These are the proceedings of the conference on Magnetic Coupling between the Interior and the Atmosphere of the Sun held December 2-5, 2008, which was planned to coincide with the centenary of the discovery of the Evershed effect at Kodaikanal in 1909.
The aim of this meeting was to bring a critical focus to the comprehensive understanding of the important issues pertaining to solar magnetism, with particular emphasis on the various MHD processes that operate in the solar atmosphere. The participants reviewed the current status of magnetic field measurements and their implications with regard to recent theories and numerical models that address the fundamental scales and processes in the highly magnetized, turbulent plasma. The conference also provided a platform for in-depth discussions of new results from various space missions, as well as a comparison with ground-based observing facilities such as the Swedish 1-m Solar Telescope.

lgli/F:\Library.nu\79\_102578.795a23238eaa4c4bda190c5248a2d516.pdf

lgrsnf/F:\Library.nu\79\_102578.795a23238eaa4c4bda190c5248a2d516.pdf

nexusstc/Magnetic Coupling between the Interior and Atmosphere of the Sun/795a23238eaa4c4bda190c5248a2d516.pdf

scihub/10.1007/978-3-642-02859-5.pdf

zlib/Astronomy/S. S. Hasan (auth.), S. Hasan, R. J. Rutten (eds.)/Magnetic Coupling between the Interior and Atmosphere of the Sun_836961.pdf

Magnetic coupling between the interior and atmosphere of the sun proceedings of the Conference "Centenary Commemoration of the Discovery of the Evershed Effect", December 2 - 5, 2008, Indian Institute of Astrophysics, Bangalore, India

Magnetic Coupling between the Interior and Atmosphere of the Sun (Astrophysics and Space Science Proceedings)

S. S Hasan; Indian Institute of Astrophysics; Conference Centenary Commemoration of the Discovery of the Evershed Effect

S. S Hasan; Robert J Rutten; Indian Institute of Astrophysics

edited by S. Hasan, R.J. Rutten

RJ Rutten;SS Hasan

Spektrum Akademischer Verlag. in Springer-Verlag GmbH

Steinkopff. in Springer-Verlag GmbH

Acta Neurologica Scandinavica

Astrophysics and space science proceedings, Berlin, New York, Germany, 2010

Astrophysics and space science proceedings, Heidelberg, ©2010

Springer Nature, Berlin, Heidelberg, 2010

Suppl 81, Vol.63

Germany, Germany

до 2011-01

sm22771789

producers:
Adobe Acrobat Pro 9.0.0

{"container_title":"Astrophysics and Space Science Proceedings","edition":"1","isbns":["3642028586","3642028594","9783642028588","9783642028595"],"issns":["1570-6591","1570-6605"],"last_page":538,"publisher":"Springer","series":"Astrophysics and Space Science Proceedings"}

类型: 期刊

作者及作者单位: RJ Rutten;SS Hasan

期刊名: Acta Neurologica Scandinavica

年份: 1981

卷号: Vol.63

期号: Suppl 81

页码: P20

摘要: ... centenary of the discovery of the Evershed effect at Kodaikanal in 1909 The aim of this meeting was...

Conference proceedings.
Includes bibliographical references and index.

Front Matter....Pages i-xxiii
Front Matter....Pages 1-1
Republication of: Radial Movement in Sunspots....Pages 2-9
Opening Remarks....Pages 10-11
Solar Physics at the Kodaikanal Observatory: A Historical Perspective....Pages 12-36
Vainu Bappu Memorial Lecture: What is a Sunspot?....Pages 37-66
Front Matter....Pages 67-67
Angular-Momentum Coupling Through the Tachocline....Pages 68-85
Outstanding Issues in Solar Dynamo Theory....Pages 86-95
Status of 3D MHD Models of Solar Global Internal Dynamics....Pages 96-100
Measuring the Hidden Aspects of Solar Magnetism....Pages 101-117
Recent Advances in Chromospheric and Coronal Polarization Diagnostics....Pages 118-140
Probability Density Functions to Represent Magnetic Fields at the Solar Surface....Pages 141-149
Spectropolarimetry with CRISP at the Swedish 1-m Solar Telescope....Pages 150-155
Spectropolarimetry with the NLST....Pages 156-165
Magnetic Coupling in the Quiet Solar Atmosphere....Pages 166-185
The Evershed Effect with SOT/Hinode....Pages 186-192
The Evershed Flow and the Brightness of the Penumbra....Pages 193-209
A Topology for the Penumbral Magnetic Fields....Pages 210-228
Theoretical Models of Sunspot Structure and Dynamics....Pages 229-242
Convection and the Origin of Evershed Flows....Pages 243-254
The Magnetic Field of Solar Spicules....Pages 255-260
Three-Dimensional Magnetic Reconnection....Pages 261-276
Front Matter....Pages 67-67
Signatures of Coronal Heating Mechanisms....Pages 277-280
Waves in Polar Coronal Holes....Pages 281-286
MHD Wave Heating Diagnostics....Pages 287-288
Coronal Mass Ejections from Sunspot and Non-Sunspot Regions....Pages 289-307
CME Observations from STEREO....Pages 308-317
Low-Frequency Radio Observations of Coronal Magnetic Fields....Pages 318-323
Evolution of Near-Sun Solar Wind Turbulence....Pages 324-331
The Solar-Stellar Connection....Pages 332-345
Summary and Perspective....Pages 346-355
Front Matter....Pages 356-356
Evidence for Return Meridional Flows in the Convection Zone....Pages 357-360
Long-Term Variations in Meridional Flows....Pages 361-363
Low-Degree High-Frequency p and g Modes in the Solar Core....Pages 364-367
Interior and Exterior Clues of Solar Activity....Pages 368-373
Do Active Regions Modify Oscillation Frequencies?....Pages 374-377
Deep-Focus Diagnostics of Sunspot Structure....Pages 378-385
Are Polar Faculae Generated by a Local Dynamo?....Pages 386-389
The Hanle Effect as Diagnostic Tool for Turbulent Magnetic Fields....Pages 390-394
Phase III of the USO Solar Vector Magnetograph....Pages 395-397
Revisit of the Classic Wilson Effect....Pages 398-401
The Waldmeier Effect in Sunspot Cycles....Pages 402-404
Front Matter....Pages 356-356
Flare-Driven Acoustic Modes in the Sun....Pages 405-409
Dynamics of Active Regions Revealed by Tracking of Doppler Features....Pages 410-412
The Growth of a Primitive Penumbra....Pages 413-416
Evershed Flow Velocities During 100 Years....Pages 417-420
The Thermal Structure of Sunspots....Pages 421-423
Bright Points in G-Band and Ca IIH Images from Hinode....Pages 424-425
Waves in the Transition Region....Pages 426-428
Viscous Damping of Alfvén Surface Waves with Steady Flows....Pages 429-432
Statistical Detection of Propagating Waves in a Polar Coronal Hole....Pages 433-436
Network Loop Oscillations with EIS/Hinode....Pages 437-439
Dynamical Evolution of X-Ray Bright Points with Hinode/XRT....Pages 440-442
Helicity at Photospheric and Chromospheric Heights....Pages 443-447
Evolution of Coronal Helicity in a Twisted Emerging Active Region....Pages 448-451
Power-Law Nanoflare Heating....Pages 452-453
Spectroscopic Diagnostics of Polar Coronal Plumes....Pages 454-458
A Flaring Polar Filament....Pages 459-462
Solar X-Ray Processes....Pages 463-464
Time-Varying Thermal Emission in Solar Flares....Pages 465-470
Multi-Wavelength View of Flare Events on 20 November 2003....Pages 471-474
Time-Delay Between Solar Soft X-Ray and EUV Flare Emissions....Pages 475-477
Front Matter....Pages 356-356
Major Surge Activity of Super-Active Region NOAA 10484....Pages 478-481
Coronal Magnetic Field Estimation Using Type-II Radio Bursts....Pages 482-484
Acceleration of CMEs Associated with Eruptive Prominences....Pages 485-488
Interplanetary Consequences of a Large CME....Pages 489-493
Solar System Resonances on Light-Travel Time Scales Set Up before Proto-Sun’s Nuclear Ignition....Pages 494-496
Front Matter....Pages 497-497
Cycle Prediction from Dynamo Theory....Pages 498-499
Why Does the Torsional Oscillation Precede the Sunspot Cycle?....Pages 500-501
The Subsurface Magnetic Structure of Solar Active Regions....Pages 502-503
Sunspot Magnetometry from Kodaikanal....Pages 504-504
Vector Magnetic Field in Emerging Flux Regions....Pages 505-506
Evolution of Umbral Dots and Penumbral Grains....Pages 507-508
Strong, Localized Downflows in a Sunspot Light Bridge....Pages 509-509
Small-Scale Velocities in Sunspot Penumbrae....Pages 510-510
Photospheric Temperatures from Ca IIH....Pages 511-512
Dual-Line Spectral Imaging of the Chromosphere....Pages 513-514
Inversions of High-Cadence SOLIS-VSM Stokes Observations....Pages 515-515
Flows in Flaring and Dormant Active Regions....Pages 516-516
Magnetic and Velocity Field Changes Related to the Solar Flares of 28 and 29 October 2003....Pages 517-517
A Numerical Investigation of Unsheared Flux Cancelation....Pages 518-519
Wave Heating of Coronal Loops with Steady Flows....Pages 520-520
Front Matter....Pages 497-497
Damping of Prominence Oscillations in Steady Equilibrium....Pages 521-521
Variation of Network Contrast with Height....Pages 522-522
A Flaring Twisted Emerging Flux Region....Pages 523-524
Evidence of Magnetic Reconnection Outflows in a Flare seen by Hinode/EIS....Pages 525-525
Does Coronal Rotation Period Depend on the Sunspot Number?....Pages 526-528
Coronal Magnetic Field from an Extreme Radio Burst....Pages 529-529
CME Kinematics and Dynamics....Pages 530-530
Solar Wind Monitoring with SWIM-SARA Onboard Chandrayaan-1....Pages 531-532
Coupling of the Solar Wind and the Magnetosphere....Pages 533-534
The FIP Effect in RV Tauri Stars....Pages 535-535
Back Matter....Pages 536-538

Solar physics in India has a tradition that can be traced to the setting up of the Kodaikanal Observatory in 1899 when the Madras Observatory was relocated to a high altitude site with a view to initiate observations of the sun. This conference on Magnetic Coupling between the Interior and the Atmosphere of the Sun during 2–5 December 2008 was planned to coincide with centenary of the Evershed effect discovery at Kodaikanal in 1909. The aim of this meeting was to bring to a critical focus a comprehensive - derstanding of the important issues pertaining to solar magnetism with particular emphasis on the various MHD processes that operate in the solar atmosphere. The current status of magnetic eld measurements and their implications in the light of recenttheoriesandnumericalmodelingthataddressthe fundamentalscalesandp- cessesinthehighlymagnetizedturbulentplasmawerereviewedduringthismeeting. The meeting was timely for the following reasons: Space observations such as from SOHO and TRACE have provided a wealth of multiwavelength observations onprocessesoccurringinregionsofthe atmosphereextendingfromthe photosphere up to the outer corona. With the launch of Hinode and STEREO in 2006 and of SDO (Solar Dynamics Observatory) shortly, this conference provided a platform for in-depth discussions on new results from various space missions as well as a comparison with ground-based observing facilities such as the Swedish 1-m Solar Telescope. Using sophisticated image processing techniques, such telescopes r- tinelygenerateobservationswitharesolutionbetterthan0. 1arcsec,therebyyielding more informative diagnostics for instance of the microstructure of ux tubes.

2011-06-04