Magnetic field vector retrieval with HMI
Borrero, J.M., Tomczyk, S., Norton, A.A., Darnell, T., Schou, J., Scherrer, P., Bush, R.I., and Lui, Y. (2006) Magnetic field vector retrieval with HMI. Proceedings of the Astronomical Society of the Pacific Conference Series. Astronomical Society of the Pacific Conference Series , 19-23 September 2005, Boulder, Colorado, USA , pp. 144-147.
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The Helioseismic and Magnetic Imager (HMI), on board the Solar Dynamics Observatory (SDO), will begin data acquisition in 2008. It will provide the first full-disk, high temporal cadence observations of the full Stokes vector with a 0.′′5 pixel size. This will allow for a continuous monitoring of the Solar magnetic-field vector. HMI data will advance our understanding of the small- and large-scale magnetic field evolution, its relation to the solar and global dynamic processes, coronal field extrapolations, flux emergence, magnetic helicity, and the nature of the polar magnetic fields. We summarize HMI’s expected operation modes, focusing on the polarization cross-talk induced by the solar oscillations, and how this affects the magnetic-field vector determination.
|Item Type:||Conference Item (Refereed Research Paper - E1)|
|FoR Codes:||02 PHYSICAL SCIENCES > 0201 Astronomical and Space Sciences > 020109 Space and Solar Physics @ 100%|
|SEO Codes:||97 EXPANDING KNOWLEDGE > 970102 Expanding Knowledge in the Physical Sciences @ 100%|
|Deposited On:||14 Apr 2010 10:42|
|Last Modified:||12 Feb 2011 23:36|
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