Fig2_HTML.jpg

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