Solar coronal magnetic fields derived using seismology techniques applied to omnipresent sunspot waves-Reference-Cited by-同舟云学术

Solar coronal magnetic fields derived using seismology techniques applied to omnipresent sunspot waves

Published:2015-11-16 Issue:2 Volume:12 Page:179-185
ISSN:1745-2473
Container-title:Nature Physics
language:en
Short-container-title:Nature Phys

Author:

Jess David B.^ORCID,Reznikova Veronika E.,Ryans Robert S. I.,Christian Damian J.,Keys Peter H.,Mathioudakis Mihalis,Mackay Duncan H.,Krishna Prasad S.,Banerjee Dipankar,Grant Samuel D. T.,Yau Sean,Diamond Conor

Publisher

Springer Science and Business Media LLC

Subject

General Physics and Astronomy

Link

http://www.nature.com/articles/nphys3544.pdf

Reference29 articles.

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3. Kramar, M., Inhester, B. & Solanki, S. K. Vector tomography for the coronal magnetic field. I. Longitudinal Zeeman effect measurements. Astron. Astrophys. 456, 665–673 (2006).

4. Nakariakov, V. M. & Ofman, L. Determination of the coronal magnetic field by coronal loop oscillations. Astron. Astrophys. 372, L53–L56 (2001).

5. Verwichte, E., Nakariakov, V. M., Ofman, L. & Deluca, E. E. Characteristics of transverse oscillations in a coronal loop arcade. Sol. Phys. 223, 77–94 (2004).

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