Magnetic Outbreak Associated with Exploding Granulations

Diagnosing the spatiotemporal pattern of magnetic flux on the Sun is vital for understanding the origin of solar magnetism and activity. Here, we report a new form of flux appearance, magnetic outbreak, using observations with an extremely high spatial resolution of 0.″16 from the 1.6 m Goode Solar...

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Published inAstrophysical journal. Letters Vol. 942; no. 1; p. L3
Main Authors Jin, Chunlan, Zhou, Guiping, Ruan, Guiping, Baildon, T., Cao, Wenda, Wang, Jingxiu
Format Journal Article
LanguageEnglish
Published Austin The American Astronomical Society 01.01.2023
IOP Publishing
Subjects
Fluctuations
Granulation
Magnetic flux
Magnetism
Outbreaks
Solar activity
Solar granulation
Solar magnetic fields
Solar magnetism
Solar observatories
Solar photosphere
Spatial resolution
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Abstract Diagnosing the spatiotemporal pattern of magnetic flux on the Sun is vital for understanding the origin of solar magnetism and activity. Here, we report a new form of flux appearance, magnetic outbreak, using observations with an extremely high spatial resolution of 0.″16 from the 1.6 m Goode Solar Telescope at the Big Bear Solar Observatory. Magnetic outbreak refers to an early growth of unipolar magnetic flux and its later explosion into fragments, in association with plasma upflow and exploding granulations; each individual fragment has flux of 10 16 –10 17 Mx, moving apart with a velocity of 0.5–2.2 km s −1 . The magnetic outbreak takes place in the hecto-Gauss region of pore moats. In this study, we identify six events of magnetic outbreak during 6 hr observations over an approximately 40″ × 40″ field of view. The newly discovered magnetic outbreak might be the first evidence of the long-anticipated convective blowup.
AbstractList Diagnosing the spatiotemporal pattern of magnetic flux on the Sun is vital for understanding the origin of solar magnetism and activity. Here, we report a new form of flux appearance, magnetic outbreak, using observations with an extremely high spatial resolution of 0.″16 from the 1.6 m Goode Solar Telescope at the Big Bear Solar Observatory. Magnetic outbreak refers to an early growth of unipolar magnetic flux and its later explosion into fragments, in association with plasma upflow and exploding granulations; each individual fragment has flux of 10 ^16 –10 ^17 Mx, moving apart with a velocity of 0.5–2.2 km s ^−1 . The magnetic outbreak takes place in the hecto-Gauss region of pore moats. In this study, we identify six events of magnetic outbreak during 6 hr observations over an approximately 40″ × 40″ field of view. The newly discovered magnetic outbreak might be the first evidence of the long-anticipated convective blowup.
Diagnosing the spatiotemporal pattern of magnetic flux on the Sun is vital for understanding the origin of solar magnetism and activity. Here, we report a new form of flux appearance, magnetic outbreak, using observations with an extremely high spatial resolution of 0.″16 from the 1.6 m Goode Solar Telescope at the Big Bear Solar Observatory. Magnetic outbreak refers to an early growth of unipolar magnetic flux and its later explosion into fragments, in association with plasma upflow and exploding granulations; each individual fragment has flux of 1016–1017 Mx, moving apart with a velocity of 0.5–2.2 km s−1. The magnetic outbreak takes place in the hecto-Gauss region of pore moats. In this study, we identify six events of magnetic outbreak during 6 hr observations over an approximately 40″ × 40″ field of view. The newly discovered magnetic outbreak might be the first evidence of the long-anticipated convective blowup.
Diagnosing the spatiotemporal pattern of magnetic flux on the Sun is vital for understanding the origin of solar magnetism and activity. Here, we report a new form of flux appearance, magnetic outbreak, using observations with an extremely high spatial resolution of 0.″16 from the 1.6 m Goode Solar Telescope at the Big Bear Solar Observatory. Magnetic outbreak refers to an early growth of unipolar magnetic flux and its later explosion into fragments, in association with plasma upflow and exploding granulations; each individual fragment has flux of 10 16 –10 17 Mx, moving apart with a velocity of 0.5–2.2 km s −1 . The magnetic outbreak takes place in the hecto-Gauss region of pore moats. In this study, we identify six events of magnetic outbreak during 6 hr observations over an approximately 40″ × 40″ field of view. The newly discovered magnetic outbreak might be the first evidence of the long-anticipated convective blowup.
Author Baildon, T.
Jin, Chunlan
Ruan, Guiping
Wang, Jingxiu
Zhou, Guiping
Cao, Wenda
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Cites_doi 10.1088/0004-637X/724/2/1083
10.1007/BF00150420
10.1088/0004-637X/690/1/279
10.1007/BF00165270
10.1051/0004-6361/201628111
10.1007/s11207-010-9510-y
10.1088/1674-4527/19/5/69
10.3847/2041-8213/aac648
10.1086/367611
10.1007/BF00161349
10.1051/0004-6361/201834628
10.1007/BF00148207
10.1088/0004-637X/720/1/233
10.1051/0004-6361:20021807
10.1038/s41550-017-0085
10.3847/1538-4357/ab917b
10.1007/s11207-011-9834-2
10.1017/S1323358000022852
10.1051/0004-6361/202038132
10.3847/1538-4357/ac37be
10.1007/BF02391657
10.3847/1538-4357/aabba0
10.1051/0004-6361:20077048
10.1007/BF00152912
10.1088/0004-637X/785/2/90
10.1086/183539
10.1086/522922
10.3847/1538-4357/ab18aa
10.1007/s11207-011-9841-3
10.1007/s11207-012-9950-7
10.1117/12.2628741
10.1038/nature01174
10.3847/1538-4365/229/1/3
10.1117/12.925494
10.1002/asna.201011390
10.1007/s11207-017-1225-x
10.1007/BF00150128
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References Centeno (apjlaca97cbib5) 2017; 229
Magara (apjlaca97cbib19) 2003; 586
Harvey (apjlaca97cbib14) 1973; 28
Spruit (apjlaca97cbib33) 1979; 61
Thomas (apjlaca97cbib37) 2002; 420
Wang (apjlaca97cbib38) 2017; 1
Zhang (apjlaca97cbib42) 2003; 399
Goode (apjlaca97cbib10) 2012; 8444
Fischer (apjlaca97cbib8) 2019; 622
November (apjlaca97cbib23) 1981; 245
Li (apjlaca97cbib17) 2019; 876
Schrijver (apjlaca97cbib29) 2000
Sheeley (apjlaca97cbib31) 1969; 9
Shine (apjlaca97cbib32) 2000
Wilson (apjlaca97cbib41) 1989; 8
Guglielmino (apjlaca97cbib12) 2010; 724
Stein (apjlaca97cbib36) 2011; 268
Wang (apjlaca97cbib39) 2012; 278
Cao (apjlaca97cbib3) 2010; 331
Moreno-Insertis (apjlaca97cbib21) 2018; 859
Rempel (apjlaca97cbib25) 2018; 859
Spruit (apjlaca97cbib34) 1987; 110
Jin (apjlaca97cbib16) 2009; 690
Cheung (apjlaca97cbib7) 2007; 467
Pesnell (apjlaca97cbib24) 2012; 275
Cao (apjlaca97cbib4) 2022; 12184
Fisher (apjlaca97cbib9) 2008
Spruit (apjlaca97cbib35) 1979; 62
Lites (apjlaca97cbib18) 2008; 672
Musman (apjlaca97cbib22) 1972; 26
Wilson (apjlaca97cbib40) 1986; 106
Jin (apjlaca97cbib15) 2019; 19
Rempel (apjlaca97cbib26) 2014; 785
Roudier (apjlaca97cbib28) 2016; 590
Scherrer (apjlaca97cbib30) 2012; 275
Cao (apjlaca97cbib2) 2012
Ahn (apjlaca97cbib1) 2016; 47
Gošić (apjlaca97cbib11) 2022; 925
Guglielmino (apjlaca97cbib13) 2020; 896
Cheung (apjlaca97cbib6) 2010; 720
Malherbe (apjlaca97cbib20) 2018; 293
Roudier (apjlaca97cbib27) 2020; 641
References_xml – volume: 724
  start-page: 1083
  year: 2010
  ident: apjlaca97cbib12
  publication-title: ApJ
  doi: 10.1088/0004-637X/724/2/1083
– volume: 61
  start-page: 363
  year: 1979
  ident: apjlaca97cbib33
  publication-title: SoPh
  doi: 10.1007/BF00150420
– volume: 690
  start-page: 279
  year: 2009
  ident: apjlaca97cbib16
  publication-title: ApJ
  doi: 10.1088/0004-637X/690/1/279
– volume: 26
  start-page: 290
  year: 1972
  ident: apjlaca97cbib22
  publication-title: SoPh
  doi: 10.1007/BF00165270
– volume: 590
  start-page: 121
  year: 2016
  ident: apjlaca97cbib28
  publication-title: A&A
  doi: 10.1051/0004-6361/201628111
– volume: 47
  start-page: 207
  year: 2016
  ident: apjlaca97cbib1
  publication-title: SPD Meeting
– volume: 268
  start-page: 271
  year: 2011
  ident: apjlaca97cbib36
  publication-title: SoPh
  doi: 10.1007/s11207-010-9510-y
– volume: 19
  start-page: 69
  year: 2019
  ident: apjlaca97cbib15
  publication-title: RAA
  doi: 10.1088/1674-4527/19/5/69
– volume: 859
  start-page: L26
  year: 2018
  ident: apjlaca97cbib21
  publication-title: ApJL
  doi: 10.3847/2041-8213/aac648
– volume: 586
  start-page: 630
  year: 2003
  ident: apjlaca97cbib19
  publication-title: ApJ
  doi: 10.1086/367611
– start-page: 2038
  year: 2000
  ident: apjlaca97cbib32
– year: 2000
  ident: apjlaca97cbib29
– start-page: 291
  year: 2012
  ident: apjlaca97cbib2
– volume: 106
  start-page: 1
  year: 1986
  ident: apjlaca97cbib40
  publication-title: SoPh
  doi: 10.1007/BF00161349
– volume: 622
  start-page: L12
  year: 2019
  ident: apjlaca97cbib8
  publication-title: A&A
  doi: 10.1051/0004-6361/201834628
– volume: 110
  start-page: 115
  year: 1987
  ident: apjlaca97cbib34
  publication-title: SoPh
  doi: 10.1007/BF00148207
– volume: 720
  start-page: 233
  year: 2010
  ident: apjlaca97cbib6
  publication-title: ApJ
  doi: 10.1088/0004-637X/720/1/233
– volume: 399
  start-page: 755
  year: 2003
  ident: apjlaca97cbib42
  publication-title: A&A
  doi: 10.1051/0004-6361:20021807
– volume: 1
  start-page: 0085
  year: 2017
  ident: apjlaca97cbib38
  publication-title: NatAs
  doi: 10.1038/s41550-017-0085
– volume: 896
  start-page: 62
  year: 2020
  ident: apjlaca97cbib13
  publication-title: ApJ
  doi: 10.3847/1538-4357/ab917b
– volume: 275
  start-page: 207
  year: 2012
  ident: apjlaca97cbib30
  publication-title: SoPh
  doi: 10.1007/s11207-011-9834-2
– volume: 8
  start-page: 32
  year: 1989
  ident: apjlaca97cbib41
  publication-title: PASAu
  doi: 10.1017/S1323358000022852
– volume: 641
  start-page: 50
  year: 2020
  ident: apjlaca97cbib27
  publication-title: A&A
  doi: 10.1051/0004-6361/202038132
– volume: 925
  start-page: 188
  year: 2022
  ident: apjlaca97cbib11
  publication-title: ApJ
  doi: 10.3847/1538-4357/ac37be
– volume: 9
  start-page: 347
  year: 1969
  ident: apjlaca97cbib31
  publication-title: SoPh
  doi: 10.1007/BF02391657
– volume: 859
  start-page: 161
  year: 2018
  ident: apjlaca97cbib25
  publication-title: ApJ
  doi: 10.3847/1538-4357/aabba0
– volume: 467
  start-page: 703
  year: 2007
  ident: apjlaca97cbib7
  publication-title: A&A
  doi: 10.1051/0004-6361:20077048
– volume: 28
  start-page: 61
  year: 1973
  ident: apjlaca97cbib14
  publication-title: SoPh
  doi: 10.1007/BF00152912
– volume: 785
  start-page: 90
  year: 2014
  ident: apjlaca97cbib26
  publication-title: ApJ
  doi: 10.1088/0004-637X/785/2/90
– volume: 245
  start-page: L123
  year: 1981
  ident: apjlaca97cbib23
  publication-title: ApJL
  doi: 10.1086/183539
– volume: 672
  start-page: 1237
  year: 2008
  ident: apjlaca97cbib18
  publication-title: ApJ
  doi: 10.1086/522922
– volume: 876
  start-page: 129
  year: 2019
  ident: apjlaca97cbib17
  publication-title: ApJ
  doi: 10.3847/1538-4357/ab18aa
– volume: 275
  start-page: 3
  year: 2012
  ident: apjlaca97cbib24
  publication-title: SoPh
  doi: 10.1007/s11207-011-9841-3
– volume: 278
  start-page: 299
  year: 2012
  ident: apjlaca97cbib39
  publication-title: SoPh
  doi: 10.1007/s11207-012-9950-7
– volume: 12184
  start-page: 1218428
  year: 2022
  ident: apjlaca97cbib4
  publication-title: Proc. SPIE
  doi: 10.1117/12.2628741
– volume: 420
  start-page: 390
  year: 2002
  ident: apjlaca97cbib37
  publication-title: Natur
  doi: 10.1038/nature01174
– volume: 229
  start-page: 3
  year: 2017
  ident: apjlaca97cbib5
  publication-title: ApJS
  doi: 10.3847/1538-4365/229/1/3
– volume: 8444
  year: 2012
  ident: apjlaca97cbib10
  publication-title: Proc. SPIE
  doi: 10.1117/12.925494
– volume: 331
  start-page: 636
  year: 2010
  ident: apjlaca97cbib3
  publication-title: AN
  doi: 10.1002/asna.201011390
– volume: 293
  start-page: 4
  year: 2018
  ident: apjlaca97cbib20
  publication-title: SoPh
  doi: 10.1007/s11207-017-1225-x
– start-page: 373
  year: 2008
  ident: apjlaca97cbib9
– volume: 62
  start-page: 15
  year: 1979
  ident: apjlaca97cbib35
  publication-title: SoPh
  doi: 10.1007/BF00150128
SSID ssj0020618
Score 2.3822668
Snippet Diagnosing the spatiotemporal pattern of magnetic flux on the Sun is vital for understanding the origin of solar magnetism and activity. Here, we report a new...
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SubjectTerms Fluctuations
Granulation
Magnetic flux
Magnetism
Outbreaks
Solar activity
Solar granulation
Solar magnetic fields
Solar magnetism
Solar observatories
Solar photosphere
Spatial resolution
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Title Magnetic Outbreak Associated with Exploding Granulations
URI https://iopscience.iop.org/article/10.3847/2041-8213/aca97c
https://www.proquest.com/docview/2759037422
https://doaj.org/article/ac83871871774af3b26af9ad3d59e490
Volume 942
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