POSSIBLE DERIVATIONS OF ORTHO- AND PARA-H₂ RATIOS IN THE ATMOSPHERES OF THE GIANT PLANETS USING THE 2μm SPECTRAL STRUCTURES OF (H₂)₂ - koreascholar

논문 상세보기

POSSIBLE DERIVATIONS OF ORTHO- AND PARA-H₂ RATIOS IN THE ATMOSPHERES OF THE GIANT PLANETS USING THE 2μm SPECTRAL STRUCTURES OF (H₂)₂ KCI 등재 SCOPUS

Kim, Sang-Joon, Lee, Yong-Sik

언어ENG
URLhttps://db.koreascholar.com/Article/Detail/267141

서비스가 종료되어 열람이 제한될 수 있습니다.

Journal of Astronomy and Space Sciences

제18권 2호 (2001.11)
pp.95-100

한국우주과학회 (The Korean Space Science Society)

키워드

Planet Atmosphere Molecule Radiative Transfer Spectroscopy

저자

Kim, Sang-Joon(Department of Astronomy and Space Science Kyung Hee University)
Lee, Yong-Sik( Department of Chemistry Kyung Hee University Yong In, Kyun Gi Do,449-701 Korea) | Lee, Yong-Sik

같은 권호 다른 논문