Three-dimensional reconstruction of UV emissivities in the solar corona using Ultraviolet Coronagraph Spectrometer data from the Whole Sun Month

Journal of Geophysical Research: Space Physics

Volumn 104, Issue A5, 1999, Pages 9721-9726

  Panasyuk, Alexander V ^a  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0005752172     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: 10.1029/1998ja900118     Document Type: Article

References (6)

1. Davila, J.M., Solar Tomography, Astrophys. J., 423, 871-877, 1994.
2. Delaboudinière, J.-P., et al., EIT: Extreme-Ultraviolet Imaging Telescope for the Soho mission, Sol. Phys., 162, 291, 1996
3. Kak, A.C., Image reconstruction from projections, Digital Image Processing Techniques, edited by M.P. Ekstrom, p.111, Academic, San Diego, Calif., 1984.
4. Kohl, J.L., et al., The Ultraviolet Coronagraph Spectrometer for the Solar and Heliospheric Observatory, Sol. Phys., 162, 31, 1995.
5. Perry, R.M., and M.D. Altschuler, A fast technique for improved 3-dimensional mapping of the solar corona, Sol, Phys., 119, 301-321, 1989.
6. Zidowitz S., B. Inhester and A. Epple, Tomographic inversion of coronagraph images, in D. Winterhalter et al., in Solar Wind 8, AIP Conf. Proc. 382, 165-168, AIP Press, College Park, Md., 1996.