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...

Full description

Bibliographic Details
Main Authors: Zhenghua Huang, Bo Li, Lidong Xia
Format: Article
Language:English
Published: INFRA-M 2019-06-01
Series:Solar-Terrestrial Physics
Subjects:
Online Access:https://naukaru.ru/en/nauka/article/29507/view
id doaj-f49a437b363245f1950c217cb3c2837f
record_format Article
spelling 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 AT zhenghuahuang observationsofsmallscaleenergeticeventsinthesolartransitionregionexplosiveeventsuvburstsandnetworkjets
AT boli observationsofsmallscaleenergeticeventsinthesolartransitionregionexplosiveeventsuvburstsandnetworkjets
AT lidongxia observationsofsmallscaleenergeticeventsinthesolartransitionregionexplosiveeventsuvburstsandnetworkjets
_version_ 1725956942197686272