The Role Of Torsional Alfvén Waves in Coronal Heating

In the context of coronal heating, among the zoo of magnetohydrodynamic (MHD) waves that exist in the solar atmosphere, Alfven waves receive special attention. Indeed, these waves constitute an attractive heating agent due to their ability to carry over the many different layers of the solar atmosph...

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Vydáno v:The Astrophysical journal Ročník 712; číslo 1; s. 494 - 510
Hlavní autoři: Antolin, P, Shibata, K
Médium: Journal Article
Jazyk:angličtina
Vydáno: Bristol IOP Publishing 20.03.2010
IOP
Témata:
ABSORPTION
ALFVEN WAVES
Astronomy
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
ATMOSPHERES
Earth, ocean, space
ELECTROMAGNETIC RADIATION
Exact sciences and technology
FLUID MECHANICS
HEATING
HYDRODYNAMICS
HYDROMAGNETIC WAVES
MAGNETIC FIELDS
MAGNETIC FLUX
MAGNETOHYDRODYNAMICS
MAIN SEQUENCE STARS
MECHANICS
MODE CONVERSION
MONOCHROMATIC RADIATION
PHOTOSPHERE
PLASMA HEATING
POLARIMETERS
RADIATIONS
SATELLITES
SHOCK HEATING
SOLAR ATMOSPHERE
SOLAR CORONA
SORPTION
SPECTRA
STARS
STELLAR ATMOSPHERES
STELLAR CORONAE
SUN
TELESCOPES
Collapse
Energetics
Alfven waves
Sun: flares
waves
Solar corona
Magnetic flux
Plasma
Magnetohydrodynamics
Mixing
Critical value
MHD waves
Flux tubes
Sun: corona
Resonant absorption
Sun
Noise spectrum
Shock heating
Hinode satellite
White noise
Solar atmosphere
Models
Magnetic fields
magnetohydrodynamics (MHD)
ISSN:0004-637X, 1538-4357
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Abstract In the context of coronal heating, among the zoo of magnetohydrodynamic (MHD) waves that exist in the solar atmosphere, Alfven waves receive special attention. Indeed, these waves constitute an attractive heating agent due to their ability to carry over the many different layers of the solar atmosphere sufficient energy to heat and maintain a corona. However, due to their incompressible nature these waves need a mechanism such as mode conversion (leading to shock heating), phase mixing, resonant absorption, or turbulent cascade in order to heat the plasma. Furthermore, their incompressibility makes their detection in the solar atmosphere very difficult. New observations with polarimetric, spectroscopic, and imaging instruments such as those on board the Japanese satellite Hinode, or the Crisp spectropolarimeter of the Swedish Solar Telescope or the Coronal Multi-channel Polarimeter, are bringing strong evidence for the existence of energetic Alfven waves in the solar corona. In order to assess the role of Alfven waves in coronal heating, in this work we model a magnetic flux tube being subject to Alfven wave heating through the mode conversion mechanism. Using a 1.5 dimensional MHD code, we carry out a parameter survey varying the magnetic flux tube geometry (length and expansion), the photospheric magnetic field, the photospheric velocity amplitudes, and the nature of the waves (monochromatic or white-noise spectrum). The regimes under which Alfven wave heating produces hot and stable coronae are found to be rather narrow. Independently of the photospheric wave amplitude and magnetic field, a corona can be produced and maintained only for long (>80 Mm) and thick (area ratio between the photosphere and corona >500) loops. Above a critical value of the photospheric velocity amplitude (generally a few km s{sup -1}) the corona can no longer be maintained over extended periods of time and collapses due to the large momentum of the waves. These results establish several constraints on Alfven wave heating as a coronal heating mechanism, especially for active region loops.
AbstractList In the context of coronal heating, among the zoo of magnetohydrodynamic (MHD) waves that exist in the solar atmosphere, Alfven waves receive special attention. Indeed, these waves constitute an attractive heating agent due to their ability to carry over the many different layers of the solar atmosphere sufficient energy to heat and maintain a corona. However, due to their incompressible nature these waves need a mechanism such as mode conversion (leading to shock heating), phase mixing, resonant absorption, or turbulent cascade in order to heat the plasma. Furthermore, their incompressibility makes their detection in the solar atmosphere very difficult. New observations with polarimetric, spectroscopic, and imaging instruments such as those on board the Japanese satellite Hinode, or the Crisp spectropolarimeter of the Swedish Solar Telescope or the Coronal Multi-channel Polarimeter, are bringing strong evidence for the existence of energetic Alfven waves in the solar corona. In order to assess the role of Alfven waves in coronal heating, in this work we model a magnetic flux tube being subject to Alfven wave heating through the mode conversion mechanism. Using a 1.5 dimensional MHD code, we carry out a parameter survey varying the magnetic flux tube geometry (length and expansion), the photospheric magnetic field, the photospheric velocity amplitudes, and the nature of the waves (monochromatic or white-noise spectrum). The regimes under which Alfven wave heating produces hot and stable coronae are found to be rather narrow. Independently of the photospheric wave amplitude and magnetic field, a corona can be produced and maintained only for long (>80 Mm) and thick (area ratio between the photosphere and corona >500) loops. Above a critical value of the photospheric velocity amplitude (generally a few km s{sup -1}) the corona can no longer be maintained over extended periods of time and collapses due to the large momentum of the waves. These results establish several constraints on Alfven wave heating as a coronal heating mechanism, especially for active region loops.
Author Antolin, P
Shibata, K
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Cites_doi 10.1086/156648
10.1086/323788
10.1126/science.1168680
10.1086/381779
10.1086/343123
10.1086/166684
10.1126/science.1153006
10.1038/31166
10.1007/s11207-007-0182-1
10.1007/s11207-007-9029-z
10.1086/309486
10.1007/BF00150014
10.1007/s11214-009-9506-9
10.1086/306930
10.1086/155949
10.1016/0010-4655(91)90071-R
10.1007/BF00149894
10.1051/0004-6361:20031328
10.1086/313064
10.12942/lrsp-2005-3
10.1086/167932
10.1007/BF00619096
10.1086/172559
10.1007/BF00154975
10.1007/s11207-006-0055-z
10.1086/429249
10.1086/167078
10.1086/592226
10.1086/512185
10.1088/0004-637X/696/1/760
10.1086/452630
10.1086/158597
10.1086/304754
10.1086/306804
10.1086/161706
10.1086/191681
10.1088/0004-637X/702/1/1
10.1088/0004-637X/710/2/1857
10.1086/343886
10.1007/BF00151968
10.1029/JA091iA04p04171
10.1029/2005JA011502
10.1007/s11207-007-0400-x
10.1126/science.1143304
10.1002/asna.200710803
10.1086/512776
10.1007/s11214-009-9535-4
10.1051/0004-6361:20030084
10.1007/BF00749277
10.1086/591998
10.1086/518001
10.1086/170015
10.1126/science.1151747
10.1086/588252
10.1086/318055
10.1086/155829
10.1086/323064
10.1086/170435
10.1007/BF00153458
10.1086/306377
10.1086/167212
10.1086/587029
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Issue 1
Keywords Collapse
Energetics
Alfven waves
Sun: flares
waves
Solar corona
Magnetic flux
Plasma
Magnetohydrodynamics
Mixing
Critical value
MHD waves
Flux tubes
Sun: corona
Resonant absorption
Sun
Noise spectrum
Shock heating
Hinode satellite
White noise
Solar atmosphere
Models
Magnetic fields
magnetohydrodynamics (MHD)
Language English
License CC BY 4.0
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References Kudoh (34) 1998; 508
Hori (28) 1997; 489
46
Takeuchi (62) 2001; 546
Yokoyama (75) 1998
48
49
Reale (50) 2002; 580
Van Doorsselaere (69) 2008; 676
Taroyan (63) 2008
Brosius (12) 2007; 656
Moriyasu (40) 2004; 601
51
52
Antolin (4) 2009
Hara (23) 2008; 678
54
11
55
56
57
14
58
59
Cranmer (15) 2007; 171
16
17
Heggland (24) 2009; 702
Matsumoto (37) 2010; 710
Aschwanden (7) 2001; 559
18
Musielak (43) 2007; 659
Williams (73) 2004
Tsuneta (67) 2008; 688
1
Aschwanden (6) 2001; 560
Kudoh (35) 1999; 514
Nakariakov (44) 2005; 2
Aschwanden (10) 2000; 541
60
61
20
64
21
65
22
66
Aschwanden (8) 2004
68
Antolin (5) 2009
26
Patsourakos (47) 2009; 696
27
Verth (70) 2009
29
Kigure (32) 2010
Erdelyi (19) 1995; 294
Ofman (45) 2002; 576
Antolin (3) 2008; 688
Muller (42) 1994; 283
Verth (71) 2010
Aschwanden (9) 2005; 633
72
30
74
Antiochos (2) 1999; 512
31
76
Chae (13) 1998; 114
33
39
Ruderman (53) 1997; 320
Landini (36) 1990; 82
Heyvaerts (25) 1983; 117
Mendoza-Briceño (38) 2005; 624
41
References_xml – ident: 30
  doi: 10.1086/156648
– volume: 559
  start-page: L171
  issn: 1538-4357
  year: 2001
  ident: 7
  publication-title: ApJ
  doi: 10.1086/323788
– ident: 31
  doi: 10.1126/science.1168680
– volume: 601
  start-page: L107
  issn: 1538-4357
  year: 2004
  ident: 40
  publication-title: ApJ
  doi: 10.1086/381779
– volume: 580
  start-page: 566
  issn: 0004-637X
  year: 2002
  ident: 50
  publication-title: ApJ
  doi: 10.1086/343123
– ident: 20
  doi: 10.1086/166684
– start-page: 513
  year: 2004
  ident: 73
  publication-title: SOHO 13, Waves, Oscillations and Small-Scale Transients Events in the Solar Atmosphere: Joint View from SOHO and TRACE
– ident: 18
  doi: 10.1126/science.1153006
– ident: 49
  doi: 10.1038/31166
– ident: 22
  doi: 10.1007/s11207-007-0182-1
– ident: 11
  doi: 10.1007/s11207-007-9029-z
– volume: 541
  start-page: 1059
  issn: 0004-637X
  year: 2000
  ident: 10
  publication-title: ApJ
  doi: 10.1086/309486
– ident: 48
  doi: 10.1007/BF00150014
– volume: 283
  start-page: 232
  issn: 0004-6361
  year: 1994
  ident: 42
  publication-title: A&A
– ident: 64
  doi: 10.1007/s11214-009-9506-9
– volume: 514
  start-page: 493
  issn: 0004-637X
  year: 1999
  ident: 35
  publication-title: ApJ
  doi: 10.1086/306930
– ident: 51
  doi: 10.1086/155949
– year: 2010
  ident: 32
– ident: 74
  doi: 10.1016/0010-4655(91)90071-R
– ident: 29
  doi: 10.1007/BF00149894
– ident: 41
  doi: 10.1051/0004-6361:20031328
– volume: 114
  start-page: 151
  issn: 0067-0049
  year: 1998
  ident: 13
  publication-title: ApJS
  doi: 10.1086/313064
– volume: 2
  start-page: 3
  issn: 1614-4961
  year: 2005
  ident: 44
  publication-title: Living Rev. Sol. Phys.
  doi: 10.12942/lrsp-2005-3
– ident: 56
  doi: 10.1086/167932
– ident: 14
  doi: 10.1007/BF00619096
– ident: 59
  doi: 10.1086/172559
– ident: 72
  doi: 10.1007/BF00154975
– year: 2004
  ident: 8
  publication-title: Physics of the Solar Corona. An Introduction
– ident: 33
  doi: 10.1007/s11207-006-0055-z
– volume: 624
  start-page: 1080
  issn: 0004-637X
  year: 2005
  ident: 38
  publication-title: ApJ
  doi: 10.1086/429249
– ident: 1
  doi: 10.1086/167078
– year: 2009
  ident: 5
– volume: 688
  start-page: 1374
  issn: 0004-637X
  year: 2008
  ident: 67
  publication-title: ApJ
  doi: 10.1086/592226
– volume: 82
  start-page: 229
  issn: 1286-4846
  year: 1990
  ident: 36
  publication-title: A&AS
– volume: 656
  start-page: L41
  issn: 1538-4357
  year: 2007
  ident: 12
  publication-title: ApJ
  doi: 10.1086/512185
– volume: 696
  start-page: 760
  issn: 0004-637X
  year: 2009
  ident: 47
  publication-title: ApJ
  doi: 10.1088/0004-637X/696/1/760
– volume: 633
  start-page: 499
  issn: 0004-637X
  year: 2005
  ident: 9
  publication-title: ApJ
  doi: 10.1086/452630
– volume: 294
  start-page: 575
  issn: 0004-6361
  year: 1995
  ident: 19
  publication-title: A&A
– ident: 55
  doi: 10.1086/158597
– volume: 489
  start-page: 426
  issn: 0004-637X
  year: 1997
  ident: 28
  publication-title: ApJ
  doi: 10.1086/304754
– volume: 512
  start-page: 985
  issn: 0004-637X
  year: 1999
  ident: 2
  publication-title: ApJ
  doi: 10.1086/306804
– ident: 26
  doi: 10.1086/161706
– ident: 60
  doi: 10.1086/191681
– year: 2009
  ident: 70
  publication-title: ApJ
– volume: 320
  start-page: 305
  issn: 0004-6361
  year: 1997
  ident: 53
  publication-title: A&A
– volume: 702
  start-page: 1
  issn: 0004-637X
  year: 2009
  ident: 24
  publication-title: ApJ
  doi: 10.1088/0004-637X/702/1/1
– volume: 710
  start-page: 1857
  issn: 0004-637X
  year: 2010
  ident: 37
  publication-title: ApJ
  doi: 10.1088/0004-637X/710/2/1857
– volume: 576
  start-page: L153
  issn: 1538-4357
  year: 2002
  ident: 45
  publication-title: ApJ
  doi: 10.1086/343886
– ident: 68
  doi: 10.1007/BF00151968
– volume: 117
  start-page: 220
  issn: 0004-6361
  year: 1983
  ident: 25
  publication-title: A&A
– ident: 65
  doi: 10.1029/JA091iA04p04171
– ident: 61
  doi: 10.1029/2005JA011502
– ident: 52
  doi: 10.1007/s11207-007-0400-x
– ident: 66
  doi: 10.1126/science.1143304
– start-page: 184
  year: 2008
  ident: 63
  publication-title: Waves & Oscillations in the Solar Atmosphere: Heating and Magneto-Seismology
– ident: 17
  doi: 10.1002/asna.200710803
– volume: 659
  start-page: 650
  issn: 0004-637X
  year: 2007
  ident: 43
  publication-title: ApJ
  doi: 10.1086/512776
– year: 2010
  ident: 71
  publication-title: ApJ
– ident: 54
  doi: 10.1007/s11214-009-9535-4
– ident: 76
  doi: 10.1051/0004-6361:20030084
– ident: 58
  doi: 10.1007/BF00749277
– volume: 688
  start-page: 669
  issn: 0004-637X
  year: 2008
  ident: 3
  publication-title: ApJ
  doi: 10.1086/591998
– volume: 171
  start-page: 520
  issn: 0067-0049
  year: 2007
  ident: 15
  publication-title: ApJS
  doi: 10.1086/518001
– start-page: 215
  year: 1998
  ident: 75
  publication-title: Solar Jets and Coronal Plumes
– ident: 46
  doi: 10.1086/170015
– ident: 16
  doi: 10.1126/science.1151747
– volume: 678
  start-page: L67
  issn: 1538-4357
  year: 2008
  ident: 23
  publication-title: ApJ
  doi: 10.1086/588252
– year: 2009
  ident: 4
– volume: 546
  start-page: L73
  issn: 1538-4357
  year: 2001
  ident: 62
  publication-title: ApJ
  doi: 10.1086/318055
– ident: 21
  doi: 10.1086/155829
– volume: 560
  start-page: 1035
  issn: 0004-637X
  year: 2001
  ident: 6
  publication-title: ApJ
  doi: 10.1086/323064
– ident: 39
  doi: 10.1086/170435
– ident: 27
  doi: 10.1007/BF00153458
– volume: 508
  start-page: 186
  issn: 0004-637X
  year: 1998
  ident: 34
  publication-title: ApJ
  doi: 10.1086/306377
– ident: 57
  doi: 10.1086/167212
– volume: 676
  start-page: L73
  issn: 1538-4357
  year: 2008
  ident: 69
  publication-title: ApJ
  doi: 10.1086/587029
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Snippet In the context of coronal heating, among the zoo of magnetohydrodynamic (MHD) waves that exist in the solar atmosphere, Alfven waves receive special attention....
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StartPage 494
SubjectTerms ABSORPTION
ALFVEN WAVES
Astronomy
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
ATMOSPHERES
Earth, ocean, space
ELECTROMAGNETIC RADIATION
Exact sciences and technology
FLUID MECHANICS
HEATING
HYDRODYNAMICS
HYDROMAGNETIC WAVES
MAGNETIC FIELDS
MAGNETIC FLUX
MAGNETOHYDRODYNAMICS
MAIN SEQUENCE STARS
MECHANICS
MODE CONVERSION
MONOCHROMATIC RADIATION
PHOTOSPHERE
PLASMA HEATING
POLARIMETERS
RADIATIONS
SATELLITES
SHOCK HEATING
SOLAR ATMOSPHERE
SOLAR CORONA
SORPTION
SPECTRA
STARS
STELLAR ATMOSPHERES
STELLAR CORONAE
SUN
TELESCOPES
Title The Role Of Torsional Alfvén Waves in Coronal Heating
URI http://iopscience.iop.org/0004-637X/712/1/494
https://www.proquest.com/docview/1671245719
https://www.proquest.com/docview/849467168
https://www.osti.gov/biblio/21394251
Volume 712
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