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 [J].

HUNDHAUSEN, AJ ;

ASBRIDGE, JR ;

BAME, SJ ;

GILBERT, HE ;

STRONG, IB .

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 [J].

LYON, EF ;

BRIDGE, HS ;

BINSACK, JH .

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MEISTER J, UNPUBLISHED MEASUREM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 [J].

WOLFE, JH ;

SILVA, RW ;

MCKIBBIN, DD ;

MASON, RH .

JOURNAL OF GEOPHYSICAL RESEARCH, 1966, 71 (13) :3329-+

[10]

1969, SCIENCE, V165, P1211

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