Dataset for average bipolar solar active region
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F26%3A00647257" target="_blank" >RIV/67985815:_____/26:00647257 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Dataset for average bipolar solar active region
Original language description
Source data files for the study published in a paper Švanda et al., Average solar active region: I. Intensities, velocities, and the photospheric magnetic field, Astronomy and Astrophysics, preprint arXiv:2506.11713. The dataset contains the final ensemble-averaged FITS files of the datacubes capturing the evolution of the average normalised bipolar active region on the Sun in various physical quantities. The datacubes record the emergence and growth of this ensemble average obtained from averaging over 36 individual bipolar active regions in the following physical quantities: the continuum intensity, line-of-sight magnetogram, vector magnetogram (Bvec), inclination of the magnetic field (Bvec_inc) and the horizontal components (Bvec_X, Bvec_Y), line-of-sight Dopplergram, horizontal velocity calculated by LCT method, and intensities in three SDO/AIA channels: 1600, 304, and 171 Angstrom.
Czech name
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Czech description
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Classification
Type
X - Unclassified
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/GF23-07633K" target="_blank" >GF23-07633K: Unveiling the principles of solar magneto-convection</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2026
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů