Understanding the Fe i Line Measurements Returned by the Helioseismic and Magnetic Imager (HMI)
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/s11207-015-0654-7.pdf
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3. Couvidat, S., Rajaguru, S.P., Wachter, R., Sankarasubramanian, K., Schou, J., Scherrer, P.H.: 2012, Line-of-sight observables algorithms for the Helioseismic and Magnetic Imager (HMI) instrument tested with Interferometric Bidimensional Spectrometer (IBIS) observations. Solar Phys. 278, 217. DOI . ADS .
4. Criscuoli, S., Ermolli, I., Del Moro, D., Giorgi, F., Tritschler, A., Uitenbroek, H., Vitas, N.: 2011, Line shape effects on intensity measurements of solar features: brightness correction to SOHO MDI continuum images. Astrophys. J. 728, 92. DOI . ADS .
5. Criscuoli, S., Ermolli, I., Uitenbroek, H., Giorgi, F.: 2013, Effects of unresolved magnetic field on Fe I 617.3 and 630.2 nm line shapes. Astrophys. J. 763, 144. DOI . ADS .
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