Differences in physical properties of coronal bright points and their ALMA counterparts within and outside coronal holes

0583585 - ASÚ 2024 RIV FR eng J - Journal Article
Matković, F. … Total 9 authors
Differences in physical properties of coronal bright points and their ALMA counterparts within and outside coronal holes.
Astronomy & Astrophysics. Roč. 670, February (2023), č. článku A146. ISSN 0004-6361. E-ISSN 1432-0746
R&D Projects: GA MŠMT LM2023059; GA MŠMT LM2023059
Research Infrastructure: EU-ARC.CZ III - 90259
Keywords : Sun * corona * chromosphere
OECD category: Astronomy (including astrophysics,space science)
Impact factor: 6.5, year: 2022
Method of publishing: Open access
https://doi.org/10.1051/0004-6361/202244160

This study investigates and compares the physical properties, such as intensity and area, of coronal bright points (CBPs) inside and outside of coronal holes (CHs) using the Atacama Large Millimeter/submillimeter Array (ALMA) and Solar Dynamics Observatory (SDO) observations.
Permanent Link: https://hdl.handle.net/11104/0351589