S
S. G. Korzennik
Researcher at Harvard University
Publications - 23
Citations - 1643
S. G. Korzennik is an academic researcher from Harvard University. The author has contributed to research in topics: Solar rotation & Radiative transfer. The author has an hindex of 11, co-authored 23 publications receiving 1587 citations.
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Journal ArticleDOI
Helioseismic Studies of Differential Rotation in the Solar Envelope by the Solar Oscillations Investigation Using the Michelson Doppler Imager
Jesper Schou,H. M. Antia,Sarbani Basu,R. S. Bogart,R. I. Bush,S. M. Chitre,Joergen Christensen-Dalsgaard,M. Di Mauro,W. A. Dziembowski,Antonio Eff-Darwich,Douglas Gough,Deborah A. Haber,J. T. Hoeksema,R. Howe,S. G. Korzennik,Alexander G. Kosovichev,R. M. Larsen,R. M. Larsen,Frank P. Pijpers,Philip H. Scherrer,Takashi Sekii,Theodore D. Tarbell,Alan M. Title,Michael Thompson,Juri Toomre +24 more
TL;DR: In this article, the authors report on joint helioseismic analyses of solar rotation in the convection zone and in the outer part of the radiative core using the Michelson Doppler Imager (MDI) on the Solar and Heliospheric Observatory (SOHO) spacecraft.
Journal ArticleDOI
The Asteroseismic potential of Kepler : first results for solar-type stars
William J. Chaplin,Thierry Appourchaux,Yvonne Elsworth,Rafael A. García,G. Houdek,Christoffer Karoff,Travis S. Metcalfe,Joanna Molenda-Żakowicz,Mário J. P. F. G. Monteiro,Michael Thompson,Timothy M. Brown,Jørgen Christensen-Dalsgaard,R. L. Gilliland,Hans Kjeldsen,William J. Borucki,David G. Koch,Jon M. Jenkins,Jon M. Jenkins,Jérôme Ballot,Sarbani Basu,Michael Bazot,Timothy R. Bedding,O. Benomar,Alfio Bonanno,I. M. Brandão,H. Bruntt,Tiago L. Campante,Orlagh Creevey,M. Di Mauro,G. Doğan,S. Dreizler,Patrick Eggenberger,L. Esch,Stephen T. Fletcher,S. Frandsen,N. Gai,Patrick Gaulme,Rasmus Handberg,Saskia Hekker,Roger T. Howe,Daniel Huber,S. G. Korzennik,J. C. Lebrun,Silvio Leccia,M. Martic,Savita Mathur,B. Mosser,Roger New,P.-O. Quirion,C. Régulo,Ian W. Roxburgh,D. Salabert,Jesper Schou,S. G. Sousa,Dennis Stello,Graham A. Verner,Torben Arentoft,Caroline Barban,Kevin Belkacem,S. Benatti,Katia Biazzo,P. Boumier,Paul A. Bradley,Anne-Marie Broomhall,Derek Buzasi,Riccardo Claudi,Margarida S. Cunha,F. D'Antona,Sébastien Deheuvels,Aliz Derekas,A. García Hernández,M. S. Giampapa,J. M. Goupil,M. Gruberbauer,Joyce A. Guzik,Steven J. Hale,Michael J. Ireland,László L. Kiss,I. N. Kitiashvili,Katrien Kolenberg,Heidi Korhonen,Alexander G. Kosovichev,Friedrich Kupka,Yveline Lebreton,B. Leroy,H.-G. Ludwig,Stéphane Mathis,E. Michel,Andrea Miglio,Josefina Montalbán,A. Moya,Arlette Noels,Robert W. Noyes,Pere L. Palle,L. Piau,H. L. Preston,T. Roca Cortés,Markus Roth,K. H. Sato,J. H. M. M. Schmitt,Aldo Serenelli,V. Silva Aguirre,Ian R. Stevens,Juan Carlos Suárez,M. D. Suran,R. Trampedach,Sylvaine Turck-Chièze,K. Uytterhoeven,Rita Ventura,Paul Wilson +109 more
TL;DR: In this article, preliminary asteroseismic results from Kepler on three G-type stars are presented, made at one-minute cadence during the first 33.5 days of science operations, reveal high signal-to-noise solar-like oscillation spectra in all three stars: about 20 modes of oscillation may be clearly distinguished in each star.
Journal ArticleDOI
The asteroseismic potential of Kepler: first results for solar-type stars
William J. Chaplin,T. Appourchaux,Yvonne Elsworth,Rafael A. García,G. Houdek,Christoffer Karoff,T. S. Metcalfe,J. Molenda-Zakowicz,Mário J. P. F. G. Monteiro,Michael Thompson,Timothy M. Brown,Jørgen Christensen-Dalsgaard,R. L. Gilliland,Hans Kjeldsen,William J. Borucki,David G. Koch,Jon M. Jenkins,Jérôme Ballot,Sarbani Basu,M. Bazot,Timothy R. Bedding,O. Benomar,Alfio Bonanno,I. M. Brandão,H. Bruntt,Tiago L. Campante,O. L. Creevey,M. Di Mauro,G. Doğan,S. Dreizler,P. Eggenberger,L. Esch,Stephen T. Fletcher,S. Frandsen,Ning Gai,Patrick Gaulme,Rasmus Handberg,Saskia Hekker,Roger T. Howe,Daniel Huber,S. G. Korzennik,J. C. Lebrun,Silvio Leccia,M. Martic,Savita Mathur,B. Mosser,Roger New,P.-O. Quirion,Clara Régulo,Ian W. Roxburgh,D. Salabert,Jesper Schou,S. G. Sousa,Dennis Stello,Graham A. Verner,Torben Arentoft,Caroline Barban,Kevin Belkacem,S. Benatti,Katia Biazzo,P. Boumier,Paul A. Bradley,Anne-Marie Broomhall,Derek Buzasi,Riccardo Claudi,Margarida S. Cunha,F. D'Antona,Sébastien Deheuvels,Aliz Derekas,A. García Hernández,M. S. Giampapa,M. J. Goupil,M. Gruberbauer,J. A. Guzik,Steven J. Hale,Michael J. Ireland,László L. Kiss,I. N. Kitiashvili,Katrien Kolenberg,Heidi Korhonen,Alexander G. Kosovichev,Friedrich Kupka,Yveline Lebreton,B. Leroy,H.-G. Ludwig,Stéphane Mathis,E. Michel,Andrea Miglio,Josefina Montalbán,A. Moya,Arlette Noels,Robert W. Noyes,Pere L. Palle,L. Piau,H. L. Preston,T. Roca Cortés,Markus Roth,K. H. Sato,J. H. M. M. Schmitt,Aldo Serenelli,V. Silva Aguirre,Ian R. Stevens,Juan Carlos Suárez,M. D. Suran,R. Trampedach,Sylvaine Turck-Chièze,K. Uytterhoeven,Rita Ventura +107 more
TL;DR: In this article, preliminary asteroseismic results from Kepler on three G-type stars are presented, made at one-minute cadence during the first 33.5d of science operations, reveal high signal-to-noise solar-like oscillation spectra in all three stars: about 20 modes of oscillation may be clearly distinguished in each star.
Journal ArticleDOI
On the Determination of Michelson Doppler Imager High-Degree Mode Frequencies
TL;DR: In this article, the authors presented the results of fitting high-degree power ridge (up to l = 900) computed from several 2-3 month long time series of full-disk observations taken with the Michelson Doppler Imager (MDI) on board the Solar and Heliospheric Observatory between 1996 and 1999.
Journal ArticleDOI
On The Determination of MDI High-Degree Mode Frequencies
TL;DR: In this article, the authors presented the results of fitting high degree power ridge (up to l = 900) computed from several two to three-month-long time-series of full-disk observations taken with the Michelson Doppler Imager (MDI) on-board the Solar and Heliospheric Observatory between 1996 and 1999.