Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1992
|
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | 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 |
| Beschreibung: | 1 Online-Ressource (VI, 296 p) |
| ISBN: | 9789401730235 9789048142125 |
| DOI: | 10.1007/978-94-017-3023-5 |
Internformat
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| 245 | 1 | 0 | |a Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants |c edited by W. F. Huebner, J. J. Keady, S. P. Lyon |
| 264 | 1 | |a Dordrecht |b Springer Netherlands |c 1992 | |
| 300 | |a 1 Online-Ressource (VI, 296 p) | ||
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| 500 | |a 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 | ||
| 650 | 4 | |a Physics | |
| 650 | 4 | |a Meteorology | |
| 650 | 4 | |a Astrophysics and Astroparticles | |
| 650 | 4 | |a Meteorology/Climatology | |
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Datensatz im Suchindex
| _version_ | 1804153084665921536 |
|---|---|
| any_adam_object | |
| author | Huebner, W. F. |
| author_facet | Huebner, W. F. |
| author_role | aut |
| author_sort | Huebner, W. F. |
| author_variant | w f h wf wfh |
| building | Verbundindex |
| bvnumber | BV042416333 |
| classification_tum | PHY 000 |
| collection | ZDB-2-PHA ZDB-2-BAE |
| ctrlnum | (OCoLC)863976269 (DE-599)BVBBV042416333 |
| dewey-full | 523.01 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.01 |
| dewey-search | 523.01 |
| dewey-sort | 3523.01 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1007/978-94-017-3023-5 |
| format | Electronic eBook |
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| indexdate | 2024-07-10T01:20:59Z |
| institution | BVB |
| isbn | 9789401730235 9789048142125 |
| language | English |
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| spelling | Huebner, W. F. Verfasser aut Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants edited by W. F. Huebner, J. J. Keady, S. P. Lyon Dordrecht Springer Netherlands 1992 1 Online-Ressource (VI, 296 p) txt rdacontent c rdamedia cr rdacarrier 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 Physics Meteorology Astrophysics and Astroparticles Meteorology/Climatology Sternatmosphäre (DE-588)4183144-5 gnd rswk-swf Luftverschmutzung (DE-588)4074381-0 gnd rswk-swf Sonnenwind (DE-588)4135572-6 gnd rswk-swf Sonnenwind (DE-588)4135572-6 s 1\p DE-604 Luftverschmutzung (DE-588)4074381-0 s 2\p DE-604 Sternatmosphäre (DE-588)4183144-5 s 3\p DE-604 Keady, J. J. Sonstige oth Lyon, S. P. Sonstige oth https://doi.org/10.1007/978-94-017-3023-5 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 2\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 3\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Huebner, W. F. Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants Physics Meteorology Astrophysics and Astroparticles Meteorology/Climatology Sternatmosphäre (DE-588)4183144-5 gnd Luftverschmutzung (DE-588)4074381-0 gnd Sonnenwind (DE-588)4135572-6 gnd |
| subject_GND | (DE-588)4183144-5 (DE-588)4074381-0 (DE-588)4135572-6 |
| title | Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants |
| title_auth | Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants |
| title_exact_search | Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants |
| title_full | Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants edited by W. F. Huebner, J. J. Keady, S. P. Lyon |
| title_fullStr | Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants edited by W. F. Huebner, J. J. Keady, S. P. Lyon |
| title_full_unstemmed | Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants edited by W. F. Huebner, J. J. Keady, S. P. Lyon |
| title_short | Solar Photo Rates for Planetary Atmospheres and Atmospheric Pollutants |
| title_sort | solar photo rates for planetary atmospheres and atmospheric pollutants |
| topic | Physics Meteorology Astrophysics and Astroparticles Meteorology/Climatology Sternatmosphäre (DE-588)4183144-5 gnd Luftverschmutzung (DE-588)4074381-0 gnd Sonnenwind (DE-588)4135572-6 gnd |
| topic_facet | Physics Meteorology Astrophysics and Astroparticles Meteorology/Climatology Sternatmosphäre Luftverschmutzung Sonnenwind |
| url | https://doi.org/10.1007/978-94-017-3023-5 |
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