Rocket Spectra of the Chromosphere
Author : H. E. Hinteregger
Publisher :
Page : 40 pages
File Size : 28,76 MB
Release : 1965
Category : Emission spectroscopy
ISBN :
Author : H. E. Hinteregger
Publisher :
Page : 40 pages
File Size : 28,76 MB
Release : 1965
Category : Emission spectroscopy
ISBN :
Author : C. de Jager
Publisher : Springer
Page : 423 pages
File Size : 49,30 MB
Release : 2013-11-11
Category : Science
ISBN : 9401763763
A good deal of our information on solar physics and on solar phenomena is derived from the solar spectrum. A quantitative interpretation of this spectrum was only possible after 1920, after the establishment of Bohr's atomic model, the discovery of Saha's law, and the development of spectrophotometry. The resolving and light gathering powers of our instruments have greatly increased since. We have seen an enormous progress in our theoretical under standing of basic atomic phenomena, and of the intricate problems concerned with the transfer of energy through a complicated structure like the sun's outer layers. In particular the observable part of the solar spectrum tremen dously enlarged since the introduction, in the years after 1945, of radio astronomy, enabling us to study the solar spectrum between wavelengths of some mm to about 15 m, of space research, giving access to the whole electro magnetic spectrum below 3000 A, down to about 0. 01 A. Further, the low and high energetic components of the solar particles spectrum have been dis covered with space probes (the solar wind), rockets, balloons (the so-called sub cosmic-ray particles) and cosmic ray monitors (solar cosmic ray bursts). The extreme wealth of this spectrum, much vaster in extent than the earlier investigators could only dream of, is an important source of information. It looked appropriate to us, after the rapid development of this branch of science, ' to invite the world's leading solar physicists to Utrecht for a summa rizing symposium on the whole solar spectrum.
Author : Cornelis de Jager
Publisher :
Page : 440 pages
File Size : 13,42 MB
Release : 1965
Category : Spectrum, Solar
ISBN :
Author : Viktor Viktorovich Sobolev
Publisher :
Page : 292 pages
File Size : 24,42 MB
Release : 1967
Category : Stars
ISBN :
Author : Katharine B. Gebbie
Publisher :
Page : 218 pages
File Size : 10,48 MB
Release : 1971
Category : Astrophysics
ISBN :
Author :
Publisher :
Page : 1296 pages
File Size : 13,82 MB
Release : 1969
Category : Science
ISBN :
Author : Siegfried Böhme
Publisher : Springer Science & Business Media
Page : 882 pages
File Size : 15,2 MB
Release : 2013-04-18
Category : Science
ISBN : 3662123169
Author : Engineers Joint Council
Publisher :
Page : 708 pages
File Size : 29,25 MB
Release : 1967
Category : Engineering
ISBN :
Author : Igorʹ Ilʹich Sobelʹman
Publisher : Nova Publishers
Page : 188 pages
File Size : 11,73 MB
Release : 1992
Category : Science
ISBN : 9781560720713
Eight highly technical studies explore a wide range of problems involved in investigating the short wavelength emission of the solar corona. The topics include the experimental results from solar X-ray investigations, the calculated excitation cross-sections for collisions of atoms and ions with charged particles, and spectra of plasmas. Annotation
Author : United States. National Bureau of Standards
Publisher :
Page : 572 pages
File Size : 45,35 MB
Release : 1980
Category : Chemistry
ISBN :