太阳光球，色球和过渡区域的高分辨率观察。协调的虹膜和SST观察数据库

论文标题

太阳光球，色球和过渡区域的高分辨率观察。协调的虹膜和SST观察数据库

High-resolution observations of the solar photosphere, chromosphere and transition region. A database of coordinated IRIS and SST observations

论文作者

van der Voort, L. H. M. Rouppe, De Pontieu, B., Carlsson, M., Rodriguez, J. de la Cruz, Bose, S., Chintzoglou, G., Drews, A., Froment, C., Gosic, M., Graham, D. R., Hansteen, V. H., Henriques, V. M. J., Jafarzadeh, S., Joshi, J., Kleint, L., Kohutova, P., Leifsen, T., Martinez-Sykora, J., Nobrega-Siverio, D., Ortiz, A., Pereira, T. M. D., Popovas, A., Noda, C. Quintero, Dalda, A. Sainz, Scharmer, G. B., Schmit, D., Scullion, E., Skogsrud, H., Szydlarski, M., Timmons, R., Vissers, G. J. M., Woods, M. M., Zacharias, P.

论文摘要

NASA的界面区域成像光谱仪（IRIS）通过紫外光谱和成像对太阳大气进行了高分辨率观测。自2013年6月发起IRIS以来，我们与La Palma的瑞典1-M太阳能望远镜（SST）进行了系统的观察活动。 SST提供了对光球和色球的互补高分辨率观察。 SST观察结果包括光晶Fin线中的光偏光成像以及色层CA II 8542 A，H-Alpha和Ca II K线中的光谱分辨成像。我们介绍了一个共对准的IRIS和SST数据集的数据库，该数据库开放向科学界分析。该数据库涵盖了各种目标，包括活动区域，黑子，杂技，安静的太阳和冠状孔。

NASA's Interface Region Imaging Spectrograph (IRIS) provides high resolution observations of the solar atmosphere through UV spectroscopy and imaging. Since the launch of IRIS in June 2013, we have conducted systematic observation campaigns in coordination with the Swedish 1-m Solar Telescope (SST) on La Palma. The SST provides complementary high-resolution observations of the photosphere and chromosphere. The SST observations include spectro-polarimetric imaging in photospheric Fe I lines and spectrally-resolved imaging in the chromospheric Ca II 8542 A, H-alpha, and Ca II K lines. We present a database of co-aligned IRIS and SST datasets that is open for analysis to the scientific community. The database covers a variety of targets including active regions, sunspots, plage, quiet Sun, and coronal holes.

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