Integral spectrum of the sun as a star in the UV (0.1-0.32 micron) and IR (1-50 microns) regions

Details Integral spectrum of the sun as a star in the UV (0.1-0.32 micron) and IR (1-50 microns) regions Integral spectrum of the sun as a star in the UV (0.1-0.32 micron) and IR (1-50 microns) regions

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2....3b&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, July-Aug. 1986, p. 3-10. In Russian.

Astronomy and Astrophysics

Astronomy

Infrared Astronomy, Solar Spectra, Spectral Energy Distribution, Ultraviolet Astronomy, Lyman Alpha Radiation, Maxima, Minima, Solar Activity, Solar Cycles

Scientific paper

Studies on the spectral energy distribution of the sun as a star in the UV and IR ranges are reviewed. The standard distribution in the UV range is derived from an analysis of 11 series of independent observations primarily from cycles 20 and 21. It is shown that the series derived for the UV range differs somewhat from the Makarova-Kharitonov series (MKS), while the MKS remains the most reliable series for the IR range.

Affiliated with

Also associated with

No associations

Rating

Integral spectrum of the sun as a star in the UV (0.1-0.32 micron) and IR (1-50 microns) regions 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 Integral spectrum of the sun as a star in the UV (0.1-0.32 micron) and IR (1-50 microns) regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Integral spectrum of the sun as a star in the UV (0.1-0.32 micron) and IR (1-50 microns) regions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-893639