Dataset for average bipolar solar active region

Kód výsledku v 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>

Výsledek na webu

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DOI - Digital Object Identifier

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Jazyk výsledku

angličtina

Název v původním jazyce

Dataset for average bipolar solar active region

Popis výsledku v původním jazyce

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.

Název v anglickém jazyce

Dataset for average bipolar solar active region

Popis výsledku anglicky

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.

Druh

X - Nezařazeno

CEP obor

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OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

<a href="/cs/project/GF23-07633K" target="_blank" >GF23-07633K: Odhalování principů konvekce v magnetických polích Slunce</a><br>

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2026

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů