Heliospheric pickup ions and Favored Acceleration Locations at the Termination Shock (FALTS): Are voyager observations really inconsistent?

被引:0
作者
Schwadron, NA [1 ]
McComas, DJ [1 ]
机构
[1] SW Res Inst, San Antonio, TX 78238 USA
来源
PHYSICS OF THE OUTER HELIOSPHERE | 2004年 / 719卷
关键词
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Pickup ions (PUIs) are created from a number of neutral sources both inside and outside the heiosphere. The combination of recent observational and theoretical work has completed the catalog of at least the major sources of Heliospheric PUIs. These PUIs are the seed population for anomalous cosmic rays (ACRs), which are accelerated to high energies at the termination shock (TS). Recently, Voyager 1 (V1) encountered strong intensity enhancements in the energy range where pickup ions are energized into ACRs. These observations may indicate that V1 has already passed beyond the TS into the bath of accelerated pickup ions in the inner heliosheath. However, opposing this conclusion, V1 magnetic field and higher energy particle observations appear very typical. Here, we advance the concept that V1 was in a special region in the heliosphere where the magnetic field is highly distorted due to solar wind shearing and footpoint motions at the Sun. These Favored Acceleration Locations at the Termination Shock (FALTS) efficiently inject pickup ions into diffusive shock acceleration due to slightly increased radial field components in the FALTS field regions. Such regions provide much more direct field-line connection to the TS than along strongly wound Parker field lines found outside of FALTS. Inside the TS, FALTS naturally enhance fluxes of accelerated pickup ions. Thus, FALTS may be responsible for the V1 observations of energetic particle enhancements. Further, FALTS provide a conduit for an inward electron heat flux from hot electrons beyond the TS, thereby heating the plasma and increasing the electron impact ionization rate. This additional ionization causes mass loading that locally weakens the TS and draws it in toward the Sun, Thus, FALTS can cause both energetic particle intensity enhancements and a weaker, locally drawn in TS; these effects may help explain the otherwise contradictory V1 observations.
引用
收藏
页码:81 / 86
页数:6
相关论文
共 20 条
  • [1] INTERPLANETARY STREAM INTERFACES
    BURLAGA, LF
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH, 1974, 79 (25): : 3717 - 3725
  • [2] Composition of anomalous cosmic rays and other heliospheric ions
    Cummings, AC
    Stone, EC
    Steenberg, CD
    [J]. ASTROPHYSICAL JOURNAL, 2002, 578 (01) : 194 - 210
  • [3] INTERPRETATION OF OBSERVED OXYGEN AND NITROGEN ENHANCEMENTS IN LOW-ENERGY COSMIC-RAYS
    FISK, LA
    KOZLOVSK.B
    RAMATY, R
    [J]. ASTROPHYSICAL JOURNAL, 1974, 190 (01) : L35 - L37
  • [4] Implications of the observed anticorrelation between solar wind speed and coronal electron temperature
    Gloeckler, G
    Zurbuchen, TH
    Geiss, J
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2003, 108 (A4)
  • [5] Interception of comet Hyakutake's ion tail at a distance of 500 million kilometres
    Gloeckler, G
    Geiss, J
    Schwadron, NA
    Fisk, LA
    Zurbuchen, TH
    Ipavich, FM
    von Steiger, R
    Balsiger, H
    Wilken, B
    [J]. NATURE, 2000, 404 (6778) : 576 - 578
  • [6] GLOECKLER G, 2004, IN PRESS ASTROPHYS J
  • [7] SOLAR-WIND STREAM INTERFACES
    GOSLING, JT
    ASBRIDGE, JR
    BAME, SJ
    FELDMAN, WC
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1978, 83 (NA4): : 1401 - 1412
  • [8] HUNDHAUSEN AJ, 1975, J GEOPHYS RES, V80, P1845, DOI 10.1029/JA080i013p01845
  • [9] Voyager 1 exited the solar wind at a distance of ∼85 AU from the Sun
    Krimigis, SM
    Decker, RB
    Hill, ME
    Armstrong, TP
    Gloeckler, G
    Hamilton, DC
    Lanzerotti, LJ
    Roelof, EC
    [J]. NATURE, 2003, 426 (6962) : 45 - 48
  • [10] HYDROMAGNETIC WAVE EXCITATION BY IONIZED INTERSTELLAR HYDROGEN AND HELIUM IN THE SOLAR-WIND
    LEE, MA
    IP, WH
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1987, 92 (A10): : 11041 - 11052