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Space Science Reviews

Volumn 143, Issue 1-4, 2009, Pages 253-262

What can be learned from x-ray spectroscopy concerning hot gas in the local bubble and charge exchange processes?

(1) Snowden, S L a

a NASA GODDARD SPACE FLIGHT CENTER (United States)

Author keywords

Interstellar medium; Solar system; X rays

Indexed keywords

ASTRONOMY; CHARGE TRANSFER; EMISSION SPECTROSCOPY; INSTRUMENTS; IONIZATION OF GASES; REMOTE SENSING; SOLAR EQUIPMENT; SOLAR WIND; SPECTRUM ANALYSIS; X RAY SPECTROMETERS; X RAY SPECTROSCOPY; X RAYS;

CHARGE EXCHANGE PROCESS; DYNAMIC INFORMATIONS; FUTURE MISSIONS; HIGH RESOLUTIONS; HIGHLY-IONIZED; HOT GAS; HOT PLASMAS; INTERSTELLAR MEDIUM; ION SPECIES; IONIZATION STATE; SOFT X-RAYS; SOLAR WIND CHARGE EXCHANGES; SPECTRAL SIGNATURES; THERMAL EMISSIONS; TWO SOURCES; X-RAY SPECTROSCOPIES;

SOLAR SYSTEM;

EID: 61449142776 PISSN: 00386308 EISSN: 15729672 Source Type: Journal
DOI: 10.1007/s11214-008-9343-2 Document Type: Article

Times cited : (14)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.