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Precision solar astrometry from SoHO/MDI
Published online by Cambridge University Press: 25 May 2016
Abstract
The SoHO/MDI experiment generates a continous record of the solar limb brightness using 1.96″ pixels. Because there is no atmospheric blurring, these data allow measurements of solar limb brightness and shape changes with a precision that has not been achieved from the ground. The first results of a 1 month astrometric timeseries from the MDI solar structure program will be described here.
- Type
- Part I: Helioseismology: From ground or space, a worldwide cooperation
- Information
- Symposium - International Astronomical Union , Volume 181: Sounding Solar and Stellar Interiors , 1997 , pp. 103 - 110
- Copyright
- Copyright © Kluwer 1997
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