Twin Null-Point-Associated Major Eruptive Three-Ribbon Flares with Unusual Microwave Spectra
On 23 July 2016 after 05:00 UTC, the first 48-antenna stage of the Siberian Radioheliograph detected two flares, M7.6 and M5.5, which occurred within half an hour in the same active region. Their multi-instrument analysis reveals the following. The microwave spectra were flattened at low frequencies...
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| Published in: | Solar physics Vol. 295; no. 9 |
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| Main Authors: | , , , , , , , , , |
| Format: | Journal Article |
| Language: | English |
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01-09-2020
Springer Nature B.V |
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| Abstract | On 23 July 2016 after 05:00 UTC, the first 48-antenna stage of the Siberian Radioheliograph detected two flares, M7.6 and M5.5, which occurred within half an hour in the same active region. Their multi-instrument analysis reveals the following. The microwave spectra were flattened at low frequencies and the spectrum of the stronger burst had a lower turnover frequency. Each flare was eruptive, emitted hard X-rays and
γ
-rays exceeding 800 keV, and had a rare three-ribbon configuration. An extended hard X-ray source associated with a longest middle ribbon was observed in the second flare. Unusual properties of the microwave spectra are accounted for by a distributed multi-loop system in an asymmetric magnetic configuration that our modeling supports. Microwave images did not resolve compact configurations in these flares, which may also be revealed incompletely in hard X-ray images because of their limited dynamic range. Being apparently simple and compact, non-thermal sources corresponded to the structures observed in the extreme ultraviolet. In the scenario proposed for two successive eruptive flares in a configuration with a coronal magnetic null, the first filament eruption causes a flare and facilitates the second eruption that also results in a flare. Three persistent flare ribbons reflect magnetic reconnection at the coronal-null region forced by the filament motions. |
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| AbstractList | On 23 July 2016 after 05:00 UTC, the first 48-antenna stage of the Siberian Radioheliograph detected two flares, M7.6 and M5.5, which occurred within half an hour in the same active region. Their multi-instrument analysis reveals the following. The microwave spectra were flattened at low frequencies and the spectrum of the stronger burst had a lower turnover frequency. Each flare was eruptive, emitted hard X-rays and
γ
-rays exceeding 800 keV, and had a rare three-ribbon configuration. An extended hard X-ray source associated with a longest middle ribbon was observed in the second flare. Unusual properties of the microwave spectra are accounted for by a distributed multi-loop system in an asymmetric magnetic configuration that our modeling supports. Microwave images did not resolve compact configurations in these flares, which may also be revealed incompletely in hard X-ray images because of their limited dynamic range. Being apparently simple and compact, non-thermal sources corresponded to the structures observed in the extreme ultraviolet. In the scenario proposed for two successive eruptive flares in a configuration with a coronal magnetic null, the first filament eruption causes a flare and facilitates the second eruption that also results in a flare. Three persistent flare ribbons reflect magnetic reconnection at the coronal-null region forced by the filament motions. On 23 July 2016 after 05:00 UTC, the first 48-antenna stage of the Siberian Radioheliograph detected two flares, M7.6 and M5.5, which occurred within half an hour in the same active region. Their multi-instrument analysis reveals the following. The microwave spectra were flattened at low frequencies and the spectrum of the stronger burst had a lower turnover frequency. Each flare was eruptive, emitted hard X-rays and γ-rays exceeding 800 keV, and had a rare three-ribbon configuration. An extended hard X-ray source associated with a longest middle ribbon was observed in the second flare. Unusual properties of the microwave spectra are accounted for by a distributed multi-loop system in an asymmetric magnetic configuration that our modeling supports. Microwave images did not resolve compact configurations in these flares, which may also be revealed incompletely in hard X-ray images because of their limited dynamic range. Being apparently simple and compact, non-thermal sources corresponded to the structures observed in the extreme ultraviolet. In the scenario proposed for two successive eruptive flares in a configuration with a coronal magnetic null, the first filament eruption causes a flare and facilitates the second eruption that also results in a flare. Three persistent flare ribbons reflect magnetic reconnection at the coronal-null region forced by the filament motions. |
| ArticleNumber | 128 |
| Author | Kochanov, A. A. Myshyakov, I. I. Zhdanov, D. A. Globa, M. V. Altyntsev, A. T. Lesovoi, S. V. Kiselev, V. I. Uralov, A. M. Meshalkina, N. S. Grechnev, V. V. |
| Author_xml | – sequence: 1 givenname: V. V. orcidid: 0000-0001-5308-6336 surname: Grechnev fullname: Grechnev, V. V. email: grechnev@iszf.irk.ru organization: Institute of Solar-Terrestrial Physics SB RAS – sequence: 2 givenname: N. S. surname: Meshalkina fullname: Meshalkina, N. S. organization: Institute of Solar-Terrestrial Physics SB RAS – sequence: 3 givenname: A. M. surname: Uralov fullname: Uralov, A. M. organization: Institute of Solar-Terrestrial Physics SB RAS – sequence: 4 givenname: A. A. orcidid: 0000-0002-8079-1310 surname: Kochanov fullname: Kochanov, A. A. organization: Institute of Solar-Terrestrial Physics SB RAS – sequence: 5 givenname: S. V. surname: Lesovoi fullname: Lesovoi, S. V. organization: Institute of Solar-Terrestrial Physics SB RAS – sequence: 6 givenname: I. I. orcidid: 0000-0002-8530-7030 surname: Myshyakov fullname: Myshyakov, I. I. organization: Institute of Solar-Terrestrial Physics SB RAS – sequence: 7 givenname: V. I. surname: Kiselev fullname: Kiselev, V. I. organization: Institute of Solar-Terrestrial Physics SB RAS – sequence: 8 givenname: D. A. surname: Zhdanov fullname: Zhdanov, D. A. organization: Institute of Solar-Terrestrial Physics SB RAS – sequence: 9 givenname: A. T. surname: Altyntsev fullname: Altyntsev, A. T. organization: Institute of Solar-Terrestrial Physics SB RAS – sequence: 10 givenname: M. V. surname: Globa fullname: Globa, M. V. organization: Institute of Solar-Terrestrial Physics SB RAS |
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| Keywords | Prominences, active Magnetic reconnection Radio bursts X-ray bursts Magnetic fields Flares |
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| Snippet | On 23 July 2016 after 05:00 UTC, the first 48-antenna stage of the Siberian Radioheliograph detected two flares, M7.6 and M5.5, which occurred within half an... |
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| SubjectTerms | Astrophysics and Astroparticles Atmospheric Sciences Configurations Flares Hard X-rays Magnetic reconnection Microwave spectra Physics Physics and Astronomy Solar physics Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics X ray sources X-rays |
| Title | Twin Null-Point-Associated Major Eruptive Three-Ribbon Flares with Unusual Microwave Spectra |
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