OXYGEN-TO-NEON ABUNDANCE RATIO IN SOLAR CORONA

被引：26

作者：

ACTON, LW ^{[1
]}

CATURA, RC ^{[1
]}

JOKI, EG ^{[1
]}

机构：

[1] LOCKHEED PALO ALTO RES LAB,RADIAT PHYS LAB,DEPT 52-14,BLDG 202,3251ST,PALO ALTO,CA 94304

来源：

关键词：

D O I：

10.1086/181718

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L93 / L95

页数：3

共 11 条

[1] BEIGMAN IL, 1971, SOV ASTRON, V14, P825
[2] NUCLEAR COMPOSITION AND ENERGY SPECTRA IN 1969 APRIL 12 SOLAR-PARTICLE EVENT
BERTSCH, DL
FICHTEL, CE
REAMES, DV
[J]. ASTROPHYSICAL JOURNAL, 1972, 171 (01) : 169 - &
[3] DUPREE AK, 1971, UNPUBLISHED RESULTS
[4] MALENOVSKY M, 1973, ASTROPHYS J, V181, P1009
[5] CALCULATED SOLAR X-RADIATION FROM 1 TO 60 A
MEWE, R
[J]. SOLAR PHYSICS, 1972, 22 (02) : 459 - &
[6] PARKINSON JH, 1971, THESIS U LEICESTER
[7] PARKINSON JH, 1974, IAU68 S BUEN AIR
[8] POTTASCH SR, 1967, B ASTRON I NETH, V19, P113
[9] RADIATION FROM A HIGH-TEMPERATURE, LOW-DENSITY PLASMA - X-RAY SPECTRUM OF SOLAR CORONA
TUCKER, WH
KOREN, M
[J]. ASTROPHYSICAL JOURNAL, 1971, 168 (02) : 283 - &
[10] RELATIVE CORONAL ABUNDANCES DERIVED FROM X-RAY OBSERVATIONS .2. NITROGEN, OXYGEN, NEON, MAGNESIUM, AND IRON
WALKER, ABC
RUGGE, HR
WEISS, K
[J]. ASTROPHYSICAL JOURNAL, 1974, 192 (01) : 169 - 180