Transverse Oscillation of Prominence and Filament Induced by an Extreme-ultraviolet Wave from the Far Side of the Sun
In this paper, we report our multi-angle observations of the transverse oscillation of a prominence and a filament induced by an EUV wave originating from the far side of the Sun on 2014 September 1. The prominence oscillation was simultaneously observed by both the Atmospheric Imaging Assembly on b...
| Main Authors: | , , , |
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| Format: | Article |
| Language: | English |
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IOP Publishing
2024-01-01
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| Series: | The Astrophysical Journal |
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| Online Access: | https://doi.org/10.3847/1538-4357/ad206d |
| _version_ | 1797271102856101888 |
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| author | Yanjie Zhang Qingmin Zhang De-chao Song Haisheng Ji |
| author_facet | Yanjie Zhang Qingmin Zhang De-chao Song Haisheng Ji |
| author_sort | Yanjie Zhang |
| collection | DOAJ |
| description | In this paper, we report our multi-angle observations of the transverse oscillation of a prominence and a filament induced by an EUV wave originating from the far side of the Sun on 2014 September 1. The prominence oscillation was simultaneously observed by both the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory spacecraft and the Extreme-UltraViolet Imager on board the Behind Solar Terrestrial Relations Observatory spacecraft. The speed of the shock traveling in interplanetary space exceeds that of the EUV wave, and the coronal dimming area experiences minimal growth. This indicates that the shock wave is driven by the CME, while the EUV wave freely propagates after the lateral motion of the CME flanks has stopped. The observed oscillation direction of the prominence, determined through three-dimensional reconstruction, further supports this point. Moreover, detailed investigation of the oscillations in the prominence and filament induced by the EUV wave reveals initial amplitudes of 16.08 and 2.15 Mm, periods of 1769 and 1863 s, damping timescales of 2640 and 1259 s, and damping ratios of 1.49 and 0.68, respectively. The radial component of the magnetic field, as derived from the prominence and filament oscillation measurements, was estimated to be 5.4 and 4.1 G, respectively. In turn, utilizing the onset times of both the prominence and filament oscillation, the average speeds of the EUV wave are determined to be 498 and 451 km s ^−1 , respectively. |
| first_indexed | 2024-04-25T02:14:50Z |
| format | Article |
| id | doaj.art-4ca00bc9d31942508321cc16ea240164 |
| institution | Directory Open Access Journal |
| issn | 1538-4357 |
| language | English |
| last_indexed | 2024-04-25T02:14:50Z |
| publishDate | 2024-01-01 |
| publisher | IOP Publishing |
| record_format | Article |
| series | The Astrophysical Journal |
| spelling | doaj.art-4ca00bc9d31942508321cc16ea2401642024-03-07T10:03:33ZengIOP PublishingThe Astrophysical Journal1538-43572024-01-01963214010.3847/1538-4357/ad206dTransverse Oscillation of Prominence and Filament Induced by an Extreme-ultraviolet Wave from the Far Side of the SunYanjie Zhang0https://orcid.org/0000-0003-1979-9863Qingmin Zhang1https://orcid.org/0000-0003-4078-2265De-chao Song2https://orcid.org/0000-0003-0057-6766Haisheng Ji3https://orcid.org/0000-0002-5898-2284Key Laboratory of Dark Matter and Space Astronomy , Purple Mountain Observatory, CAS, Nanjing 210023, People's Republic of China ; zhangyj@pmo.ac.cnKey Laboratory of Dark Matter and Space Astronomy , Purple Mountain Observatory, CAS, Nanjing 210023, People's Republic of China ; zhangyj@pmo.ac.cn; Yunnan Key Laboratory of Solar physics and Space Science , Kunming 650216, People's Republic of ChinaKey Laboratory of Dark Matter and Space Astronomy , Purple Mountain Observatory, CAS, Nanjing 210023, People's Republic of China ; zhangyj@pmo.ac.cnKey Laboratory of Dark Matter and Space Astronomy , Purple Mountain Observatory, CAS, Nanjing 210023, People's Republic of China ; zhangyj@pmo.ac.cnIn this paper, we report our multi-angle observations of the transverse oscillation of a prominence and a filament induced by an EUV wave originating from the far side of the Sun on 2014 September 1. The prominence oscillation was simultaneously observed by both the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory spacecraft and the Extreme-UltraViolet Imager on board the Behind Solar Terrestrial Relations Observatory spacecraft. The speed of the shock traveling in interplanetary space exceeds that of the EUV wave, and the coronal dimming area experiences minimal growth. This indicates that the shock wave is driven by the CME, while the EUV wave freely propagates after the lateral motion of the CME flanks has stopped. The observed oscillation direction of the prominence, determined through three-dimensional reconstruction, further supports this point. Moreover, detailed investigation of the oscillations in the prominence and filament induced by the EUV wave reveals initial amplitudes of 16.08 and 2.15 Mm, periods of 1769 and 1863 s, damping timescales of 2640 and 1259 s, and damping ratios of 1.49 and 0.68, respectively. The radial component of the magnetic field, as derived from the prominence and filament oscillation measurements, was estimated to be 5.4 and 4.1 G, respectively. In turn, utilizing the onset times of both the prominence and filament oscillation, the average speeds of the EUV wave are determined to be 498 and 451 km s ^−1 , respectively.https://doi.org/10.3847/1538-4357/ad206dSolar flaresSolar coronal mass ejectionsSolar prominences |
| spellingShingle | Yanjie Zhang Qingmin Zhang De-chao Song Haisheng Ji Transverse Oscillation of Prominence and Filament Induced by an Extreme-ultraviolet Wave from the Far Side of the Sun The Astrophysical Journal Solar flares Solar coronal mass ejections Solar prominences |
| title | Transverse Oscillation of Prominence and Filament Induced by an Extreme-ultraviolet Wave from the Far Side of the Sun |
| title_full | Transverse Oscillation of Prominence and Filament Induced by an Extreme-ultraviolet Wave from the Far Side of the Sun |
| title_fullStr | Transverse Oscillation of Prominence and Filament Induced by an Extreme-ultraviolet Wave from the Far Side of the Sun |
| title_full_unstemmed | Transverse Oscillation of Prominence and Filament Induced by an Extreme-ultraviolet Wave from the Far Side of the Sun |
| title_short | Transverse Oscillation of Prominence and Filament Induced by an Extreme-ultraviolet Wave from the Far Side of the Sun |
| title_sort | transverse oscillation of prominence and filament induced by an extreme ultraviolet wave from the far side of the sun |
| topic | Solar flares Solar coronal mass ejections Solar prominences |
| url | https://doi.org/10.3847/1538-4357/ad206d |
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