太阳黑子观测数据档案:邓恩太阳望远镜的持续运行。

IF 2.4 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Sean G. Sellers, Juie Shetye, Damian J. Christian, David B. Jess, Peter H. Keys, Gordon A. MacDonald, R. T. James McAteer, Jason Jackiewicz, Colin Hancock, Michael S. Thompson, Jamey E. Eriksen, Sara Jeffreys
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引用次数: 0

摘要

太阳黑子天文台数据档案(SSODA)存储了从2018年2月至今理查德·邓恩太阳望远镜(DST)上的一套仪器获得的数据。DST的仪器继续提供太阳光球和色球在3500 Å到11000 Å波长范围内的高节奏成像、光谱和偏振测量。在撰写本文时,该档案包含超过520个观测日(从2018年2月1日开始)的大约374 TiB数据。这些数字是近似值,因为DST仍在运行,并且正在积极地向存档添加新数据。SSODA包括原始数据和校准数据。该档案的一个子集包含使用Hazel-2.0代码进行光球和色球光谱偏振反演的结果,以获得磁场、温度和速度流的地图。SSODA是研究整个太阳大气层等离子体过程、空间天气事件的起源以及太阳周期25上升期间活动区性质的独特资源。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The Sunspot Solar Observatory Data Archive: Continuing Operations at the Dunn Solar Telescope

The Sunspot Solar Observatory Data Archive (SSODA) stores data acquired with the suite of instruments at the Richard B. Dunn Solar Telescope (DST) from February 2018 to the present. The instrumentation at the DST continues to provide high cadence imaging, spectroscopy, and polarimetry of the solar photosphere and chromosphere across a wavelength range from 3500 Å to 11,000 Å. At the time of writing, the archive contains approximately 374 TiB of data across more than 520 observing days (starting on February 1, 2018). These numbers are approximate as the DST remains operational, and is actively adding new data to the archive. The SSODA includes both raw and calibrated data. A subset of the archive contains the results of photospheric and chromospheric spectropolarimetric inversions using the Hazel-2.0 code to obtain maps of magnetic fields, temperatures, and velocity flows. The SSODA represents a unique resource for the investigation of plasma processes throughout the solar atmosphere, the origin of space weather events, and the properties of active regions throughout the rise of Solar Cycle 25.

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来源期刊
Solar Physics
Solar Physics 地学天文-天文与天体物理
CiteScore
5.10
自引率
17.90%
发文量
146
审稿时长
1 months
期刊介绍: Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Papers on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun.
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