The Infrared Handbook
Author | : Environmental Research Institute of Michigan. Infrared Information and Analysis Center |
Publisher | : |
Total Pages | : 1740 |
Release | : 1978 |
Genre | : Infrared radiation |
ISBN | : |
Download Observations Of The Infrared Sunspot Spectrum Between 11340a And 24778a full books in PDF, epub, and Kindle. Read online free Observations Of The Infrared Sunspot Spectrum Between 11340a And 24778a ebook anywhere anytime directly on your device. Fast Download speed and no annoying ads. We cannot guarantee that every ebooks is available!
Author | : Environmental Research Institute of Michigan. Infrared Information and Analysis Center |
Publisher | : |
Total Pages | : 1740 |
Release | : 1978 |
Genre | : Infrared radiation |
ISBN | : |
Author | : Smithsonian Astrophysical Observatory |
Publisher | : |
Total Pages | : 602 |
Release | : 1976 |
Genre | : Artificial satellites |
ISBN | : |
Author | : Gerald M. Stokes |
Publisher | : |
Total Pages | : 128 |
Release | : 1984 |
Genre | : Atmospheric carbon dioxide |
ISBN | : |
Author | : R. A. McClatchey |
Publisher | : |
Total Pages | : 92 |
Release | : 1973 |
Genre | : Absorption spectra |
ISBN | : |
The report describes a compilation of the molecular spectroscopic parameters for a number of infrared-active molecules occurring naturally in the terrestrial atmsophere. The following molecules are included in this compilation: water vapor; carbon dioxide; ozone; nitrous oxide; carbon monoxide; methane; and oxygen. The spectral region covered extends from less than 1 micrometer to the far infrared, and data are presented on more than 100, 000 spectral lines. The parameters included in the compilation for each line are: frequency, intensity, half-width, energy of the lower state of the transition, vibrational and rotational identifications of the upper and lower energy states, an isotopic identification, and a molecular identification. A discussion is provided separately for each molecular species, indicating the sources and accuracy of the data and a general discussion of how the data were obtained.
Author | : C. de Jager |
Publisher | : Springer Science & Business Media |
Total Pages | : 383 |
Release | : 2012-12-06 |
Genre | : Science |
ISBN | : 9401031053 |
The changing character of the IAU General Assemblies becomes most clear from a comparison of the agenda of the Brighton meeting with that of one of the earlier meetings. The fourth General Assembly (Cambridge Mass. , 1932) had about 240 participants, registered guests included, the Brighton meeting had about 2300 people attending. The Cambridge meeting lasted 5, working days, of which, however, three half days were exclusively devoted to excursions, leaving four real meeting days. At that time the nearly 30 commissions had each only one meeting, during part of a morning or afternoon; some commissions did not meet at all. There was one public lecture, by Sir Arthur Eddington, on 'The Expanding Universe'. Most of the small European countries were represented by two or three delegates only, but the delegations of France and Great Britain were composed of 20 and 18 scientists respectively; at that time there were only two delegates from Germany. After the Brighton General Assembly, with about 200 commission meetings - one commission met eleven times! - six Joint Discussions, four Invited Discourses, a Special Meeting and hardly time for excursions, there were a few complaints about too many overlapping meetings.
Author | : R.R. Bowker Company. Department of Bibliography |
Publisher | : |
Total Pages | : 2258 |
Release | : 1978 |
Genre | : United States |
ISBN | : |
Author | : Peter Ulmschneider |
Publisher | : Springer Science & Business Media |
Total Pages | : 663 |
Release | : 2013-06-29 |
Genre | : Science |
ISBN | : 364287455X |
One of the great problems of astrophysics is the unanswered question about the origin and mechanism of chromospheric and coronal heating. Just how these outer stellar envelopes are heated is of fundamental importance, since all stars have hot chromospheric and coronal shells where the temperature rises to millions of degrees, comparable to the temperatures in the stars' cores. Here for the first time is a comprehensive inventory of the proposed chromospheric and coronal heating theories. The proposed heating processes are critically compared, and the observational evidence for the various mechanisms is reviewed. This is essential reading for all those working in such fields as stellar activity, radio and XUV emission, rotation, and mass loss, for whom a detailed and consistent presentation of our knowledge of chromospheric and coronal heating mechanisms is urgently needed.
Author | : Kitt Peak National Observatory |
Publisher | : |
Total Pages | : 158 |
Release | : 1970 |
Genre | : Astronomy |
ISBN | : |