A Time–Distance Helioseismology Method for Quasi-Linear Geometries
Author:
Funder
NASA
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/s11207-019-1547-y.pdf
Reference25 articles.
1. Cameron, R., Gizon, L., Duvall, T.L. Jr.: 2008, Helioseismology of sunspots: confronting observations with three-dimensional MHD simulations of wave propagation. Solar Phys.251, 291. DOI . ADS .
2. Couvidat, S., Zhao, J., Birch, A.C., Kosovichev, A.G., Duvall, T.L. Jr., Parchevsky, K., Scherrer, P.H.: 2012, Implementation and comparison of acoustic travel-time measurement procedures for the Solar Dynamics Observatory/Helioseismic and Magnetic Imager time–distance helioseismology pipeline. Solar Phys.275, 357. DOI . ADS .
3. Domingo, V., Fleck, B., Poland, A.I.: 1995, The SOHO mission: an overview. Solar Phys.162, 1. DOI . ADS .
4. Duvall, T.L. Jr., Gizon, L.: 2000, Time–distance helioseismology with $f$ modes as a method for measurement of near-surface flows. Solar Phys.192, 177. ADS .
5. Duvall, T.L. Jr., Jefferies, S.M., Harvey, J.W., Pomerantz, M.A.: 1993, Time–distance helioseismology. Nature362, 430. DOI . ADS .
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