Calcium Bright Knots and the Formation of Chromospheric Anemone Jets on the Sun

Space-based observations show that the solar atmosphere from the solar chromosphere to the solar corona is filled with small-scale jets and is linked with small-scale explosions. These jets may be produced by mechanisms similar to those of large-scale flares and such jets may be related to the heati...
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Autor*in:	Kunwar Alkendra Pratap Singh [verfasserIn] Keisuke Nishida [verfasserIn] Kazunari Shibata [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2024

Schlagwörter:	Solar chromosphere Solar magnetic reconnection

Übergeordnetes Werk:	In: The Astrophysical Journal Letters - IOP Publishing, 2022, 962(2024), 2, p L35
Übergeordnetes Werk:	volume:962 ; year:2024 ; number:2, p L35

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/2041-8213/ad24e7

Katalog-ID:	DOAJ101416911

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language	English
source	In The Astrophysical Journal Letters 962(2024), 2, p L35 volume:962 year:2024 number:2, p L35
sourceStr	In The Astrophysical Journal Letters 962(2024), 2, p L35 volume:962 year:2024 number:2, p L35
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Solar chromosphere Solar magnetic reconnection Astrophysics
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container_title	The Astrophysical Journal Letters
authorswithroles_txt_mv	Kunwar Alkendra Pratap Singh @@aut@@ Keisuke Nishida @@aut@@ Kazunari Shibata @@aut@@
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callnumber-first	Q - Science
author	Kunwar Alkendra Pratap Singh
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topic_title	QB460-466 Calcium Bright Knots and the Formation of Chromospheric Anemone Jets on the Sun Solar chromosphere Solar magnetic reconnection
topic	misc QB460-466 misc Solar chromosphere misc Solar magnetic reconnection misc Astrophysics
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title	Calcium Bright Knots and the Formation of Chromospheric Anemone Jets on the Sun
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title_sort	calcium bright knots and the formation of chromospheric anemone jets on the sun
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title_auth	Calcium Bright Knots and the Formation of Chromospheric Anemone Jets on the Sun
abstract	Space-based observations show that the solar atmosphere from the solar chromosphere to the solar corona is filled with small-scale jets and is linked with small-scale explosions. These jets may be produced by mechanisms similar to those of large-scale flares and such jets may be related to the heating of the corona and chromosphere as well as the acceleration of solar wind. The chromospheric anemone jets on the Sun remain puzzling because their footpoints (or bright knots) have not been well resolved and the formation process of such enigmatic small-scale jets remains unclear. We propose a new model for chromospheric jets using the 3D magnetohydrodynamic simulations, which show that the continuous, upward rising of small-scale twisted magnetic flux ropes in a magnetized solar chromosphere drives small-scale magnetic reconnection and the launching of several small-scale jets during the evolution of the chromospheric anemone jets. Our new, self-consistent, 3D computer modeling of small-scale, but ever-changing flux rope emergence in the magnetized solar atmosphere is fully consistent with observations and provides a universal mechanism for nanoflare and jet formation.
abstractGer	Space-based observations show that the solar atmosphere from the solar chromosphere to the solar corona is filled with small-scale jets and is linked with small-scale explosions. These jets may be produced by mechanisms similar to those of large-scale flares and such jets may be related to the heating of the corona and chromosphere as well as the acceleration of solar wind. The chromospheric anemone jets on the Sun remain puzzling because their footpoints (or bright knots) have not been well resolved and the formation process of such enigmatic small-scale jets remains unclear. We propose a new model for chromospheric jets using the 3D magnetohydrodynamic simulations, which show that the continuous, upward rising of small-scale twisted magnetic flux ropes in a magnetized solar chromosphere drives small-scale magnetic reconnection and the launching of several small-scale jets during the evolution of the chromospheric anemone jets. Our new, self-consistent, 3D computer modeling of small-scale, but ever-changing flux rope emergence in the magnetized solar atmosphere is fully consistent with observations and provides a universal mechanism for nanoflare and jet formation.
abstract_unstemmed	Space-based observations show that the solar atmosphere from the solar chromosphere to the solar corona is filled with small-scale jets and is linked with small-scale explosions. These jets may be produced by mechanisms similar to those of large-scale flares and such jets may be related to the heating of the corona and chromosphere as well as the acceleration of solar wind. The chromospheric anemone jets on the Sun remain puzzling because their footpoints (or bright knots) have not been well resolved and the formation process of such enigmatic small-scale jets remains unclear. We propose a new model for chromospheric jets using the 3D magnetohydrodynamic simulations, which show that the continuous, upward rising of small-scale twisted magnetic flux ropes in a magnetized solar chromosphere drives small-scale magnetic reconnection and the launching of several small-scale jets during the evolution of the chromospheric anemone jets. Our new, self-consistent, 3D computer modeling of small-scale, but ever-changing flux rope emergence in the magnetized solar atmosphere is fully consistent with observations and provides a universal mechanism for nanoflare and jet formation.
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title_short	Calcium Bright Knots and the Formation of Chromospheric Anemone Jets on the Sun
url	https://doi.org/10.3847/2041-8213/ad24e7 https://doaj.org/article/36df1e032ba94e7c8a2cac39bde178b3 https://doaj.org/toc/2041-8205
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