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On 2D Linear Polarimetry in Prominences

Published online by Cambridge University Press:  06 January 2014

V. V. Popov
Affiliation:
Lomonosov Moscow State University, Sternberg Astronomical institute, 119992 Universitetsky pr-t, 13, Moscow, Russia email: [email protected]
I. S. Kim
Affiliation:
Lomonosov Moscow State University, Sternberg Astronomical institute, 119992 Universitetsky pr-t, 13, Moscow, Russia email: [email protected]
E. Z. Suyunova
Affiliation:
Lomonosov Moscow State University, Sternberg Astronomical institute, 119992 Universitetsky pr-t, 13, Moscow, Russia email: [email protected]
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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
Copyright
Copyright © International Astronomical Union 2013 

References

Bommier, V., Leroy, J. L., & Sahal-Brechot, S. 1994, Solar Phys. 154 p. 231CrossRefGoogle Scholar
Chae, J., Yun, H. S., Sakurai, T., & Ichimoto, K. 1998, Solar Phys. 183 p. 229CrossRefGoogle Scholar
Kim, I. S., Lisin, D. V., Popov, V. V., & Popova, E. V., 2011, ASP-CS 437 p. 181Google Scholar
Suyunova, E. Z., Kim, I. S., Popov, V. V., & Bugaenko, O. I. 2013, CEAB, 37.Google Scholar