重新审视SATIRE-S辐照度重建:威尔森山磁图和Ca II K观测的遗产

IF 5.8 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Theodosios Chatzistergos, Natalie A. Krivova, Sami K. Solanki, Kok Leng Yeo
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引用次数: 0

摘要

上下文。关于太阳辐照度长期变化的准确信息对了解太阳对地球气候的影响很重要,但由于星载实验的寿命相对较短,无法从直接辐照度测量中获得。利用太阳光球磁场测量值作为输入的模型可以提供对这些变化的独立评估。卫星时代的光谱和总辐照度重建(SATIRE-S)模型就是这样做的。不幸的是,SATIRE-S用于恢复辐照度变化的磁图档案也相对较短,相互重叠周期较短,因此难以评估其一致性。为了克服这个问题并更可靠地连接各种档案,我们包括了额外的输入数据集。我们改进了SATIRE-S总太阳辐照度(TSI)重建,首先结合了威尔逊山天文台的磁图,以及从默东、罗马和圣费尔南多岛 II K数据重建的无签名磁图,其次,通过重新分析各个档案结果之间重叠的所有时期。我们从所有8个输入档案中合并的每日辐照度重建与辐照度的直接测量结果非常吻合,特别是与TSIS1/TIM(总和光谱太阳辐照度传感器总辐照度监测器)数据相比,我们发现相关系数为0.98。1976年至2019年的最小TSI值差值为- 0.2±0.17 Wm−2,而1986年至2019年的最小TSI值差值无统计学意义(- 0.06±0.13 Wm−2)。我们的分析还揭示了TSI在所谓的ACRIM差距上所显示的趋势,不利于该时期TSI增加趋势的假设。通过纳入更多的直接和间接磁图时间序列,我们使SATIRE-S重建的TSI更加稳健和准确。新序列显示了近半个世纪以来TSI的下降趋势,这与大多数测量TSI的组合很好地吻合。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Revisiting the SATIRE-S irradiance reconstruction: Heritage of Mt Wilson magnetograms and Ca II K observations
Context. Accurate information on long-term variations in solar irradiance, important for understanding the solar influence on Earth’s climate, cannot be derived from direct irradiance measurements due to the comparatively short lifetimes of space-borne experiments. Models using measurements of the solar photospheric magnetic field as input can provide an independent assessment of the changes.Aims. The Spectral And Total Irradiance Reconstruction in the satellite era (SATIRE-S) model does just that. Unfortunately, the magnetogram archives used by SATIRE-S to recover irradiance variations are also relatively short-lived and have short mutual overlapping periods, making it difficult to evaluate their consistency. To overcome this and bridge the various archives more reliably, we include additional input data sets.Methods. We improve SATIRE-S total solar irradiance (TSI) reconstruction by firstly incorporating magnetograms from the Mt Wilson Observatory as well as unsigned magnetograms reconstructed from Meudon, Rome, and San Fernando Ca II K data, and secondly, by re-analysing all periods of overlaps between the various archives.Results. Our combined daily irradiance reconstruction from all eight input archives returns an excellent agreement with direct measurements of irradiance, in particular we find a correlation coefficient of 0.98 when compared to TSIS1/TIM (Total and Spectral Solar Irradiance Sensor Total Irradiance Monitor) data. The minimum-to-minimum TSI difference between 1976 and 2019 is −0.2 ± 0.17 Wm−2, while the TSI difference between the 1986 and 2019 minima is statistically insignificant (−0.06 ± 0.13 Wm−2). Our analysis also sheds light on the trend shown by the TSI over the so-called ACRIM gap, disfavouring a hypothesised increasing trend in TSI in that period.Conclusions. By including more direct and indirect magnetogram time series, we have made the TSI reconstructed by SATIRE-S more robust and accurate. The new series shows a reduced trend of decreasing TSI over the last half century, which agrees well with most composites of measured TSI.
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
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