LUNAR-SURFACE MAGNETIC-FIELD CONCENTRATIONS ANTIPODAL TO YOUNG LARGE IMPACT BASINS

被引：53

作者：

LIN, RP

ANDERSON, KA

HOOD, LL

机构：

[1] UNIV CALIF BERKELEY, DEPT PHYS, BERKELEY, CA 94720 USA

[2] UNIV ARIZONA, LUNAR & PLANETARY LAB, TUCSON, AZ 85721 USA

来源：

ICARUS | 1988年 / 74卷 / 03期

关键词：

D O I：

10.1016/0019-1035(88)90119-4

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：529 / 541

页数：13

共 37 条

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HOOD, LL .

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[14] MAGNETIC-FIELD AMPLIFICATION AND GENERATION IN HYPER-VELOCITY METEOROID IMPACTS WITH APPLICATION TO LUNAR PALEOMAGNETISM [J].

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[15]

HOOD LL, 1981, 12TH P LUN PLAN SCI, P817

[16]

HOOD LL, 1978, P LUNAR PLANET SCI C, P3057

[17] ENERGETIC ELECTRON SCATTERING FROM THE LUNAR REMANENT MAGNETIC FIELD [J].

Howe, Herbert C. ;

Lin, R. P. ;

McGuire, R. E. ;

Anderson, K. A. .

GEOPHYSICAL RESEARCH LETTERS, 1974, 1 (03) :101-104

[18] CONSTRAINTS ON THE ORIGINS OF LUNAR MAGNETISM FROM ELECTRON REFLECTION MEASUREMENTS OF SURFACE MAGNETIC-FIELDS [J].

LIN, RP .

PHYSICS OF THE EARTH AND PLANETARY INTERIORS, 1979, 20 (2-4) :271-280

[19]

LIN RP, 1976, P LUNAR PLANET SCI C, P2691

[20]

LIN RP, 1979, P LUNAR PLANET SCI C, P2259

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