Observations of small-scale energetic events in the solar transition region: explosive events, UV bursts, and network jets
In this paper, we review observational aspects of three common small-scale energetic events in the solar transition region (TR), namely TR explosive events, ultraviolet bursts and jets. These events are defined in either (both) spectral or (and) imaging data. The development of multiple instruments...
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doaj-f49a437b363245f1950c217cb3c2837f2020-11-24T21:32:35ZengINFRA-M Solar-Terrestrial Physics2500-05352019-06-0152586810.12737/stp-52201909Observations of small-scale energetic events in the solar transition region: explosive events, UV bursts, and network jetsZhenghua Huang0Bo Li1Lidong Xia2Institute of Space Sciences, Shandong University, Weihai, Shandong, ChinaInstitute of Space Sciences, Shandong University, Weihai, Shandong, ChinaInstitute of Space Sciences, Shandong University, Weihai, Shandong, ChinaIn this paper, we review observational aspects of three common small-scale energetic events in the solar transition region (TR), namely TR explosive events, ultraviolet bursts and jets. These events are defined in either (both) spectral or (and) imaging data. The development of multiple instruments capable of observing the TR has allowed researchers to gain numerous insights into these phenomena in recent years. These events have provided a proxy to study how mass and energy are transported between the solar chromosphere and the corona. As the physical mechanisms responsible for these small-scale events might be similar to the mechanisms responsible for large-scale phenomena, such as flares and coronal mass ejections, analysis of these events could also help our understanding of the solar atmosphere from small to large scales. The observations of these small-scale energetic events demonstrate that the TR is extremely dynamic and is a crucial layer in the solar atmosphere between the chromosphere and the corona. https://naukaru.ru/en/nauka/article/29507/viewtransition regionmagnetic reconnectionsmall-scale dynamicsspectroscopic observations |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Zhenghua Huang Bo Li Lidong Xia |
spellingShingle |
Zhenghua Huang Bo Li Lidong Xia Observations of small-scale energetic events in the solar transition region: explosive events, UV bursts, and network jets Solar-Terrestrial Physics transition region magnetic reconnection small-scale dynamics spectroscopic observations |
author_facet |
Zhenghua Huang Bo Li Lidong Xia |
author_sort |
Zhenghua Huang |
title |
Observations of small-scale energetic events in the solar transition region: explosive events, UV bursts, and network jets |
title_short |
Observations of small-scale energetic events in the solar transition region: explosive events, UV bursts, and network jets |
title_full |
Observations of small-scale energetic events in the solar transition region: explosive events, UV bursts, and network jets |
title_fullStr |
Observations of small-scale energetic events in the solar transition region: explosive events, UV bursts, and network jets |
title_full_unstemmed |
Observations of small-scale energetic events in the solar transition region: explosive events, UV bursts, and network jets |
title_sort |
observations of small-scale energetic events in the solar transition region: explosive events, uv bursts, and network jets |
publisher |
INFRA-M |
series |
Solar-Terrestrial Physics |
issn |
2500-0535 |
publishDate |
2019-06-01 |
description |
In this paper, we review observational aspects of three common small-scale energetic events in the solar transition region (TR), namely TR explosive events, ultraviolet bursts and jets. These events are defined in either (both) spectral or (and) imaging data. The development of multiple instruments capable of observing the TR has allowed researchers to gain numerous insights into these phenomena in recent years. These events have provided a proxy to study how mass and energy are transported between the solar chromosphere and the corona. As the physical mechanisms responsible for these small-scale events might be similar to the mechanisms responsible for large-scale phenomena, such as flares and coronal mass ejections, analysis of these events could also help our understanding of the solar atmosphere from small to large scales. The observations of these small-scale energetic events demonstrate that the TR is extremely dynamic and is a crucial layer in the solar atmosphere between the chromosphere and the corona. |
topic |
transition region magnetic reconnection small-scale dynamics spectroscopic observations |
url |
https://naukaru.ru/en/nauka/article/29507/view |
work_keys_str_mv |
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1725956942197686272 |