SCOPUS 정보 검색 플랫폼

Nature

Volumn 418, Issue 6894, 2002, Pages 157-159

Possible in situ formation of meteoritic nanodiamonds in the early Solar System

(6) Dai, Z R a Bradley, J P a Joswiak, D J b Brownlee, D E b Hill, H G M c Genge, M J d

a Georgia Institute of Technology ^* (United States)

b UNIVERSITY OF WASHINGTON (United States)

c NASA GODDARD SPACE FLIGHT CENTER (United States)

d DEPARTMENT OF LIFE SCIENCES (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

DIAMONDS; EARTH ATMOSPHERE; METEORITES;

PRESOLAR GRAINS;

SOLAR SYSTEM;

ASTRONOMY; METEORITE; SOLAR SYSTEM;

ARTICLE; ASTRONOMY; ATMOSPHERE; CIRCULATION; DUST; EVOLUTION; GRAIN; METEOROLOGICAL PHENOMENA; PRIORITY JOURNAL; SUN; VELOCITY;

ASTEROIDEA;

EID: 0037062995 PISSN: 00280836 EISSN: None Source Type: Journal
DOI: 10.1038/nature00897 Document Type: Article

Times cited : (154)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.