Astronomy and Astrophysics – Astronomy
Scientific paper
May 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002apj...570..408f&link_type=abstract
The Astrophysical Journal, Volume 570, Issue 1, pp. 408-422.
Astronomy and Astrophysics
Astronomy
38
Methods: Data Analysis, Sun: Corona
Scientific paper
Solar rotational tomography is used to determine the three-dimensional electron density distribution of the solar corona from 2.4 to 6.0 Rsolar. The robust, regularized, positive estimation method, described in a previous paper, is demonstrated on test cases and on LASCO-C2 data. Because the solar rotational pole is inclined to the plane of the ecliptic by about 7°, the tomographic inversion requires a full three-dimensional treatment instead of a series of two-dimensional inversions. The LASCO data are taken from the first Whole Sun Month, which was a period of low solar activity.
Frazin Richard A.
Janzen Paul
No associations
LandOfFree
Tomography of the Solar Corona. II. Robust, Regularized, Positive Estimation of the Three-dimensional Electron Density Distribution from LASCO-C2 Polarized White-Light Images does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Tomography of the Solar Corona. II. Robust, Regularized, Positive Estimation of the Three-dimensional Electron Density Distribution from LASCO-C2 Polarized White-Light Images, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Tomography of the Solar Corona. II. Robust, Regularized, Positive Estimation of the Three-dimensional Electron Density Distribution from LASCO-C2 Polarized White-Light Images will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1727222