SUGGESTED ZODIACAL LIGHT MEASUREMENTS FROM SPACE PROBES

被引：19

作者：

GIESE, RH

VONDZIEM.C

机构：

[1] Bereich extraterrestrische Physik, Ruhr-Universität Bochum

[2] Max-Planck-Institut für extraterrestrische Physik, Garching b. München

来源：

PLANETARY AND SPACE SCIENCE | 1969年 / 17卷 / 05期

关键词：

D O I：

10.1016/0032-0633(69)90100-7

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Zodiacal light measurements including higher ecliptical latitudes can be fairly approximated by Mie-scattering of interplanetary dust particles in the mun size range (0.3 - 19 μ in dia.). Measurements of brightness and polarization from space probes will provide valuable information on the spatial distribution of dust including possible differences between the distribution of absorbing and dielectric particles. © 1969.

引用

页码：949 / &

共 12 条

[1]

ALLER LH, 1967, NASA SP150, P243

[2]

Blackwell D.E., 1967, ADV ASTRON ASTROPHYS, V5, P1

[3]

Giese R., 1963, SPACE SCI REV, V1, P589, DOI 10.1007/BF00225274

[4]

GIESE RH, 1962, Z ASTROPHYS, V54, P200

[5]

GIFSE RH, 1967, NASA150 SPEC REP, P271

[6] OBSERVATIONS OF THE ZODIACAL LIGHT FROM A VERY HIGH ALTITUDE STATION .4. THE NATURE AND DISTRIBUTION OF THE INTERPLANETARY DUST [J].

INGHAM, MF .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1961, 122 (02) :157-176

[7] ABSOLUTE PHOTOMETRY OF ZODIACAL LIGHT [J].

SMITH, LL ;

ROACH, FE ;

OWEN, RW .

PLANETARY AND SPACE SCIENCE, 1965, 13 (03) :207-&

[8]

van de Hulst H.C., 1981, LIGHT SCATTERING SMA

[9]

WEINBERG JL, 1964, ANN ASTROPHYS, V27, P718

[10]

WEINBERG JL, 1967, NASA150 SPEC REP ED, P271

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