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On 2D Linear Polarimetry in Prominences
Published online by Cambridge University Press: 06 January 2014
Abstract
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An approach for high-precision 2D linear polarimetry is briefly described. The key components are reducing random errors, reducing systematic errors, and obtaining 2D distributions of the linear polarization degree, p, and polarization angle, χ (deviation of the polarization plane from the direction tangential to the solar limb).
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 8 , Symposium S300: Nature of Prominences and their role in Space Weather , June 2013 , pp. 462 - 463
- Copyright
- Copyright © International Astronomical Union 2013
References
Chae, J., Yun, H. S., Sakurai, T., & Ichimoto, K. 1998, Solar Phys. 183 p. 229CrossRefGoogle Scholar
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