Solar Composition and its Evolution — from Core to Corona: Proceedings of an ISSI Workshop 26–30 January 1998, Bern, Switzerland
Gespeichert in:
| Weitere Verfasser: | , |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1998
|
| Schriftenreihe: | Space Sciences Series of ISSI
5 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | The discovery of chemical elements in celestial bodies and the first estimates of the chemical composition of the solar atmosphere were early results of Astrophysics - the subdiscipline of Astronomy that was originally concerned with the general laws of radiation and with spectroscopy. Following the initial quantitative abundance studies by Henry Norris Russell and by Cecilia Payne-Gaposchkin, a tremendous amount of theoretical, observational, laboratory and computational work led to a steadily improving body of knowledge of photospheric abundances - a body of knowledge that served to guide the theory of stellar evolution. Solar abundances determined from photospheric spectra, together with the very similar abundances determined from carbonaceous chondrites (where extensive information on isotopic composition is available as well), are nowadays the reference for all cosmic composition measures. Early astrophysical studies of the solar photospheric composition made use of atmosphere models and atomic data. Consistent abundances derived from different atmospheric layers and from lines of different strength helped to confirm and establish both models and atomic data, and eventually led to the now accepted, so-called "absolute" abundance values - which, for practical reasons, however, are usually given relative to the number of hydrogen nuclei |
| Beschreibung: | 1 Online-Ressource (XII, 431 p) |
| ISBN: | 9789401148207 9789401060226 |
| ISSN: | 1385-7525 |
| DOI: | 10.1007/978-94-011-4820-7 |
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| 245 | 1 | 0 | |a Solar Composition and its Evolution — from Core to Corona |b Proceedings of an ISSI Workshop 26–30 January 1998, Bern, Switzerland |c edited by C. Fröhlich, M. C. E. Huber, S. K. Solanki, R. Steiger |
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| 500 | |a The discovery of chemical elements in celestial bodies and the first estimates of the chemical composition of the solar atmosphere were early results of Astrophysics - the subdiscipline of Astronomy that was originally concerned with the general laws of radiation and with spectroscopy. Following the initial quantitative abundance studies by Henry Norris Russell and by Cecilia Payne-Gaposchkin, a tremendous amount of theoretical, observational, laboratory and computational work led to a steadily improving body of knowledge of photospheric abundances - a body of knowledge that served to guide the theory of stellar evolution. Solar abundances determined from photospheric spectra, together with the very similar abundances determined from carbonaceous chondrites (where extensive information on isotopic composition is available as well), are nowadays the reference for all cosmic composition measures. Early astrophysical studies of the solar photospheric composition made use of atmosphere models and atomic data. Consistent abundances derived from different atmospheric layers and from lines of different strength helped to confirm and establish both models and atomic data, and eventually led to the now accepted, so-called "absolute" abundance values - which, for practical reasons, however, are usually given relative to the number of hydrogen nuclei | ||
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Datensatz im Suchindex
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| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 520 - Astronomy and allied sciences |
| dewey-raw | 520 |
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| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1007/978-94-011-4820-7 |
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| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:58Z |
| institution | BVB |
| isbn | 9789401148207 9789401060226 |
| issn | 1385-7525 |
| language | English |
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| spelling | Fröhlich, C. edt Solar Composition and its Evolution — from Core to Corona Proceedings of an ISSI Workshop 26–30 January 1998, Bern, Switzerland edited by C. Fröhlich, M. C. E. Huber, S. K. Solanki, R. Steiger Proceedings of an ISSI Workshop, 26-30 January 1998, Bern, Switzerland Dordrecht Springer Netherlands 1998 1 Online-Ressource (XII, 431 p) txt rdacontent c rdamedia cr rdacarrier Space Sciences Series of ISSI 5 1385-7525 The discovery of chemical elements in celestial bodies and the first estimates of the chemical composition of the solar atmosphere were early results of Astrophysics - the subdiscipline of Astronomy that was originally concerned with the general laws of radiation and with spectroscopy. Following the initial quantitative abundance studies by Henry Norris Russell and by Cecilia Payne-Gaposchkin, a tremendous amount of theoretical, observational, laboratory and computational work led to a steadily improving body of knowledge of photospheric abundances - a body of knowledge that served to guide the theory of stellar evolution. Solar abundances determined from photospheric spectra, together with the very similar abundances determined from carbonaceous chondrites (where extensive information on isotopic composition is available as well), are nowadays the reference for all cosmic composition measures. Early astrophysical studies of the solar photospheric composition made use of atmosphere models and atomic data. Consistent abundances derived from different atmospheric layers and from lines of different strength helped to confirm and establish both models and atomic data, and eventually led to the now accepted, so-called "absolute" abundance values - which, for practical reasons, however, are usually given relative to the number of hydrogen nuclei Physics Astronomy, Observations and Techniques Astrophysics and Astroparticles Huber, M. C. E. edt Solanki, S. K. Sonstige oth Steiger, R. Sonstige oth Space Sciences Series of ISSI 5 (DE-604)BV013841030 5 https://doi.org/10.1007/978-94-011-4820-7 Verlag Volltext |
| spellingShingle | Solar Composition and its Evolution — from Core to Corona Proceedings of an ISSI Workshop 26–30 January 1998, Bern, Switzerland Space Sciences Series of ISSI Physics Astronomy, Observations and Techniques Astrophysics and Astroparticles |
| title | Solar Composition and its Evolution — from Core to Corona Proceedings of an ISSI Workshop 26–30 January 1998, Bern, Switzerland |
| title_alt | Proceedings of an ISSI Workshop, 26-30 January 1998, Bern, Switzerland |
| title_auth | Solar Composition and its Evolution — from Core to Corona Proceedings of an ISSI Workshop 26–30 January 1998, Bern, Switzerland |
| title_exact_search | Solar Composition and its Evolution — from Core to Corona Proceedings of an ISSI Workshop 26–30 January 1998, Bern, Switzerland |
| title_full | Solar Composition and its Evolution — from Core to Corona Proceedings of an ISSI Workshop 26–30 January 1998, Bern, Switzerland edited by C. Fröhlich, M. C. E. Huber, S. K. Solanki, R. Steiger |
| title_fullStr | Solar Composition and its Evolution — from Core to Corona Proceedings of an ISSI Workshop 26–30 January 1998, Bern, Switzerland edited by C. Fröhlich, M. C. E. Huber, S. K. Solanki, R. Steiger |
| title_full_unstemmed | Solar Composition and its Evolution — from Core to Corona Proceedings of an ISSI Workshop 26–30 January 1998, Bern, Switzerland edited by C. Fröhlich, M. C. E. Huber, S. K. Solanki, R. Steiger |
| title_short | Solar Composition and its Evolution — from Core to Corona |
| title_sort | solar composition and its evolution from core to corona proceedings of an issi workshop 26 30 january 1998 bern switzerland |
| title_sub | Proceedings of an ISSI Workshop 26–30 January 1998, Bern, Switzerland |
| topic | Physics Astronomy, Observations and Techniques Astrophysics and Astroparticles |
| topic_facet | Physics Astronomy, Observations and Techniques Astrophysics and Astroparticles |
| url | https://doi.org/10.1007/978-94-011-4820-7 |
| volume_link | (DE-604)BV013841030 |
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