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

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

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999jgr...104.9721p&link_type=abstract

Journal of Geophysical Research, Volume 104, Issue A5, p. 9721-9726

Astronomy and Astrophysics

Astrophysics

19

Solar Physics, Astrophysics, And Astronomy

Scientific paper

UV coronal intensity data collected by the Ultraviolet Coronagraph Spectrometer on SOHO in a daily synoptic program during the Whole Sun Month are used to reconstruct the three-dimensional distribution of emissivities in the solar corona for H I Ly α and the O VI doublet at 1032 and 1037 Å. We discuss the specifics that complicate a tomographic reconstruction of the solar corona and estimate the uncertainties introduced in the reconstruction by them.

Affiliated with

Also associated with

No associations

Rating

Three-dimensional reconstruction of UV emissivities in the solar corona using Ultraviolet Coronagraph Spectrometer data from the Whole Sun Month 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 Three-dimensional reconstruction of UV emissivities in the solar corona using Ultraviolet Coronagraph Spectrometer data from the Whole Sun Month, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Three-dimensional reconstruction of UV emissivities in the solar corona using Ultraviolet Coronagraph Spectrometer data from the Whole Sun Month will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1377511