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Solar Active Region Evolution Comparing Models With Observations: Comparing Models With Observations Proceedings of Fourteenth International Summer Workshop, National Solar Observ Book

Solar Active Region Evolution Comparing Models With Observations: Comparing Models With Observations  Proceedings of Fourteenth International Summer Workshop, National Solar Observ
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Solar Active Region Evolution Comparing Models With Observations: Comparing Models With Observations Proceedings of Fourteenth International Summer Workshop, National Solar Observ, , Solar Active Region Evolution Comparing Models With Observations: Comparing Models With Observations Proceedings of Fourteenth International Summer Workshop, National Solar Observatory/Sacramento Peak, Sunspot, new
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  • Solar Active Region Evolution Comparing Models With Observations: Comparing Models With Observations Proceedings of Fourteenth International Summer Workshop, National Solar Observatory/Sacramento Peak, Sunspot, new
  • Written by author K. S. Balasubramaniam, George W. Simon, National Solar Observatory, Sacramento Peak Summer Workshop 1993 Sunsp, Balasuba
  • Published by Astronomical Society of the Pacific, The, 6/1/1994
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Authors

Preface
Workshop Participants
Group Photograph
Active Regions on the Sun 1
Latitude Dependence of Solar Activity From a Statistical Study of Flares from 1938 to 1992 17
Wavelet Analysis of Active Regions 24
Volume Reconstruction of Magnetic Fields using Solar Imagery 30
RISE/PSPT as an Experiment to Study Active Region Irradiance and Luminosity Evolution 37
Solar Irradiance and Luminosity Variations from Active Regions 43
Movies of and Comments on the Organization of Flows and Fields in Active Regions 44
Modeling Solar Magnetoconvection 45
Three-Dimensional Compressible Magnetoconvection 56
A Study of Small Scale Features in Compressible Magnetoconvection 62
Downflow Plumes in the Solar Convection Zone 69
A Possible Siphon Flow Associated with Emergence of New Flux 75
Long-Lived Convective Flows in Quiet and Active Regions 78
Kinematic Modeling of Magnetic Field Diffusion at the Solar Surface 87
Solar Magnetic Elements: Models Compared with Observations 96
Production of Magnetic Flux Bundles For Solar Activity By Cascade of Energy in Global Torsional MHD Waves 102
Convective Turbulence and Mixing in Penetrative Convection 107
Convection and Magnetic Fields 108
Models of Rising Active Region Flux Tubes 109
Dynamics of Flux Tube Ensembles 118
Direct Measurements of Fluxtube Inclinations in Plages 131
Emerging Flux Tube Geometry and Sunspot Proper Motions 138
Evidence for Twisted Emerging Flux in NOAA AR 7260 145
Time-Dependent Petschek-Type Reconnection Model for Solar Flares 149
Dynamics of Small Flux Tubes 157
Role of Electric Currents in Magnetic Flux Tube Physics 158
Electric Current Systems in Solar Active Regions 171
Current Filaments Induced in a Resistive Corona by Continuous Footpoint Motions 180
Magnetic Coronal Heating and Global Restructuring of the Coronal Magnetic Field by Reconnective Relaxation 194
Motions of Loops and Ribbons of Two-Ribbon Flares 202
Numerical Simulations of Magnetic Reconnection in 3-D 210
The Generation of Solar Magnetic Activity 211
The Asymptotic Behavior of Force-Free Magnetic-Field Configurations 219
Deducing Coronal Magnetic Fields from Vector Magnetograms 225
Photospheric Magnetic Field Measurement Errors and the Inferred Properties of Coronal Magnetic Fields 233
A Method for Reconstructing the Coronal Magnetic Field from Vector Magnetograph Measurements at the Photosphere 240
Magnetic Configuration of a Short-Lived Delta Spot 244
Evolution and Disruption of Magnetic Arcades 251
On the Role of Separatrices and Separators of Coronal Magnetic Fields in Solar Flares 258
Simultaneous Filter and Spectrograph Observations of Active Regions with the Advanced Stokes Polarimeter 262
Active Region Development: Results from the JHU/APL Vector Magnetograph 263
Observational Criteria for Filament Models 264
Observations of Active Region Dynamics: Preflare Flows and Field Observations 265
Observations of Flows around Sunspot Groups 283
Flow Patterns in Active Regions 286
Magnetic Field Strength and Filling Factor Sensitivity of the MgI 12 [mu]m Infrared Lines in Solar Plage 294
An Analytical Model for Fluted Sunspots, and its Relation with Evershed Flow and X-Ray Anemone 300
Integrated Force-Balance Equations for the Magnetic Field in Spherical Geometry 307
The Discrete Nature of the Variable Emission in Active Region Loops 314
Structures in Transition Region Plasma of Active Regions 321
The NIXT and SWATH Experiments 329
Are Flares Necessary? 335
Rapid Sunspot Motion Associated with Large Solar Flares 336
A Correlation Between Sunspot Whirls and Filament Type 337
Magnetic Reconnection in the Solar Corona 338
Coronal Structures in Active Regions: Quantitative Results from Multi-Wavelength Observations and Comparisons with Models 356
A Multiband Study of Radio Emission from Solar Active Regions 369
Are X-Ray Bright Points the Signature of Magnetic Field Reconnection? 377
Analysis of Chromospheric Proxies of Coronal Bright Points 389
A Study of Active Region Magnetic Fields Using Radio, X-ray and Optical Observations 395
Magnetic Field Observations of Active Region Prominences 403
Can Coronal Magnetic Structures be Quasi-Static? 409
Filament Tether Cutting Before a Major Eruptive Flare 411
Small-Scale Brightening Events in H[alpha] and Soft X-rays in Active Regions 412
Comments and Perspectives 413
Author Index 420


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