Author: H. E. Hinteregger
Publisher:
ISBN:
Category : Emission spectroscopy
Languages : en
Pages : 40
Book Description
Rocket Spectra of the Chromosphere
Author: H. E. Hinteregger
Publisher:
ISBN:
Category : Emission spectroscopy
Languages : en
Pages : 40
Book Description
Publisher:
ISBN:
Category : Emission spectroscopy
Languages : en
Pages : 40
Book Description
The Solar Spectrum
Author: C. de Jager
Publisher: Springer
ISBN: 9401763763
Category : Science
Languages : en
Pages : 423
Book Description
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.
Publisher: Springer
ISBN: 9401763763
Category : Science
Languages : en
Pages : 423
Book Description
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.
Theory of Stellar Spectra
Author: Viktor Viktorovich Sobolev
Publisher:
ISBN:
Category : Stars
Languages : en
Pages : 292
Book Description
Publisher:
ISBN:
Category : Stars
Languages : en
Pages : 292
Book Description
The Solar Spectrum
Author: Cornelis de Jager
Publisher:
ISBN:
Category : Spectrum, Solar
Languages : en
Pages : 440
Book Description
Publisher:
ISBN:
Category : Spectrum, Solar
Languages : en
Pages : 440
Book Description
NASA Technical Translation
Author:
Publisher:
ISBN:
Category : Science
Languages : en
Pages : 1296
Book Description
Publisher:
ISBN:
Category : Science
Languages : en
Pages : 1296
Book Description
Memoirs of the Royal Astronomical Society
Author: Royal Astronomical Society
Publisher:
ISBN:
Category : Astronomy
Languages : en
Pages : 854
Book Description
Publisher:
ISBN:
Category : Astronomy
Languages : en
Pages : 854
Book Description
Memoirs
Author: Royal Astronomical Society
Publisher:
ISBN:
Category :
Languages : en
Pages : 856
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages : 856
Book Description
Literature 1979, Part 1
Author: Siegfried Böhme
Publisher: Springer Science & Business Media
ISBN: 3662123169
Category : Science
Languages : en
Pages : 882
Book Description
Publisher: Springer Science & Business Media
ISBN: 3662123169
Category : Science
Languages : en
Pages : 882
Book Description
Thesaurus of Engineering and Scientific Terms
Author: Engineers Joint Council
Publisher:
ISBN:
Category : Engineering
Languages : en
Pages : 708
Book Description
Publisher:
ISBN:
Category : Engineering
Languages : en
Pages : 708
Book Description
Atomic and Ionic Spectra and Elementary Processes in Plasma
Author: Igorʹ Ilʹich Sobelʹman
Publisher: Nova Publishers
ISBN: 9781560720713
Category : Science
Languages : en
Pages : 188
Book Description
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
Publisher: Nova Publishers
ISBN: 9781560720713
Category : Science
Languages : en
Pages : 188
Book Description
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