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Abstract
We present an up-to-date latitude–time map of the solar zonal flows at 0.99 R⊙ from global helioseismology using data from the Global Oscillation Network Group, the Michelson Doppler Imager, and the Helioseismic and Magnetic Imager.
Original language | English |
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Article number | 261 |
Journal | Research Notes of the AAS |
Volume | 6 |
Issue number | 12 |
DOIs | |
Publication status | Published - 31 Dec 2022 |
Bibliographical note
Acknowledgments:This work utilizes data obtained by the Global Oscillation Network Group (GONG) program, managed by the National Solar Observatory, which is operated by AURA, Inc. under a cooperative agreement with the National Science Foundation. The data were acquired by instruments operated by the Big Bear Solar Observatory, High Altitude Observatory, Learmonth Solar Observatory, Udaipur Solar Observatory, Instituto de Astrofísica de Canarias, and Cerro Tololo Interamerican Observatory. SOHO is a project of international cooperation between ESA and NASA. HMI data courtesy of NASA/SDO and the HMI science team. R.H. and Y.P.E. acknowledge the support of the UK Science and Technology Facilities Council (STFC) through grant ST/V000500/1.
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Dive into the research topics of 'Update on Global Helioseismic Observations of the Solar Torsional Oscillation'. Together they form a unique fingerprint.Projects
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Helioseismology at Birmingham & Queen Mary
Chaplin, B. (Principal Investigator)
SCIENCE & TECHNOLOGY FACILITIES COUNCIL
1/04/21 → 31/12/24
Project: Research Councils