A Blowout Jet Associated with One Obvious Extreme-ultraviolet Wave and One Complicated Coronal Mass Ejection Event
In this paper, we present a detailed analysis of a coronal blowout jet eruption that was associated with an obvious extreme-ultraviolet (EUV) wave and one complicated coronal mass ejection (CME) event based on the multiwavelength and multi-view-angle observations from the Solar Dynamics Observatory...
| Main Authors: | , , , , , , , |
|---|---|
| Format: | Article |
| Published: |
American Astronomical Society
2018
|
| Subjects: |
| _version_ | 1825721659980513280 |
|---|---|
| author | Miao, Yuhu Liu, Yu Li, Hong Bo Shen, Yuan Deng Yang, Shu Hong Elmhamdi, Abouazza Kordi, Ayman S. Abidin, Zamri Zainal |
| author_facet | Miao, Yuhu Liu, Yu Li, Hong Bo Shen, Yuan Deng Yang, Shu Hong Elmhamdi, Abouazza Kordi, Ayman S. Abidin, Zamri Zainal |
| author_sort | Miao, Yuhu |
| collection | UM |
| description | In this paper, we present a detailed analysis of a coronal blowout jet eruption that was associated with an obvious extreme-ultraviolet (EUV) wave and one complicated coronal mass ejection (CME) event based on the multiwavelength and multi-view-angle observations from the Solar Dynamics Observatory and the Solar Terrestrial Relations Observatory. It is found that the triggering of the blowout jet was due to the emergence and cancellation of magnetic fluxes on the photosphere. During the rising stage of the jet, the EUV wave appeared just ahead of the jet top, lasting about 4 minutes and at a speed of 458-762 km s-1. In addition, obvious dark material is observed along the EUV jet body, which confirms the observation of a mini-filament eruption at the jet base in the chromosphere. Interestingly, two distinct but overlapped CME structures can be observed in corona together with the eruption of the blowout jet. One is a narrow jet shape, while the other one is a bubble shape. The jet-shaped component was unambiguously related to the outwardly running jet itself, while the bubble-like one might either be produced due to the reconstruction of the high coronal fields or by the internal reconnection during the mini-filament ejection according to the double-CME blowout jet model first proposed by Shen et al., suggesting more observational evidence should be supplied to clear the current ambiguity based on large samples of blowout jets in future studies. |
| first_indexed | 2024-03-06T05:53:44Z |
| format | Article |
| id | um.eprints-21290 |
| institution | Universiti Malaya |
| last_indexed | 2024-03-06T05:53:44Z |
| publishDate | 2018 |
| publisher | American Astronomical Society |
| record_format | dspace |
| spelling | um.eprints-212902019-05-24T03:31:57Z http://eprints.um.edu.my/21290/ A Blowout Jet Associated with One Obvious Extreme-ultraviolet Wave and One Complicated Coronal Mass Ejection Event Miao, Yuhu Liu, Yu Li, Hong Bo Shen, Yuan Deng Yang, Shu Hong Elmhamdi, Abouazza Kordi, Ayman S. Abidin, Zamri Zainal Q Science (General) QC Physics In this paper, we present a detailed analysis of a coronal blowout jet eruption that was associated with an obvious extreme-ultraviolet (EUV) wave and one complicated coronal mass ejection (CME) event based on the multiwavelength and multi-view-angle observations from the Solar Dynamics Observatory and the Solar Terrestrial Relations Observatory. It is found that the triggering of the blowout jet was due to the emergence and cancellation of magnetic fluxes on the photosphere. During the rising stage of the jet, the EUV wave appeared just ahead of the jet top, lasting about 4 minutes and at a speed of 458-762 km s-1. In addition, obvious dark material is observed along the EUV jet body, which confirms the observation of a mini-filament eruption at the jet base in the chromosphere. Interestingly, two distinct but overlapped CME structures can be observed in corona together with the eruption of the blowout jet. One is a narrow jet shape, while the other one is a bubble shape. The jet-shaped component was unambiguously related to the outwardly running jet itself, while the bubble-like one might either be produced due to the reconstruction of the high coronal fields or by the internal reconnection during the mini-filament ejection according to the double-CME blowout jet model first proposed by Shen et al., suggesting more observational evidence should be supplied to clear the current ambiguity based on large samples of blowout jets in future studies. American Astronomical Society 2018 Article PeerReviewed Miao, Yuhu and Liu, Yu and Li, Hong Bo and Shen, Yuan Deng and Yang, Shu Hong and Elmhamdi, Abouazza and Kordi, Ayman S. and Abidin, Zamri Zainal (2018) A Blowout Jet Associated with One Obvious Extreme-ultraviolet Wave and One Complicated Coronal Mass Ejection Event. The Astrophysical Journal, 869 (1). p. 39. ISSN 0004-637X, DOI https://doi.org/10.3847/1538-4357/aaeac1 <https://doi.org/10.3847/1538-4357/aaeac1>. https://doi.org/10.3847/1538-4357/aaeac1 doi:10.3847/1538-4357/aaeac1 |
| spellingShingle | Q Science (General) QC Physics Miao, Yuhu Liu, Yu Li, Hong Bo Shen, Yuan Deng Yang, Shu Hong Elmhamdi, Abouazza Kordi, Ayman S. Abidin, Zamri Zainal A Blowout Jet Associated with One Obvious Extreme-ultraviolet Wave and One Complicated Coronal Mass Ejection Event |
| title | A Blowout Jet Associated with One Obvious Extreme-ultraviolet Wave and One Complicated Coronal Mass Ejection Event |
| title_full | A Blowout Jet Associated with One Obvious Extreme-ultraviolet Wave and One Complicated Coronal Mass Ejection Event |
| title_fullStr | A Blowout Jet Associated with One Obvious Extreme-ultraviolet Wave and One Complicated Coronal Mass Ejection Event |
| title_full_unstemmed | A Blowout Jet Associated with One Obvious Extreme-ultraviolet Wave and One Complicated Coronal Mass Ejection Event |
| title_short | A Blowout Jet Associated with One Obvious Extreme-ultraviolet Wave and One Complicated Coronal Mass Ejection Event |
| title_sort | blowout jet associated with one obvious extreme ultraviolet wave and one complicated coronal mass ejection event |
| topic | Q Science (General) QC Physics |
| work_keys_str_mv | AT miaoyuhu ablowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent AT liuyu ablowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent AT lihongbo ablowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent AT shenyuandeng ablowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent AT yangshuhong ablowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent AT elmhamdiabouazza ablowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent AT kordiaymans ablowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent AT abidinzamrizainal ablowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent AT miaoyuhu blowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent AT liuyu blowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent AT lihongbo blowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent AT shenyuandeng blowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent AT yangshuhong blowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent AT elmhamdiabouazza blowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent AT kordiaymans blowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent AT abidinzamrizainal blowoutjetassociatedwithoneobviousextremeultravioletwaveandonecomplicatedcoronalmassejectionevent |