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Solar-stellar dynamos as revealed by helio- and asteroseismology |
The inhomogeneous response across the solar disc of unresolved Doppler velocity observations
Anne-Marie Broomhall, William J. Chaplin, Yvonne Elsworth and Roger New
Are p-mode frequencies predictable from one solar cycle to the next?
Anne-Marie Broomhall, William J Chaplin, Yvonne Elsworth, Brek A. Miller, Roger New and Graham Verner
Benjamin Brown
Raymond Burston, Laurent Gizon, Yacine Saidi and Sami Solanki
Effect of surface activity on amplitudes of high-degree solar p-modes
Olga Burtseva, Sushant Tripathy, Frank Hill and Shukur Kholikov
Influence of magnetic activity on lifetime of high-l solar p-modes
Olga Burtseva, Frank Hill and Shukur Kholikov
Paul Cally
Hamed Moradi and Paul Cally
Robert Cameron and Hannah Schunker
A new method to probe the interaction between solar acoustic waves and magnetic regions
Dean-Yi Chou
Jørgen Christensen-Dalsgaard
Orlagh L. Creevey
Testing the potential and limitations of seismic stellar systems
Orlagh L. Creevey
Sensitivity of p-modes for determining the microscopic diffusion coefficient at the base of the convection zone
Orlagh L. Creevey, Savita Mathur and Rafael A. Garcia
Ashley Crouch
Mausumi Dikpati, Paul Cally, Peter Gilman and Mark Miesch
Thomas Duvall and Shravan Hanasoge
John Allison, Ian Barnes, Anne-Marie Broomhall, William J. Chaplin, Guy Davies, Yvonne Elsworth, Stephen T. Fletcher, Steven Hale, Barry Jackson, Brek A. Miller and Roger New
Modeling the subsurface evolution of emerging active region flux tubes
Yuhong Fan
The generation of more realistic BiSON-like artificial helioseismic data
Stephen Fletcher, Anne-Marie Broomhall, William Chaplin, Yvonne Elsworth and Roger New
Stephen Fletcher, William Chaplin, Yvonne Elsworth and Roger New
Spatial Cross Spectrum: reducing the incoherent convective background of resolved helioseismic instruments
Rafael A. Garcia, Savita Mathur, Irene Gonzalez Hernandez, Antonio Jimenez
Antonio Jimenez and Rafael Garcia
GOLF: Analysis of the low frequency spectrum and comparison with a calculated solar g-mode spectrum
Gerard Grec, Janine Provost and Catherine Renaud
Gustavo Guerrero and Elisabete de Gouveia Dal Pino
Exploring uncertainties in solar model physics and predictions arising from the new abundances
Joyce Guzik, Alexander Friedland, L.S. Watson, Andrew Reindel and David Kilcrease
Deborah Haber and Bradley Hindman
Margit Haberreiter, Juan Fontenla, Irene Gonzalez-Hernandez, Charles Lindsey and Eric Quemérais
Signatures of emerging subsurface structures in acoustic power maps
Thomas Hartlep and Alexander Kosovichev
David Hathaway, Peter Williams and Manfred Cuntz
Improving the prediction capability of the helioseismic far-side maps
Irene Gonzalez Hernandez, Philip Scherrer, Charles Lindsey, Doug Braun, Frank Hill
Meridional circulation in the declining phase of solar cycle 23
Irene Gonzalez Hernandez, Shukur Kholikov, Frank Hill, Rachel Howe, Rudolph Komm
A different approach to calculate the far-side seismic migration Green's functions
Fernando Perez Hernandez and Irene Gonzalez Hernandez
Frank Hill
Bradley Hindman
Rachel Howe, Irene Gonzalez Hernandez, Rudi Komm and Frank Hill
The torsional oscillation and the solar cycle: is it minimum yet?
Rachel Howe, Frank Hill, Rudi Komm, Timothy P. Larson, Jesper Schou, Michael J. Thompson and Roger Ulrich
Rachel Howe
Time-Distance Solar Far-Side Imaging Using Three-Skip Acoustic Signals
Stathis Ilonidis and Junwei Zhao
Jason Jackiewicz, Laurent Gizon and Aaron Birch
Realistic MHD Simulations of Solar Convection and Oscillations in Magnetic Regions: Mode Excitation and Effect of Acoustic Halo
Laetitia Jacoutot, Alexander Kosovichev, Alan Wray and Nagi Mansour
Rekha Jain and Bradley Hindman
Christoffer Karoff
Steven Kawaler
Elena Khomenko
Implementation of Data Assimilation Methods for Dynamo Models to Predict Solar Activity
Irina Kitiashvili and Alexander Kosovichev
Rudolf Komm, Frank Hill, Rachel Howe and Irene Gonzalez Hernandez
Rudolf Komm, Frank Hill and Rachel Howe
Subsurface flow properties of flaring versus flare-quiet active regions
Ryan Ferguson, Rudolf Komm, Frank Hill, Graham Barnes and K.D. Leka
Resolving Sharp Boundaries in Inversion of Helioseismic Parameters
Antonio Eff-Darwich and Sylvain G. Korzennik
On the Dependence of our Inferences about the Solar Internal Rotation on the Frequency Fitting Methodology
Sylvain Korzennik and Antonio Eff-Darwich
Results from fitting long and very-long MDI time series of sphericalharmonics coefficients, at low and intermediate degrees
Sylvain Korzennik
Alexander Kosovichev, Takashi Sekii, Junwei Zhao, Kaori Nagashima and Urmila Mitra-Kraev
Michal Svanda, Alexander Kosovichev, Miroslav Klvana, Michal Sobotka and Duvall Jr. Thomas
Evidence of enhanced high frequency velocity oscillations in the Sun observed during solar flare using disk integrated Doppler signals
Brajesh Kumar and Parmeswaran Venkatakrishnan
Dr. Rainer Kuschnig, Werner Weis and Anthony Moffat
Timothy Larson and Jesper Schou
Calculation of solar p-mode oscillation frequency splittings based on a two-dimensional solar model
Linghuai Li, Sarbani Basu, Sabatino Sofia and Pierre Demarque
Simulations of the Near-Surface Interaction Between Waves and Sunspots
Charles Lindsey
Magneto-Seismic Study of the X1.2 15 January 2005 Solar Flare
Juan Carlos Martinez-Oliveros and Alina Donea
Savita Mathur, S. Jimenez-Reyes and R.A Garcia
What can be learnt with g modes on the structure and the dynamics of the solar core?
Savita Mathur, et al.
Travis Metcalfe
Mark Miesch, Benjamin Brown, Matthew Browning, Allan Sacha Brun and Juri Toomre
Katie Mussack
Analysis of GOLF power spectra weighted to account for noise variations through the data set
Roger New, Stephen Fletcher, William Chaplin, Yvonne Elsworth and Rafael Garcia
Excitation, propagation and conversion of helioseismic MHD waves in strong field regions
Konstantin Parchevsky and Alexander Kosovichev
Hugh E Potts and Declan A Diver
Structural Variations of the Near-Surface Layers of the Sun during the Solar Cycle
M. Cristina Rabello-Soares and S. G. Korzennik
Daniel Reese, Keith MacGregor, Stephen Jackson, Andrew Skumanich and Travis Metcalfe
Andrew Reindel, Sotirios Tsantilas, Joyce Ann Guzik and Paul Bradley
Matthias Rempel
Comparing properties of convection in stars with different masses and evolutionary states
Frank Robinson, Joel Tanner, Sarbani Basu and Pierre Demarque
Markus Roth
Using Solar Regions as Seen by Hinode XRT to Model the Coronae of Inactive Stars and Magnetic Minima
Steven Saar and Paola Testa
The Activity Cycles and Surface Differential Rotation of Single Dwarfs
Steven Saar
From the collapsograms to the overlapograms: low-frequency solar p modes as seen by GOLF instrument
David Salabert and Rafael A. Garcia
First performances of the GOLF-NG instrumental prototype observing the Sun in Tenerife
David Salabert, Sylvaine Turck-Chieze (P.I.), and the GOLF-NG team
The impact of low-frequency p modes on the inversions of the internal rotation of the Sun
David Salabert, Antonio Eff-Darwich, Howe Rachel, Thierry Appourchaux and John Leibacher
P mode power variation as seen over the solar cycle in intensity and velocity helioseismic measurements
Rosaria Simoniello, David Salabert, Carl Henneyand Rafael A. Garcia
Ariane Schad, Markus Roth and Jens Timmer
The Helioseismic and Magnetic Imager - Calibration, Expected Performance and Future Challenges
Jesper Schou
Toward Eliminating Systematic Errors in Intermediate-degree p-mode Measurements
Sergei Vorontsov, Stuart Jefferies, Cindy Giebink and Jesper Schou
Hannah Schunker, Robert Cameron and Laurent Gizon
Numerical simulation of acoustic wave propagation in the solar subphotosphere with localized magnetic field concentration
Serhii Shelyag, S Zharkov, V Fedun, R Erdelyi and Michael Thompson
Robert Stein, Ake Nordlund, Dali Georgobiani, Benson David and Werner Schaffenberger
Michael Sudnik and Michael J. Thompson
Steven Tomczyk and Scott McIntosh
Correlation analysis of mode frequencies with activity proxies at different phases of the solar cycle
Kiran Jain, Sushant C. Tripathy and Frank Hill
Does the Selection of a Quiet Region Influence the Local Helioseismic Inferences?
Sushanta Tripathy, Kiran Jain and Frank Hill
Variation of oscillation mode parameters over the solar cycle 23: An analysis on different time scales
Sushanta Tripathy, Kiran Jain, John Leibacher and Frank Hill
Realistic Magnetohydrodynamic Simulation of Solar Local Supergranulation
Sergey Ustyugov
On the Long-Term Cyclic Period of North-South Asymmetry of Solar Active Region Phenomena
Virendra K. Verma
Martin Woodard
The solar subsurface radial gradient of the horizontal zonal flow as revealed by Ring diagram analysis
Amel Zaatri and Thierry Corbard
Sound-Speed Image of Tachocline and Its Evolution from Time-Distance Helioseismology
Junwei Zhao, Thomas Hartlep, Alexander Kosovichev and Nagi Mansour
Time-distance analisis of numerical simulation of acoustic wave propagation in the solar subphotosphere with localized magnetic field concentration
Sergei Zharkov, S Shelyag and Michael Thompson
Last Updated by Mausumi Dikpati on 07/17/08