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Evolution of emerging anti-Hale region and associated eruptive solar flares

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Evolution of emerging anti-Hale region and associated eruptive solar flares


Overview of the solar eruptions in NOAA AR 12882. (a), (b) AIA 335 Å and 211 Å pictures exhibiting the C2.7 and M1.6 flares on 2021 October 8 and 9, respectively. The yellow arrow factors to the primary flaring area. (c), (d) Lasco/C2 and Stereo/COR2 distinction pictures exhibiting the CMEs following the 2 flares, as indicated by two white arrows. (e), (f): HMI continuum depth and line-of-sight magnetogram exhibiting the final configuration of AR 12882. The FOV is indicated by the black field in (b). The flare ribbons are superposed on the HMI magnetogram as yellow contours in (f). Credit score: The Astrophysical Journal Letters (2022). DOI: 10.3847/2041-8213/ac8fef

Dr. Xu Zhe, Prof. Yan Xiaoli and colleagues from the Yunnan Observatories of the Chinese language Academy of Sciences have revealed how an energetic area (AR) evolves, re-configures the higher coronal constructions, and ultimately contributes to solar eruptions. Outcomes have been revealed in The Astrophysical Journal Letters.

Photo voltaic energetic areas hardly ever violate the Hale-Nicholson rule, however as soon as these areas shaped, they are typically flare-productive. Utilizing the joint observations from the New Vacuum Photo voltaic Telescope and the Photo voltaic Dynamics Observatory, the researchers investigated the evolution of an rising anti-Hale area and its related solar flare eruption.

They discovered that in NOAA AR 12882, magnetic vitality and helicity have been equipped to the corona by the brand new emergence and powerful shearing motions of an anti-Hale bipole close to the preexisting sunspot. A magnetic flux rope was shaped concurrently within the upper atmosphere with the ejection of magnetic helicity. The profitable eruptions of this flux rope ultimately produced C-class and M-class flares.

Specifically, a cusp construction was noticed to type close to the post-flare loops, suggesting an interplay between the rising anti-Hale area and the preexisting active region.

Because the researchers declare, the flux emergence in a proximity to an current sunspot and the anti-Hale orientation of a bipole, have been acknowledged as keys to supply robust flares. This AR 12882 internet hosting each traits on the identical time is essential for understanding the origin of solar flares.


Exploring eruptions from the Sun


Extra info:
Zhe Xu et al, Evolution of an Rising Anti-Hale Area and its Related Eruptive Photo voltaic Flares in NOAA AR 12882, The Astrophysical Journal Letters (2022). DOI: 10.3847/2041-8213/ac8fef

Quotation:
Evolution of rising anti-Hale area and related eruptive solar flares (2022, September 28)
retrieved 28 September 2022
from https://phys.org/information/2022-09-evolution-emerging-anti-hale-region-eruptive.html

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