書誌事項
- 公開日
- 2019-05-21
- 資源種別
- journal article
- 権利情報
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- http://www.springer.com/tdm
- http://www.springer.com/tdm
- DOI
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- 10.1007/s11214-019-0597-7
- 10.48350/156801
- 公開者
- Springer Science and Business Media LLC
この論文をさがす
説明
Interplanetary dust particles and meteoroids mostly originate from comets and asteroids. Understanding their distribution in the Solar system, their dynamical behavior and their properties, sheds light on the current state and the dynamical behavior of the Solar system. Dust particles can endanger Earth-orbiting satellites and deep-space probes, and a good understanding of the spatial density and velocity distribution of dust and meteoroids in the Solar system is important for designing proper spacecraft shielding. The study of interplanetary dust and meteoroids provides clues to the formation of the Solar system. Particles having formed 4.5 billion years ago can survive planetary accretion and those that survived until now did not evolve significantly since then. Meteoroids and interplanetary dust can be observed by measuring the intensity and polarization of the zodiacal light, by observing meteors entering the Earth’s atmosphere, by collecting them in the upper atmosphere, polar ices and snow, and by detecting them with in-situ detectors on space probes.
(Topical Collection: Cosmic Dust from the Laboratory to the Stars, Edited by Rafael Rodrigo, Jürgen Blum, Hsiang-Wen Hsu, Detlef Koschny, Anny-Chantal Levasseur-Regourd, Jesús Martín-Pintado, Veerle Sterken and Andrew Westphal)
International audience
収録刊行物
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- Space Science Reviews
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Space Science Reviews 215 (4), 34-, 2019-05-21
Springer Science and Business Media LLC
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キーワード
詳細情報 詳細情報について
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- CRID
- 1361412890933959936
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- ISSN
- 15729672
- 00386308
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- 資料種別
- journal article
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- データソース種別
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- Crossref
- KAKEN
- OpenAIRE
