校准和发布在威尔逊山 150 英尺塔式望远镜 (MWO) 上获取的磁图/多普勒图

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Roger K. Ulrich, John Boyden, Tham Tran
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引用次数: 0

摘要

威尔逊山天文台的太阳磁盘磁场、多普勒速度和光谱线强度观测档案是研究 1967 年至 2013 年太阳状态的资源。在解释这一记录时,必须考虑这一时期仪器的变化/升级。该记录的部分内容此前已经发布。本出版物记录了数据记录,以便对其进行独立解释。档案可通过两个目录树获取,访问网址为 http://sha.stanford.edu/mwo/msm.html。观测数据的校准受到太阳表面对流的影响,对差转和经向环流函数都产生了偏移。在本出版物和其他出版物中,已通过时间平均法减少了这些偏移的影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Calibration and Release of Magnetograms/Dopplergrams Obtained at the Mt. Wilson 150-Foot Tower Telescope (MWO)

The Mt. Wilson Observatory archive of observations of solar disk magnetic fields, Doppler velocities, and spectral line intensities is a resource for studying the Sun’s state from 1967 to 2013. Instrument changes/upgrades during this time must be considered when interpreting this record. Portions of this record have been previously released. This publication documents the data record in order to allow its independent interpretation. The archive is available through two directory trees which can be accessed at http://sha.stanford.edu/mwo/msm.html. The calibration of the observations is impacted by the solar surface convective flows, which produce offsets for both differential rotation and meridional circulation functions. The effects of these offsets have been reduced in this and other publications by temporal averaging.

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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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