TOPICAL REVIEW The solar UV-x-ray spectrum from 1.5 to 2000 Å

Details TOPICAL REVIEW The solar UV-x-ray spectrum from 1.5 to 2000 Å TOPICAL REVIEW The solar UV-x-ray spectrum from 1.5 to 2000 Å

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010jphb...43w2001d&link_type=abstract

Journal of Physics B: Atomic, Molecular, and Optical Physics, Volume 43, Issue 23, pp. 232001 (2010).

Physics

1

Scientific paper

This review illustrates the potential of UV-x-ray spectroscopy for determining the physical conditions in the solar chromosphere, transition region and corona, and how spectroscopy can be used as a tool to understand the physical mechanisms governing the atmosphere. It also illustrates the potential for understanding transient events such as solar flares. This is a vast topic, and therefore the review is necessarily not complete, but we have tried to be as general as possible in showing in particular how solar spectra are currently being used to understand the solar upper atmosphere. The review is intended for non-solar physicists with an interest in spectroscopy as well as for solar physicists who are not specialists in spectroscopy.

Affiliated with

Also associated with

No associations

Rating

TOPICAL REVIEW The solar UV-x-ray spectrum from 1.5 to 2000 Å 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 TOPICAL REVIEW The solar UV-x-ray spectrum from 1.5 to 2000 Å, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and TOPICAL REVIEW The solar UV-x-ray spectrum from 1.5 to 2000 Å will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1297789