Spectropolarimetric observations of the solar atmosphere in the H alpha 6563 angstrom line
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00556498" target="_blank" >RIV/67985815:_____/22:00556498 - isvavai.cz</a>
Výsledek na webu
<a href="https://doi.org/10.1051/0004-6361/202141834" target="_blank" >https://doi.org/10.1051/0004-6361/202141834</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/202141834" target="_blank" >10.1051/0004-6361/202141834</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Spectropolarimetric observations of the solar atmosphere in the H alpha 6563 angstrom line
Popis výsledku v původním jazyce
We present novel spectropolarimetric observations of the hydrogen H alpha line taken with the Zurich Imaging Polarimeter (ZIMPOL) at the Gregory Coude Telescope of the Istituto Ricerche Solari Locarno (IRSOL). The linear polarization is clearly dominated by the scattering of anisotropic radiation and the Hanle effect, while the circular polarization is dominated by the Zeeman effect. The observed linear polarization signals show a rich spatial variability, the interpretation of which would open a new window for probing the solar chromosphere. We study their spatial variation within coronal holes, finding a different behaviour for the U/I signals near the north and south solar poles. We identify some spatial patterns, which may facilitate the interpretation of the observations. In close-to-the-limb regions with sizable circular polarization signals, we find similar asymmetric Q/I profiles. We also show examples of net circular polarization profiles (NCP), along with the corresponding linear polarization signals. The application of the weak field approximation to the observed circular polarization signals gives 10 G (40-60 G) close to the limb quiet (plage) regions for the average longitudinal field strength over the spatio-temporal resolution element.
Název v anglickém jazyce
Spectropolarimetric observations of the solar atmosphere in the H alpha 6563 angstrom line
Popis výsledku anglicky
We present novel spectropolarimetric observations of the hydrogen H alpha line taken with the Zurich Imaging Polarimeter (ZIMPOL) at the Gregory Coude Telescope of the Istituto Ricerche Solari Locarno (IRSOL). The linear polarization is clearly dominated by the scattering of anisotropic radiation and the Hanle effect, while the circular polarization is dominated by the Zeeman effect. The observed linear polarization signals show a rich spatial variability, the interpretation of which would open a new window for probing the solar chromosphere. We study their spatial variation within coronal holes, finding a different behaviour for the U/I signals near the north and south solar poles. We identify some spatial patterns, which may facilitate the interpretation of the observations. In close-to-the-limb regions with sizable circular polarization signals, we find similar asymmetric Q/I profiles. We also show examples of net circular polarization profiles (NCP), along with the corresponding linear polarization signals. The application of the weak field approximation to the observed circular polarization signals gives 10 G (40-60 G) close to the limb quiet (plage) regions for the average longitudinal field strength over the spatio-temporal resolution element.
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10308 - Astronomy (including astrophysics,space science)
Návaznosti výsledku
Projekt
<a href="/cs/project/GA19-20632S" target="_blank" >GA19-20632S: Dopředné modelování a inverze polarizovaných slunečních spekter ve vícedimenzionálních geometriích</a><br>
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2022
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Astronomy & Astrophysics
ISSN
0004-6361
e-ISSN
1432-0746
Svazek periodika
659
Číslo periodika v rámci svazku
March
Stát vydavatele periodika
FR - Francouzská republika
Počet stran výsledku
16
Strana od-do
A179
Kód UT WoS článku
000773023600009
EID výsledku v databázi Scopus
2-s2.0-85127386308