Magnetic Field Observations as Voyager 1 Entered the Heliosheath Depletion Region

被引:157
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
相关论文
共 27 条
[1]  
Behannon K., 1997, SPACE SCI REV, V21, P235
[2]  
Berdichevsky D. B., 2009, White Paper, Voyager Mission, Detailed Processing of Weak Magnetic Fields IConstraints to the Uncertainties of the Calibrated Magnetic Field Signal in the Voyager Missions
[3]   Consequences of the heliopause instability caused by charge exchange [J].
Borovikov, Sergey N. ;
Pogorelov, Nikolai V. ;
Zank, Gary P. ;
Kryukov, Igor A. .
ASTROPHYSICAL JOURNAL, 2008, 682 (02) :1404-1415
[4]   HELIOSHEATH MAGNETIC FIELDS BETWEEN 104 AND 113 AU IN A REGION OF DECLINING SPEEDS AND A STAGNATION REGION [J].
Burlaga, L. F. ;
Ness, N. F. .
ASTROPHYSICAL JOURNAL, 2012, 749 (01)
[5]   Current sheets in the heliosheath: Voyager 1, 2009 [J].
Burlaga, L. F. ;
Ness, N. F. .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2011, 116
[6]   Crossing the termination shock into the hetiosheath:: Magnetic fields [J].
Burlaga, LF ;
Ness, NF ;
Acuña, IH ;
Acuña, MH ;
Lepping, RP ;
Connerney, JEP ;
Stone, EC ;
McDonald, FB .
SCIENCE, 2005, 309 (5743) :2027-2029
[7]   Voyager 1 in the foreshock, termination shock, and heliosheath [J].
Decker, RB ;
Krimigis, SM ;
Roelof, EC ;
Hill, ME ;
Armstrong, TP ;
Gloeckler, G ;
Hamilton, DC ;
Lanzerotti, LJ .
SCIENCE, 2005, 309 (5743) :2020-2024
[8]   No meridional plasma flow in the heliosheath transition region [J].
Decker, Robert B. ;
Krimigis, Stamatios M. ;
Roelof, Edmond C. ;
Hill, Matthew E. .
NATURE, 2012, 489 (7414) :124-127
[9]   Heliopause stability in the presence of neutral atoms: Rayleigh-Taylor dispersion analysis and axisymmetric MHD simulations [J].
Florinski, V ;
Zank, GP ;
Pogorelov, NV .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2005, 110 (A7)
[10]  
Frisch P. C., 2012, P 10 ANN INT ASTR C, V1436, P239