APOLLO-11 SOLAR WIND COMPOSITION EXPERIMENT - FIRST RESULTS

被引：37

作者：

BUHLER, F

EBERHARD.P

GEISS, J

MEISTER, J

SIGNER, P

机构：

[1] Physikalisches Institut, University of Berne

[2] Institute of Crystallography and Petrography, Eidgenössische Technische Hochschule

来源：

SCIENCE | 1969年 / 166卷 / 3912期

关键词：

D O I：

10.1126/science.166.3912.1502

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

The helium-4 solar wind flux during the Apollo 11 lunar surface excursion was (6.3 ± 1.2) x 106 atoms per square centimeter per second. The solar wind direction and energy are essentially not perturbed by the moon. Evidence for a lunar solar wind albedo was found.

引用

页码：1502 / &

共 10 条

[1] AXFORD WI, 1968, SPACE SCI REV, V8, P331, DOI 10.1007/BF00184740
[2] VELA 3 SATELLITE OBSERVATIONS OF SOLAR WIND IONS - A PRELIMINARY REPORT
HUNDHAUSEN, AJ
ASBRIDGE, JR
BAME, SJ
GILBERT, HE
STRONG, IB
[J]. JOURNAL OF GEOPHYSICAL RESEARCH, 1967, 72 (01): : 87 - +
[3] HUNDHAUSEN AJ, 1968, SPACE SCI REV, V8, P690, DOI 10.1007/BF00175116
[4] EXPLORER 35 PLASMA MEASUREMENTS IN VICINITY OF MOON
LYON, EF
BRIDGE, HS
BINSACK, JH
[J]. JOURNAL OF GEOPHYSICAL RESEARCH, 1967, 72 (23): : 6113 - +
[5] MEISTER J, UNPUBLISHED MEASUREM
[6] ROBBINS DL, 1969, EOS T AM GEOPHYS UN, V50, P302
[7] SNYDER CW, 1964, P INT SPACE SCI S, V4, P89
[8] WGILVIE KW, 1969, SOLAR PHYSICS, V8, P435
[9] COMPOSITIONAL ANISOTROPIC AND NONRADIAL FLOW CHARACTERISTICS OF SOLAR WIND
WOLFE, JH
SILVA, RW
MCKIBBIN, DD
MASON, RH
[J]. JOURNAL OF GEOPHYSICAL RESEARCH, 1966, 71 (13): : 3329 - +
[10] 1969, SCIENCE, V165, P1211

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