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Title: |
Solar-Stellar Dynamos as Revealed by Helio- and Asteroseismology: GONG 2008/SOHO 21
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Volume: |
416
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Year: |
2009
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View this Volume on ADS
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Editors: |
Dikpati, M.; Arentoft, T.; González Hernández, I.; Lindsey, C.; Hill, F.
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Synopsis: |
These proceedings report the latest progress in the fields of helio- and asteroseismology, which use sound waves to probe the interior of stars. Every two years, researchers in these fields convene under the auspices of the Global Oscillation Network Group (GONG) and the Solar and Heliospheric Observatory (SOHO) programs.
This volume contains a total of 102 papers contributed by 107 participants. The proceedings of previous GONG meetings have been published as ASPCS volumes 42 and 76. The focus of this meeting was on what seismology could reveal about the dynamo mechanism underlying solar and stellar activity. The topical sessions included Local Helioseismology; Global Helioseismology; Asteroseismology; Solar Activity: Convection, Tachocline, Dynamo, and Data Assimilation; and Major Observational Programs.
The current solar activity minimum has been unusually deep and lengthy, reminding us how poorly we understand the mechanism underlying stellar activity. Seismology is the only way we can penetrate the surface of a star and probe its interior. Future observational programs, such as the Solar Dynamics Observatory, Kepler, and Picard, along with the current efforts of GONG, SOHO, and CoRoT, promise to provide clues to one of the deepest mysteries of the universe: the properties of the interiors of stars.
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ISBN: |
978-1-58381-712-4
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eISBN:
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978-1-58381-713-1
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Paper Title |
Page |
Authors |
Front matter |
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Volume Cover |
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Dikpati, M.; Arentoft, T.; González Hernández, I.; Lindsey, C.; Hill, F. |
Front matter |
1 |
Dikpati, M.; Arentoft, T.; González Hernández, I.; Lindsey, C.; Hill, F. |
Conference Photograph |
1 |
Dikpati, M.; Arentoft, T.; González Hernández, I.; Lindsey, C.; Hill, F. |
Part 1. Keynote Address |
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Seismology and the Dynamo: History and Prospects |
3 |
Cally, P. S. |
Part 2. Local Helioseismology |
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Helioseismic Measurement of Large-Scale Solar Flows |
15 |
Woodard, M. F. |
Time-Distance Helioseismic Imaging of a Numerically Simulated Solar Tachocline |
25 |
Zhao, J.; Hartlep, T.; Kosovichev, A. G.; Mansour N. N. |
Simulations of Waves in Sunspots |
31 |
Khomenko, E. |
New Results of High-Resolution Helioseismology from Hinode |
41 |
Kosovichev, A. G.; Zhao, J.; Sekii, T.; Nagashima, K.; Mitra-Kraev, U. |
Numerical Simulations of Quiet Sun Oscillations |
49 |
Schunker, H.; Cameron, R.; Gizon, L. |
Absorption of p Modes by Magnetic Plage |
55 |
Jain, R.; Hindman, B. W.; Braun, D. C.; Birch, A. C. |
Excitation, Propagation and Conversion of Helioseismic MHD Waves in Strong Field Regions |
61 |
Parchevsky, K. V.; Kosovichev, A. G. |
Realistic MHD Simulations of Solar Convection and Oscillations in Magnetic Regions: Mode Excitation and Effects of Acoustic Halos |
67 |
Jacoutot, L.; Kosovichev, A. G.; Wray, A.; Mansour, N. |
Analysis of Acoustic Wave Propagation in the Subphotosphere with Localized Magnetic Field Concentration |
75 |
Zharkov, S.; Shelyag, S.; Thompson, M. J. |
Magnetoseismic Study of the Active Region AR10720 |
81 |
Martínez-Oliveros, J. C.; Donea, A.-C. |
Improving the Prediction Capability of Seismic Far-Side Maps |
87 |
González Hernández, I.; Scherrer, P.; Hill, F.; Lindsey, C.; Braun, D. |
Time-Distance Envelope Widths: What Can They Tell Us? |
93 |
Armstrong, J. D. |
The Solar Subsurface Radial Gradient of Angular Velocity as Revealed by Ring Diagram Analysis |
99 |
Zaatri, A.; Corbard, T. |
Measuring Meridional Circulation in the Sun |
103 |
Duvall, T. L. Jr.; Hanasoge, S. M. |
New Multiple-Ridge Ring Analysis |
111 |
Haber, D. A. |
Temporal Variation of Subsurface Flows of Active Regions |
115 |
Komm, R.; Howe, R.; Hill, F. |
The Evolution of the Sub-Surface Structure of Long-Lived Active Regions |
119 |
Baldner, C. S.; Bogart, R. S.; Basu, S.; Antia, H. M. |
Subsurface Zonal Flows of Active and Quiet Regions |
123 |
Komm, R.; Howe, R.; Hill, F.; González Hernández, I. |
Subsurface Flow Properties of Flaring Versus Flare-Quiet Active Regions |
127 |
Ferguson, R.; Komm, R.; Hill, F.; Barnes, G.; Leka K. D. |
How Much Data Do We Need to Detect the Deep Solar Meridional Circulation? |
131 |
Braun, D. C.; Birch, A. C. |
Travel-Time Errors Due To Data Gaps |
135 |
Beck, J. G.; Duvall, T. L. Jr.; Zhao, J. |
Does the Selection of a Quiet Region Influence the Local Helioseismic Inferences? |
139 |
Tripathy, S. C.; Antia, H. M.; Jain, K.; Hill, F. |
Investigating The Role of Strong Magnetic Fields on Helioseismic Wave Propagation |
143 |
Moradi, H.; Hanasoge, S. M.; Cally, P. S. |
Signatures of Emerging Subsurface Structures in Acoustic Power Maps |
147 |
Hartlep, T.; Kosovichev, A. G.; Zhao, J.; Mansour, N. N. |
Ring Diagram Analysis of an Artificial 96 × 96 × 20 Mm Data Set |
151 |
Howe, R.; González Hernández, I.; Komm, R.; Hill, F. |
Can Sunspot Moats Tell Us β for the SolarDynamo? |
155 |
Lindsey, C. |
A Different Approach to Calculate the Far-Side Seismic Migration |
159 |
Pérez Hernández, F.; González Hernández, I. |
Time-Distance Solar Far-Side Imaging Using Three-Skip Acoustic Signals |
163 |
Ilonidis, S.; Zhao, J.; Hartlep, T. |
Numerical Simulation of Acoustic Wave Propagation in the Solar Sub-Photosphere with Localized Magnetic Field Concentration |
167 |
Shelyag, S.; Zharkov, S.; Fedun, V.; Erdélyi, R.; Thompson, M. J. |
Part 3. Global Helioseismology |
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Magnetic Fields and Temporal Variation |
173 |
Howe, R. |
Are Low-Degree p-Mode Frequencies Predictable from one Cycle to the Next? |
183 |
Broomhall, A.-M.; Chaplin, W. J.; Elsworth, Y.; New, R.; Verner, G. A. |
Correlation Analysis of Mode Frequencies with Activity Proxies at Different Phases of the Solar Cycle |
189 |
Jain, K.; Tripathy, S. C.; Hill, F. |
The Solar Metallicity Problem: What is the Solution? |
193 |
Basu, S. |
Measuring Solar Abundances with Seismology |
203 |
Mussack, K.; Gough, D. |
GOLF: Analysis of the Low Frequency Spectrum and Comparison with a Calculated Solar g-Mode Spectrum |
209 |
Grec, G.; Provost, J.; Renaud, C. |
What Can We Learn on the Structure and the Dynamics of the Solar Core with g Modes? |
215 |
Mathur, S.; Eff-Darwich, A.; García, R. A.; Jiménez-Reyes, S. J.; Korzennik, S. G.; Turck-Chièze, S. |
On the Dependence of our Inferences about the Solar Internal Rotation on the Frequency Fitting Methodology |
221 |
Korzennik, S. G.; Eff-Darwich, A. |
BiSON Update |
227 |
Allison, J.; Barnes, I.; Broomhall, A.-M.; Chaplin, W.; Davies, G.; Elsworth, Y.; Hale, S.; Jackson, B.; Miller, B. |
On Flare-Driven Global Waves |
233 |
Karoff, C. |
Post-hoc Derivation of MDI Flat Fields |
239 |
Potts, H. E.; Diver, D. A. |
The Inhomogeneous Response Across the Solar Disc of Unresolved Doppler Velocity Observations |
245 |
Broomhall, A.-M.; Chaplin, W. J.; Elsworth, Y.; New, R. |
Exploring Changes in Solar Model Physics to Mitigate the Solar Abundance Problem |
249 |
Guzik, J. A. |
Impact of Low-Frequency p Modes on the Inversions of the Internal Rotation of the Sun |
253 |
Salabert, D.; Eff-Darwich, A.; Howe, R.; Korzennik, S. G. |
Time-Frequency Analysis of Global Solar Oscillation Time Series |
257 |
Schad, A.; Roth, M.; Timmer, J. |
What is New with Zonal Flows? |
265 |
Antia, H. M.; Basu, S.; Chitre, S. M. |
The Torsional Oscillation and the Solar Cycle: Is it Minimum Yet? |
269 |
Howe, R.; Komm, R.; Hill, F.; Larson, T.; Schou, J.; Thompson, M. J.; Ulrich, R. K. |
Sensitivity of p Modes for Constraining Velocities of Microscopic Diffusion of the Elements |
273 |
Creevey, O. L.; Mathur, S.; García R. |
Search for Structural Variations of the Near-Surface Layers of the Sun during the Solar Cycle |
277 |
Rabello-Soares, M. C.; Korzennik, S. G. |
Variation in p-Mode Power over Solar Cycle 23 as seen from BiSON and GOLF Observations |
281 |
Simoniello, R.; Salabert, D.; García, R. A. |
Variation of Oscillation Mode Parameters over Solar Cycle 23: An Analysis on Different Time Scales |
285 |
Tripathy, S. C.; Hill, F.; Jain, K.; Leibacher, J. W. |
Changing Magnetic Fields in the Solar Interior |
289 |
Baldner, C. S.; H. M.; Basu, S.; Larson, T. P. |
Amplitudes of High-Degree p Modes in the Quiet and Active Sun |
293 |
O. Burtseva, O.; Tripathy, S. C.; Hill, F.; Kholikov, S.; Raouafi, N.-E.; Lindsey, C. |
Spatial Cross Spectrum: Reducing Incoherent Convective Background of Resolved Helioseismic Instruments |
297 |
García, R. A.; Mathur, S.; González Hernández, I.; Jiménez, A. |
Toward Eliminating Systematic Errors in Intermediate-Degree p-Mode Measurements |
301 |
Vorontsov, S. V.; Jefferies, S. M.; Giebink, C.; Schou, J. |
On the Solar Origin of the 220.7 µHz Signal |
307 |
Jiménez, A.; García, R. A. |
Variations in Global Mode Analysis |
311 |
Larson, T.; Schou, J. |
Results from Fitting Long and Very-Long MDI Time-Series at Low and Intermediate Degrees |
315 |
Korzennik, S. G. |
Calculation of Solar p-Mode Oscillation Frequency Splittings Based on a Two-Dimensional Solar Model |
321 |
Li, L.; Basu, S.; Sofia, S.; Demarque, P. |
Analysis of GOLF Power Spectra Weighted to Account for Noise Variations Through the Data Set |
325 |
New, R.; Fletcher, S.; Chaplin, W.; Elsworth, Y.; García, R. A. |
Low-Frequency Solar p Modes as Seen by the GOLF and GONG Instruments |
329 |
Salabert, D.; García, R. A. |
Evidence of Enhanced High Frequency Velocity Oscillations in the Sun Observed During Solar Flares Using Disk-Integrated Doppler Signals |
333 |
Kumar, B.; Venkatakrishnan, P. |
The Simulation of Realistic BiSON-like Helioseismic Data |
337 |
Fletcher, S.; New, R.; Broomhall, A.-M.; Chaplin, W.; Elsworth, Y. |
First Performance of the GOLF-NG Instrumental Prototype Observing the Sun in Tenerife |
341 |
Salabert, D.; Turck-Chièze, S.; Barrière, J. C.; Carton, P. H.; Daniel-Thomas, P.; Delbart, A.; García, R. A.; Granelli, R.; Jiménez-Reyes, S. J.; Lahonde-Hamdoun, C.; Loiseau, D.; Mathur, S.; Nunio, F.; Pallé, P. L.; Piret, Y.; Robillot, J. M.; Simoniello, R. |
Part 4. Asteroseismology |
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Optimizing Weights for the Detection of Stellar Oscillations: Application to α Centauri A and B, and β Hydri |
347 |
Arentoft, T.; Kjeldsen, H.; Bedding, T. R. |
Comparing Properties of Convection in the Surface Layers of Stars With Different Masses and Evolutionary States |
357 |
Robinson, F.; Tanner, J.; Basu, S.; Demarque, P. |
Testing the Potential and Limitations of Seismic Data |
363 |
Creevey, O. L. |
Dynamo Action and Wreaths of Magnetism in a Younger Sun |
369 |
Brown, B. P.; Browning, M. K.; Brun, A. S.; Miesch, M. S.; Toomre, J. |
The Activity Cycles and Surface Differential Rotation of Single Dwarfs |
375 |
Saar, S. H. |
Differential Rotation in Stars: Expectations and Asteroseismic Diagnostics |
385 |
Kawaler, S. D. |
Pulsation Modes with High Azimuthal Orders in Stellar Models Based on the Self-Consistent Field Method |
395 |
Reese, D. R.; MacGregor, K. B.; Jackson, S.; Skumanich, A.; Metcalfe, T. S. |
Discovery of New Hot Pulsators in the CoRoT Exoplanet Database and Their Potential for Asteroseismology |
401 |
Aerts, C.; Debosscher, J.; Sarro, L.; Degroote, P.; Neiner, C.; Maceroni, C.; Ribas, I.; Auvergne, M.; Deleuil, M.; Ollivier, M.; Jorda, L.; Samadi, R. |
Asteroseismic Age and Radius of Kepler stars |
407 |
Creevey, O. L. |
Iterative Inversion for Solar and Stellar Internal Rotation |
411 |
Sudnik M.; Thompson, M. J. |
Asteroseismic Tests of Heavy Element Diffusion in Low-Mass Stars |
415 |
Gai, N.; Bi, S. L.; Tang, Y. K. |
Part 5. Solar Activity: Convection, Tachocline, Dynamo, and Data Assimilation |
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Supergranulation-Scale Convection Simulations |
421 |
Stein, R. F.; Nordlund, Å.; Georgoviani, D.; Benson, D.; Schaffenberger, W. |
Realistic Magnetohydrodynamical Simulations of Local Solar Supergranulation |
427 |
Ustyugov, S. D. |
From Fibril to Diffuse Fields During Dynamo Saturation |
433 |
Brandenburg, A. |
Three-Dimensional Simulations of Solar and Stellar Dynamos: The Influence of a Tachocline |
443 |
Miesch, M. S.; Browning, M. K.; Brun, A. S.; Toomre, J.; Brown, B. P. |
Exploring Turbulent Effects in Babcock-Leighton Solar Dynamo Models |
453 |
Guerrero, G.; de Gouveia Dal Pino, E. M.; Dikpati, M. |
Radiative-MHD Simulations of Sunspot Structure |
461 |
Rempel, M. |
Instabilities in the Magnetic Tachocline |
467 |
Arlt, R. |
Solar-Cycle Related Changes at the Base of the Convection Zone |
477 |
Baldner, C. S.; Larson, T. P.; Basu, S. |
On the Long-Term Cyclic Period of North-South Asymmetry of Solar Active Region Phenomena |
483 |
Verma, V. K. |
Modeling the Subsurface Evolution of Active-Region Flux Tubes |
489 |
Fan, Y. |
The Advection of Supergranules by Large-Scale Flows |
495 |
Hathaway, D. H.; Williams, P. E.; Cuntz, M. |
Data Assimilation and Helio- & Asteroseismology |
501 |
Roth, M. |
Implementation of Data Assimilation Methods for Dynamo Models to Predict Solar Activity |
511 |
Kitiashvili I.; Kosovichev, A. |
Pseudo-Global Fitting of Gapped Helioseismic Data |
519 |
Fletcher, S.; New, R.; Chaplin, W.; Elsworth, Y. |
Axisymmetric MHD Instabilities in Solar/Stellar Tachoclines |
525 |
Dikpati, M.; Cally, P. S.; Gilman, P. A.; Miesch, M. S. |
GOLF: A New Proxy for Solar Magnetism |
529 |
Mathur, S.; Jiménez-Reyes, S. J.; García, R. A. |
Applying Fourier and Variable Sine Algorithmic Analysis to Solar Data |
533 |
Reindel, A.; Bradley, P. A.; Tsantilas, S.; Guzik, J. A. |
An Investigation of Solar Magnetic Indices for Space Weather Forecasting |
537 |
Brockman, A.; Giersch, O.; Kennewell, J. |
Using Solar Regions as Seen by Hinode XRT to Model the Coronae of Inactive Stars and Magnetic Minima |
543 |
Saar, S.; Testa, P.; Weber, M.; Marsh, J. |
Transport of Supergranules and their Vertical Coherence |
547 |
Švanda, M.; Kosovichev, A. G.; Klvana, M.; Sobotka, M.; Duvall, T. L., Jr. |
Group Discussion: Solar Activity: The Role of Convection, the Tachocline and the Dynamo and Applications of Data Assimilation |
551 |
Rempel, M.; Dikpati, M. |
Part 6. Major Observational Programs |
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The Future of Helioseismology |
557 |
Hill, F. |
Asteroseismology and the Solar-Stellar Connection |
567 |
Metcalfe, T. S. |
PLATO: PLAnetary Transits and Oscillations of Stars |
577 |
Arentoft, T.; ESA PLATO Science Study team |
The Stellar Observations Network Group—the Prototype |
579 |
Grundahl, F.; Christensen-Dalsgaard, J.; Kjeldsen, H.; Jørgensen, U. G.; Arentoft, T.; Frandsen, S.; Kjærgaard, P. |
BRITE-Constellation |
587 |
Kuschnig, R.; Weiss, W. W.; Moffat, A.; Kudelka, O. |
SIAMOIS: Seismic Interferometer to Measure Oscillations in the Interiors of Stars |
591 |
Mosser B.; the SIAMOIS Team |
Back matter |
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Indexes |
593 |
Dikpati, M.; Arentoft, T.; González Hernández, I.; Lindsey, C.; Hill, F. |
Back matter |
598 |
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