Magnetic Field Observations as Voyager 1 Entered the Heliosheath Depletion Region

被引:152
|
作者
Burlaga, L. F. [1 ]
Ness, N. F. [2 ]
Stone, E. C. [3 ]
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Catholic Univ Amer, Washington, DC 20064 USA
[3] CALTECH, Pasadena, CA 91125 USA
关键词
TERMINATION SHOCK; HELIOSPHERE; VELOCITY; PLASMA; SYSTEM; FLOW; AU;
D O I
10.1126/science.1235451
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 (V1) show that the spacecraft crossed the boundary of an unexpected region five times between days 210 and similar to 238 in 2012. The magnetic field strength B increased across this boundary from approximate to 0.2 to approximate to 0.4 nanotesla, and B remained near 0.4 nanotesla until at least day 270, 2012. The strong magnetic fields were associated with unusually low counting rates of >0.5 mega-electron volt per nuclear particle. The direction of B did not change significantly across any of the five boundary crossings; it was very uniform and very close to the spiral magnetic field direction, which was observed throughout the heliosheath. The observations indicate that V1 entered a region of the heliosheath (the heliosheath depletion region), rather than the interstellar medium.
引用
收藏
页码:147 / 150
页数:4
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