The Sun at millimeter wavelengths: II. Small-scale dynamic events in ALMA Band 3

0553644 - ASÚ 2022 RIV FR eng J - Článek v odborném periodiku
Eklund, H. … celkem 5 autorů
The Sun at millimeter wavelengths: II. Small-scale dynamic events in ALMA Band 3.
Astronomy & Astrophysics. Roč. 644, December (2020), č. článku A152. ISSN 0004-6361. E-ISSN 1432-0746
Výzkumná infrastruktura: EU-ARC.CZ II - 90106
Klíčová slova: Sun * chromosphere * radio radiation
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 5.803, rok: 2020
Způsob publikování: Omezený přístup
https://doi.org/10.1051/0004-6361/202038250

ALMA intensity data at millimeter(mm)-wavelengths are used for a first detailed systematic assessment of the occurrence and properties of small-scale dynamical features in the quiet Sun. We analyzed ALMA Band 3 data (similar to 3 mm/100 GHz) with a spatial resolution of similar to 1.4-2.1 arcsec and a duration of similar to 40 min together with SDO/HMI magnetograms. The temporal evolution of the mm maps is studied to detect pronounced dynamical features, which then are connected to dynamical events via a k-means clustering algorithm. We studied the physical properties of the resulting events and explored whether or not they show properties consistent with propagating shock waves. For this purpose, we calculated observable shock wave signatures at mm wavelengths from one- and three-dimensional model atmospheres. We detect 552 dynamical events with an excess in brightness temperature (Delta T-b) of at least >= 400 K. The events show a large variety in size up to similar to 9 '', amplitude Delta T-b up to similar to 1200 K with typical values in the range similar to 450-750 K, and lifetime at full width at half maximum of Delta T-b of between similar to 43 and 360 s, with typical values between similar to 55 and 125 s. Furthermore, many of the events show signature properties suggesting that they are likely produced by propagating shock waves. There are a lot of small-scale dynamic structures detected in the Band 3 data, even though the spatial resolution sets limitations on the size of events that can be detected. The number of dynamic signatures in the ALMA mm data is very low in areas with photospheric footpoints with stronger magnetic fields, which is consistent with the expectation for propagating shock waves.
Trvalý link: http://hdl.handle.net/11104/0328390