Magnetic Field and Plasma Density Observations of a Pressure Front by Voyager 1 during 2020 in the Very Local Interstellar Medium

被引:22
|
作者
Burlaga, L. F. [1 ]
Kurth, W. S. [2 ]
Gurnett, D. A. [2 ]
Berdichevsky, D. B. [3 ,4 ]
Jian, L. K. [5 ]
Ness, N. F.
Park, J. [5 ,6 ]
Szabo, A. [5 ]
机构
[1] Leonard F Burlaga Inc, Davidsonville, MD 21035 USA
[2] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
[3] IFIR CONICET UNR, Esmeralda & 27 Febrero, Rosario, Santa Fe, Argentina
[4] DANIEL B Partnership, TRIDENT BERDICHEVSKY, Greenbelt, MD 20770 USA
[5] NASA, Heliophs Sci Div, GSFC, Greenbelt, MD 20771 USA
[6] Univ Maryland Baltimore Cty, Baltimore, MD 21250 USA
来源
ASTROPHYSICAL JOURNAL | 2021年 / 911卷 / 01期
关键词
SOLAR-WIND; HELIOSHEATH; INTERMITTENCY; HELIOPAUSE; TURBULENCE; WHETHER; SHOCKS;
D O I
10.3847/1538-4357/abeb6a
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Voyager 1 has been moving through the very local interstellar medium (VLISM) from the time that it crossed the heliopause on 2012/DOY 238 to 2020/DOY 292. Three notable objects in the magnetic field of the VLISM have been observed: two shocks and one pressure front. This paper reports the observation of a fourth object observed near 2020/DOY 147. There were no upstream electron plasma oscillations of the type often observed ahead of shocks, abrupt increases in energetic particles, or fluctuations in the 48 s increments of the magnetic field associated with this feature, suggesting that it was probably not a shock. This feature was associated with a relatively large increase in the magnetic field strength (B2/B1 = 1.35) and in the electron density determined by the Plasma Wave Science experiment (N2/N1 = 1.36) using a new method described in this paper. This feature appears to be a pressure front associated with a compressive wave in the VLISM. The two shocks and the two pressure fronts were associated with the four largest maxima observed in B(t) between 2012/DOY 238 and 2020/DOY 292. Each feature was associated with a jump-ramp structure. The jump-ramp structures were separated by long relatively undisturbed quiet intervals.
引用
收藏
页数:9
相关论文
共 25 条
  • [21] MAGNETIC FIELD STRENGTH FLUCTUATIONS IN THE HELIOSHEATH: VOYAGER 1 OBSERVATIONS DURING 2009
    Burlaga, L. F.
    Ness, N. F.
    ASTROPHYSICAL JOURNAL, 2012, 744 (01):
  • [22] Magnitude and direction of the local interstellar magnetic field inferred from Voyager 1 and 2 interstellar data and global heliospheric model
    Izmodenov, Vladislav V.
    Alexashov, Dmitry B.
    ASTRONOMY & ASTROPHYSICS, 2020, 633
  • [23] MAGNETIC FIELD FLUCTUATIONS OBSERVED IN THE HELIOSHEATH AND INTERSTELLAR MAGNETIC FIELD BY VOYAGER 1 AT 115.7-124.9 AU DURING 2011-2013
    Burlaga, L. F.
    Ness, N. F.
    Florinski, V.
    Heerikhuisen, J.
    ASTROPHYSICAL JOURNAL, 2014, 792 (02):
  • [24] Radial spatiotemporal evolution of rf magnetic field and plasma current in a very-high-frequency plasma source over a wide range of plasma density and pressure
    Zhao, Jianping
    Ventzek, Peter L. G.
    Lane, Barton
    Iwao, Toshihiko
    Ishibashi, Kiyotaka
    PHYSICAL REVIEW E, 2021, 104 (02)
  • [25] Radial spatiotemporal evolution of rf magnetic field and plasma current in a very-high-frequency plasma source over a wide range of plasma density and pressure
    Zhao, Jianping
    Ventzek, Peter L. G.
    Lane, Barton
    Iwao, Toshihiko
    Ishibashi, Kiyotaka
    Physical Review E, 2021, 104 (02):