Dynamics and Kinematics of the EUV Wave Event on 6 May 2019
We present here the kinematics of the EUV wave associated with a GOES M1.0-class solar flare, which originates in NOAA AR 12740. The event is thoroughly observed with Atmospheric Imaging Assembly (AIA) onboard Solar Dynamics Observatory (SDO) with high spatio-temporal resolutions. This event display...
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2022
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ftmdpi:oai:mdpi.com:/2075-4434/10/2/58/ 2023-08-20T04:08:37+02:00 Dynamics and Kinematics of the EUV Wave Event on 6 May 2019 Ramesh Chandra P. F. Chen Pooja Devi Reetika Joshi Y. W. Ni 2022-04-10 application/pdf https://doi.org/10.3390/galaxies10020058 EN eng Multidisciplinary Digital Publishing Institute https://dx.doi.org/10.3390/galaxies10020058 https://creativecommons.org/licenses/by/4.0/ Galaxies; Volume 10; Issue 2; Pages: 58 EUV wave flare coronal hole Text 2022 ftmdpi https://doi.org/10.3390/galaxies10020058 2023-08-01T04:43:08Z We present here the kinematics of the EUV wave associated with a GOES M1.0-class solar flare, which originates in NOAA AR 12740. The event is thoroughly observed with Atmospheric Imaging Assembly (AIA) onboard Solar Dynamics Observatory (SDO) with high spatio-temporal resolutions. This event displays many features of EUV waves, which are very decisive for the understanding of the nature of EUV waves. These features include: a fast-mode wave, a pseudo wave, a slow-mode wave and stationary fronts, probably due to mode conversion. One fast-mode wave also propagates towards the coronal hole situated close to the north pole and the wave speed does not change when it encounters the coronal hole. We intend to provide self-consistent interpretations for all these different features. Text North Pole MDPI Open Access Publishing North Pole Galaxies 10 2 58 |
institution |
Open Polar |
collection |
MDPI Open Access Publishing |
op_collection_id |
ftmdpi |
language |
English |
topic |
EUV wave flare coronal hole |
spellingShingle |
EUV wave flare coronal hole Ramesh Chandra P. F. Chen Pooja Devi Reetika Joshi Y. W. Ni Dynamics and Kinematics of the EUV Wave Event on 6 May 2019 |
topic_facet |
EUV wave flare coronal hole |
description |
We present here the kinematics of the EUV wave associated with a GOES M1.0-class solar flare, which originates in NOAA AR 12740. The event is thoroughly observed with Atmospheric Imaging Assembly (AIA) onboard Solar Dynamics Observatory (SDO) with high spatio-temporal resolutions. This event displays many features of EUV waves, which are very decisive for the understanding of the nature of EUV waves. These features include: a fast-mode wave, a pseudo wave, a slow-mode wave and stationary fronts, probably due to mode conversion. One fast-mode wave also propagates towards the coronal hole situated close to the north pole and the wave speed does not change when it encounters the coronal hole. We intend to provide self-consistent interpretations for all these different features. |
format |
Text |
author |
Ramesh Chandra P. F. Chen Pooja Devi Reetika Joshi Y. W. Ni |
author_facet |
Ramesh Chandra P. F. Chen Pooja Devi Reetika Joshi Y. W. Ni |
author_sort |
Ramesh Chandra |
title |
Dynamics and Kinematics of the EUV Wave Event on 6 May 2019 |
title_short |
Dynamics and Kinematics of the EUV Wave Event on 6 May 2019 |
title_full |
Dynamics and Kinematics of the EUV Wave Event on 6 May 2019 |
title_fullStr |
Dynamics and Kinematics of the EUV Wave Event on 6 May 2019 |
title_full_unstemmed |
Dynamics and Kinematics of the EUV Wave Event on 6 May 2019 |
title_sort |
dynamics and kinematics of the euv wave event on 6 may 2019 |
publisher |
Multidisciplinary Digital Publishing Institute |
publishDate |
2022 |
url |
https://doi.org/10.3390/galaxies10020058 |
geographic |
North Pole |
geographic_facet |
North Pole |
genre |
North Pole |
genre_facet |
North Pole |
op_source |
Galaxies; Volume 10; Issue 2; Pages: 58 |
op_relation |
https://dx.doi.org/10.3390/galaxies10020058 |
op_rights |
https://creativecommons.org/licenses/by/4.0/ |
op_doi |
https://doi.org/10.3390/galaxies10020058 |
container_title |
Galaxies |
container_volume |
10 |
container_issue |
2 |
container_start_page |
58 |
_version_ |
1774720996268310528 |