Crossing the termination shock into the hetiosheath:: Magnetic fields

被引:216
作者
Burlaga, LF [1 ]
Ness, NF
Acuña, IH
Acuña, MH
Lepping, RP
Connerney, JEP
Stone, EC
McDonald, FB
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Catholic Univ Amer, Washington, DC 20064 USA
[3] CALTECH, Pasadena, CA 91109 USA
[4] Univ Maryland, Inst Phys Sci & Technol, College Pk, MD 20742 USA
关键词
D O I
10.1126/science.1117542
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
Magnetic fields measured by Voyager 1 show that the spacecraft crossed or was crossed by the termination shock on about 16 December 2004 at 94.0 astronomical units. An estimate of the compression ratio of the magnetic field strength B (+/- standard error of the mean) across the shock is B-2/B-1 = 3.05 +/- 0.04, but ratios in the range from 2 to 4 are admissible. The average B in the heliosheath from day 1 through day 110 of 2005 was 0.136 +/- 0.035 nanoteslas, similar to 4.2 times that predicted by Parker's model for B. The magnetic field in the heliosheath from day 361 of 2004 through day 110 of 2005 was pointing away from the Sun along the Parker spiral. The probability distribution of hourly averages of B in the heliosheath is a Gaussian distribution. The cosmic ray intensity increased when B was relatively large in the hetiosheath.
引用
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页码:2027 / 2029
页数:3
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