Comment on “Resolving the 180° Ambiguity in Solar Vector Magnetic Field Data: Evaluating the Effects of Noise, Spatial Resolution, and Method Assumptions”-Reference-Cited by-同舟云学术

Comment on “Resolving the 180° Ambiguity in Solar Vector Magnetic Field Data: Evaluating the Effects of Noise, Spatial Resolution, and Method Assumptions”

Published:2011-07-27 Issue:1-2 Volume:276 Page:423-440
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Georgoulis Manolis K.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/s11207-011-9819-1.pdf

Reference26 articles.

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2. Aly, J.J.: 1987, On the uniqueness of the determination of the coronal potential magnetic field from line-of-sight boundary conditions. Solar Phys. 111, 287 – 296. doi: 10.1007/BF00148521 .

3. Chiu, Y.T., Hilton, H.H.: 1977, Exact Green’s function method of solar force-free magnetic-field computations with constant alpha. I – Theory and basic test cases. Astrophys. J. 212, 873 – 885. doi: 10.1086/155111 .

4. Crouch, A.D., Barnes, G., Leka, K.D.: 2009, Resolving the azimuthal ambiguity in vector magnetogram data with the divergence-free condition: application to discrete data. Solar Phys. 260, 271 – 287. doi: 10.1007/s11207-009-9454-2 .

5. Gary, G.A.: 1989, Linear force-free magnetic fields for solar extrapolation and interpretation. Astrophys. J. Suppl. 69, 323 – 348. doi: 10.1086/191316 .

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