DUST MEASUREMENTS AT HIGH ECLIPTIC LATITUDES

被引:31
作者
BAGUHL, M
HAMILTON, DP
GRUN, E
DERMOTT, SF
FECHTIG, H
HANNER, MS
KISSEL, J
LINDBLAD, BA
LINKERT, D
LINKERT, G
MANN, I
MCDONNELL, JAM
MORFILL, GE
POLANSKEY, C
RIEMANN, R
SCHWEHM, G
STAUBACH, P
ZOOK, HA
机构
[1] UNIV FLORIDA, GAINESVILLE, FL 32611 USA
[2] JET PROPULS LAB, PASADENA, CA 91109 USA
[3] MAX PLANCK INST AERON, D-37191 KATLENBURG DUHM, GERMANY
[4] LUND OBSERV, S-221 LUND, SWEDEN
[5] UNIV KENT, CANTERBURY CT2 7NR, KENT, ENGLAND
[6] MAX PLANCK INST EXTRATERR PHYS, D-85748 GARCHING, GERMANY
[7] EUROPEAN SPACE TECHNOL CTR, 2200 AG NOORDWIJK, NETHERLANDS
[8] NASA, LYNDON B JOHNSON SPACE CTR, HOUSTON, TX 77058 USA
关键词
D O I
10.1126/science.268.5213.1016
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
Along Ulysses' path from Jupiter to the south ecliptic pole, the onboard dust detector measured a dust impact rate that varied slowly from 0.2, to 0.5 impacts per day. The dominant component of the dust flux arrived from an ecliptic latitude and longitude of 10 degrees +/- 10 degrees and 280 degrees +/- 30 degrees which indicates an interstellar origin. An additional flux of small particles, which do not come from the interstellar direction and are unlikely to be zodiacal dust grains, appeared south of -45 degrees latitude. One explanation is that these particles are beta-meteoroids accelerated away from the sun by radiation pressure and electromagnetic forces.
引用
收藏
页码:1016 / 1019
页数:4
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