Properties and Interactions of Interplanetary Dust: Proceedings of the 85th Colloquium of the International Astronomical Union, Marseille, France, July 9–12, 1984
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1985
|
| Schriftenreihe: | Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews
119 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | Investigation of the interplanetary dust cloud is characterized by contributions from quite different methods and fields, such as research on zodiacal light, meteors, micrometeoroids, asteroids, and comets. Since the earth's environment and interplanetary space became accessible to space vehicles these interrelations are clearly evident and extremely useful. Space measurements by micrometeoroid detectors, for example, provide individual and eventually detailed information on impact events, which however are limited in number and therefore restricted in statistical significance. On the other hand, zodiacal light measurements involve scattered light from many particles and therefore provide global information about the average values of physical properties and spatial distribution of interplanetary grains. Additional knowledge stems from lunar samples and from dust collections in the atmosphere and in deep sea sediments. All these sources of complementary information must be put together into a synoptical synthesis. This also has to take into account dynamical aspects and the results of laboratory investigations concerning physical properties of small grains. Such considerable effort is not merely an academic exercise for a few specialists interested in the solar dust cloud. Since this same cloud exclusively allows direct in-situ acess to investigate extraterrestrial dust particles over a wide range of sizes and materials, it provides valuable information for realistic treatment of dust phenomena in other remote cosmic regions such as in dense molecular clouds, circumstellar dust shells, and even protostellar or protoplanetary systems |
| Beschreibung: | 1 Online-Ressource (XXVI, 444 p) |
| ISBN: | 9789400954649 9789401089128 |
| ISSN: | 0067-0057 |
| DOI: | 10.1007/978-94-009-5464-9 |
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| 245 | 1 | 0 | |a Properties and Interactions of Interplanetary Dust |b Proceedings of the 85th Colloquium of the International Astronomical Union, Marseille, France, July 9–12, 1984 |c edited by R. H. Giese, P. Lamy |
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| 500 | |a Investigation of the interplanetary dust cloud is characterized by contributions from quite different methods and fields, such as research on zodiacal light, meteors, micrometeoroids, asteroids, and comets. Since the earth's environment and interplanetary space became accessible to space vehicles these interrelations are clearly evident and extremely useful. Space measurements by micrometeoroid detectors, for example, provide individual and eventually detailed information on impact events, which however are limited in number and therefore restricted in statistical significance. On the other hand, zodiacal light measurements involve scattered light from many particles and therefore provide global information about the average values of physical properties and spatial distribution of interplanetary grains. Additional knowledge stems from lunar samples and from dust collections in the atmosphere and in deep sea sediments. All these sources of complementary information must be put together into a synoptical synthesis. This also has to take into account dynamical aspects and the results of laboratory investigations concerning physical properties of small grains. Such considerable effort is not merely an academic exercise for a few specialists interested in the solar dust cloud. Since this same cloud exclusively allows direct in-situ acess to investigate extraterrestrial dust particles over a wide range of sizes and materials, it provides valuable information for realistic treatment of dust phenomena in other remote cosmic regions such as in dense molecular clouds, circumstellar dust shells, and even protostellar or protoplanetary systems | ||
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Datensatz im Suchindex
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| 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 | 10.1007/978-94-009-5464-9 |
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| spelling | Giese, R. H. Verfasser aut Properties and Interactions of Interplanetary Dust Proceedings of the 85th Colloquium of the International Astronomical Union, Marseille, France, July 9–12, 1984 edited by R. H. Giese, P. Lamy Dordrecht Springer Netherlands 1985 1 Online-Ressource (XXVI, 444 p) txt rdacontent c rdamedia cr rdacarrier Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews 119 0067-0057 Investigation of the interplanetary dust cloud is characterized by contributions from quite different methods and fields, such as research on zodiacal light, meteors, micrometeoroids, asteroids, and comets. Since the earth's environment and interplanetary space became accessible to space vehicles these interrelations are clearly evident and extremely useful. Space measurements by micrometeoroid detectors, for example, provide individual and eventually detailed information on impact events, which however are limited in number and therefore restricted in statistical significance. On the other hand, zodiacal light measurements involve scattered light from many particles and therefore provide global information about the average values of physical properties and spatial distribution of interplanetary grains. Additional knowledge stems from lunar samples and from dust collections in the atmosphere and in deep sea sediments. All these sources of complementary information must be put together into a synoptical synthesis. This also has to take into account dynamical aspects and the results of laboratory investigations concerning physical properties of small grains. Such considerable effort is not merely an academic exercise for a few specialists interested in the solar dust cloud. Since this same cloud exclusively allows direct in-situ acess to investigate extraterrestrial dust particles over a wide range of sizes and materials, it provides valuable information for realistic treatment of dust phenomena in other remote cosmic regions such as in dense molecular clouds, circumstellar dust shells, and even protostellar or protoplanetary systems Physics Astrophysics and Astroparticles Interplanetarer Staub (DE-588)4162118-9 gnd rswk-swf 1\p (DE-588)1071861417 Konferenzschrift 1984 Marseille gnd-content Interplanetarer Staub (DE-588)4162118-9 s 2\p DE-604 Lamy, P. Sonstige oth https://doi.org/10.1007/978-94-009-5464-9 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 |
| spellingShingle | Giese, R. H. Properties and Interactions of Interplanetary Dust Proceedings of the 85th Colloquium of the International Astronomical Union, Marseille, France, July 9–12, 1984 Physics Astrophysics and Astroparticles Interplanetarer Staub (DE-588)4162118-9 gnd |
| subject_GND | (DE-588)4162118-9 (DE-588)1071861417 |
| title | Properties and Interactions of Interplanetary Dust Proceedings of the 85th Colloquium of the International Astronomical Union, Marseille, France, July 9–12, 1984 |
| title_auth | Properties and Interactions of Interplanetary Dust Proceedings of the 85th Colloquium of the International Astronomical Union, Marseille, France, July 9–12, 1984 |
| title_exact_search | Properties and Interactions of Interplanetary Dust Proceedings of the 85th Colloquium of the International Astronomical Union, Marseille, France, July 9–12, 1984 |
| title_full | Properties and Interactions of Interplanetary Dust Proceedings of the 85th Colloquium of the International Astronomical Union, Marseille, France, July 9–12, 1984 edited by R. H. Giese, P. Lamy |
| title_fullStr | Properties and Interactions of Interplanetary Dust Proceedings of the 85th Colloquium of the International Astronomical Union, Marseille, France, July 9–12, 1984 edited by R. H. Giese, P. Lamy |
| title_full_unstemmed | Properties and Interactions of Interplanetary Dust Proceedings of the 85th Colloquium of the International Astronomical Union, Marseille, France, July 9–12, 1984 edited by R. H. Giese, P. Lamy |
| title_short | Properties and Interactions of Interplanetary Dust |
| title_sort | properties and interactions of interplanetary dust proceedings of the 85th colloquium of the international astronomical union marseille france july 9 12 1984 |
| title_sub | Proceedings of the 85th Colloquium of the International Astronomical Union, Marseille, France, July 9–12, 1984 |
| topic | Physics Astrophysics and Astroparticles Interplanetarer Staub (DE-588)4162118-9 gnd |
| topic_facet | Physics Astrophysics and Astroparticles Interplanetarer Staub Konferenzschrift 1984 Marseille |
| url | https://doi.org/10.1007/978-94-009-5464-9 |
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