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Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants - W.F. Huebner
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W.F. Huebner:
Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants - nieuw boek

ISBN: 9789048142125

ID: 978904814212

A quantitative measure of the accuracy of the rate coefficients and the excess energies is a desirable goal of this analysis. There are two major sources of uncertainties: The atomic and molecular data and the solar irradiance. The cross sections and branching ratios used in this analysis come from many different sources; many of them without any error indications. For this reason, we must confine ourselves to a qualitative indication of the reliability of the results. Specifically we give a quality scale in Table II for the data of each mother molecule; A indicating the highest quality of atomic and molecular data and F the lowest quality. The letter B typically means that the threshold is uncertain. For most molecules the cross section at threshold is very small and the rate coefficient for these molecules is therefore not influenced by this uncertainty. For atomic species the cross section is usually large near threshold, but for these species the threshold is known quite accurately. The letter B, therefore, indicates that the rate coefficient is most likely quite accurate, but the excess energy is less accurately known. The letter C usually means that the branching ratios are not well known. This means that the total rate coefficient is very good, but the rate coefficients and the excess energies for the individual branches are less accurate. W.F. Huebner, Books, Science and Nature, Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants Books>Science and Nature, Springer-Verlag/Sci-Tech/Trade

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Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants - W.F. Huebner; J.J. Keady; S.P. Lyon
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W.F. Huebner; J.J. Keady; S.P. Lyon:
Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants - pocketboek

ISBN: 9789048142125

ID: 9789048142125

A quantitative measure of the accuracy of the rate coefficients and the excess energies is a desirable goal of this analysis. There are two major sources of uncertainties: The atomic and molecular data and the solar irradiance. The cross sections and branching ratios used in this analysis come from many different sources; many of them without any error indications. For this reason, we must confine ourselves to a qualitative indication of the reliability of the results. Specifically we give a quality scale in Table II for the data of each mother molecule; A indicating the highest quality of atomic and molecular data and F the lowest quality. The letter B typically means that the threshold is uncertain. For most molecules the cross section at threshold is very small and the rate coefficient for these molecules is therefore not influenced by this uncertainty. For atomic species the cross section is usually large near threshold, but for these species the threshold is known quite accurately. The letter B, therefore, indicates that the rate coefficient is most likely quite accurate, but the excess energy is less accurately known. The letter C usually means that the branching ratios are not well known. This means that the total rate coefficient is very good, but the rate coefficients and the excess energies for the individual branches are less accurate. Books > Physics Soft cover, Springer Shop

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Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants
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Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants - pocketboek

ISBN: 9048142121

gebonden uitgave, ID: 13444809

Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants ab 200.49 € als Taschenbuch: Softcover reprint of hardcover 1st ed. 1992.. Aus dem Bereich: Bücher, Wissenschaft, Physik, Medien > Bücher, Springer Netherlands

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Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants als Buch von
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Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants als Buch von - pocketboek

ISBN: 9789048142125

gebonden uitgave, ID: 13444809

Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants ab 200.49 EURO Softcover reprint of hardcover 1st ed. 1992. Medien > Bücher, Springer Netherlands

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Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants - W.F. Huebner; J.J. Keady; S.P. Lyon
(*)
W.F. Huebner; J.J. Keady; S.P. Lyon:
Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants - nieuw boek

ISBN: 9789048142125

ID: 9789048142125

Physics; Astrophysics and Astroparticles; Atmospheric Sciences Planet, atmosphere, satellite, solar Books, Springer Nature

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Bijzonderheden over het boek
Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants

Unattenuated solar photo rate coefficient and excess energies for dissociation, ionization, and dissociative ionization are needed for atomic and molecular species that have been identified or are suspected to exist in the atmosphere of planets, satellites (moons), comets, or as pollutants in the Earth atmosphere. This book presents the branching ratios and cross sections with resonances and have been tabulated to the greatest detail possible and the rate coefficients and excess energies have been calculated from them on a grid of small wavelength bins for the quiet and the active Sun at 1 AU heliocentric distance.

Gedetalleerde informatie over het boek. - Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants


EAN (ISBN-13): 9789048142125
ISBN (ISBN-10): 9048142121
Gebonden uitgave
pocket book
Verschijningsjaar: 2010
Uitgever: Springer-Verlag/Sci-Tech/Trade
304 Bladzijden
Gewicht: 0,462 kg
Taal: eng/Englisch

Boek bevindt zich in het datenbestand sinds 05.05.2011 15:33:19
Boek voor het laatst gevonden op 13.02.2019 17:46:56
ISBN/EAN: 9789048142125

ISBN - alternatieve schrijfwijzen:
90-481-4212-1, 978-90-481-4212-5


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