Excerpt from Further Tests of Stellar Radiometers and Some Measurements of Planetary Radiation
The purpose of the present paper is to describe improvement in the radiometric apparatus used and the results (of interest to physicists) of some preliminary measurements of planetary radia tion as well as a verification of the measurements obtained a year ago in determining stellar temperatures by means of spectral transmission screens.
In this connection it is relevant to point out that the results obtained in mapping the spectral energy distribution of a' star by means of a spectrobolometer may not be essentially different from those obtained by the use of transmission screens. For, as may be seen from inspection of photographs of stellar spectra, the spectrum of a star consists of a bright continuous background superposed upon a series of absorption (and in some cases bright emission) lines. Hence, unless a very large dispersion can be used, the spectrobolometer will merely bridge over wide regions of the spectrum containing bright and dark bands. The spectral transmission screen does practically the same thing, in the sense that it integrates the energy present in a certain spectral region (without indicating the amount lost in the spectral absorption lines) and has the advantage of utilizing perhaps 40 per cent of the total intensity of the incident radiations, which is lost by employing a spectroscope.
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Paperback. Condizione: New. Print on Demand. This book explores the testing of our solar system's stars, the moon, and various planets using radiometers and spectral transmission screens. The author was provided an opportunity to continue their research on stellar and planetary thermal radiation, which they had previously pursued in 1921. The aim of this endeavor was to obtain insights into these celestial bodies' spectral energy distribution and effective temperatures and contribute to the broader understanding of the thermal properties of the planets, the moon, and certain types of stars. The findings suggest that the outer atmosphere of Jupiter does not gain sufficient heat to noticeably emit long wavelength radiation. What's more, the intensity of this low wavelength (7 to 12 micrometer) radiation increases as the density of the surrounding atmosphere decreases. This book will appeal to astronomy enthusiasts, scientists, and anyone seeking to broaden their knowledge of our solar system and the methods used to study it. This book is a reproduction of an important historical work, digitally reconstructed using state-of-the-art technology to preserve the original format. In rare cases, an imperfection in the original, such as a blemish or missing page, may be replicated in the book. print-on-demand item. Codice articolo 9781334253997_0
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Da: PBShop.store US, Wood Dale, IL, U.S.A.
PAP. Condizione: New. New Book. Shipped from UK. Established seller since 2000. Codice articolo LW-9781334253997
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Da: PBShop.store UK, Fairford, GLOS, Regno Unito
PAP. Condizione: New. New Book. Shipped from UK. Established seller since 2000. Codice articolo LW-9781334253997
Quantità: 15 disponibili