Download Astrophysik V: Verschiedenes / Astrophysics V: Miscellaneous by R. R. Mcmath, O. C. Mohler (auth.), S. Flügge (eds.) PDF

By R. R. Mcmath, O. C. Mohler (auth.), S. Flügge (eds.)

Show description

Read or Download Astrophysik V: Verschiedenes / Astrophysics V: Miscellaneous PDF

Best astrophysics & space science books

The Emission-Line Universe

This ebook provides lectures through prestigious researchers and skilled observers from the eighteenth wintry weather college of the Canary Islands Astrophysics Institute (IAC), dedicated to emission strains and the astrophysical gadgets that produce them. It indicates how emission strains in numerous wavelengths, from ultraviolet to close infrared, offers crucial info on realizing the formation and evolution of astrophysical gadgets, from the 1st stars to things in our Galaxy.

Astronomy and History Selected Essays

The gathering of papers assembled the following on numerous themes in old and medieval astronomy used to be initially prompt via Noel Swerdlow of the collage of Chicago. He used to be additionally instrumental in creating a choice* which might, more often than not, be at the comparable point as my e-book the precise Sciences in Antiquity.

The Mathematical Theory of Black Holes

This quantity has turn into one of many smooth classics of relativity thought. whilst it used to be written in 1983 there has been little actual proof for the lifestyles of black holes. contemporary discoveries have purely served to underscore the dependent conception constructed the following, and the publication continues to be one of many clearest statements of the appropriate arithmetic.

Extra info for Astrophysik V: Verschiedenes / Astrophysics V: Miscellaneous

Sample text

14, 337 (1927). Sect. 12. 25 Spectroscopes. mirror. This circumstance, and the use of paraboloidal mirrors for the concaves, limits the field of view to nearly a single spectrum line. The design provides a wider choice of positions for the dispersing element (grating or prism) than is the case for the Ebert system. A limited extent of the focal surface of good image quality is a common characteristic of all plane grating spectroscopes in use for solar research. The range of wavelengths covered at adequate plate scale (not less than t A/mm for usual solar work) is not more than a few hundred angstroms at best, but for many types of observation of the Sun it would be desirable to record the entire photographic spectrum from 13000 to 2900 A at high dispersion and high resolving power.

And others: Vistas in Astronomy, ed. by A. BEER, Vol. 1, p. 400. London and New York: Pergamon Press 1955. - Several sections contain discussions by different authors of instruments and instrumental problems of solar astronomy. The section by H. VON KLUBER: "Spectroscopic Measurements of Magnetic Fields on the Sun" is exceptionally complete. , and R. v. D. R. WOOLEY: Eclipses of the Sun and Moon, Chap. 9, p. 57. Oxford: Clarendon Press 1937. - Brief descriptions of some of the important instruments used for solar observation at eclipse time.

18. Table. Solar tower teleBlank spaces in the table remain where information to fill them could not be obtained. - Only solar tower telescopes are listed. It is intended to supplement the information in the table by H. GOLLNOW (Naturwiss. 36, 175, 213 (1949)], and to give data for solar tower telescopes not completed at the date of GOLLNOW'S compilation. The telescopes are a) Coelostats. 5 m tower University of Michigan 1940 15 Kanzelhohe University of Graz 1947 16 Rome Monte Mario 1948 17 Capri Fraunhofer Institut 1953 30 18 Co.

Download PDF sample

Rated 4.01 of 5 – based on 24 votes