ACCELERATION FROM FIELD-ALIGNED POTENTIAL DROPS

被引:64
作者
HAERENDEL, G
机构
[1] Max-Planck-Inst. F. E.
关键词
ACCELERATION OF PARTICLES; MHD; PLASMAS;
D O I
10.1086/191901
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Unstable field-aligned currents are seen as the origin of field-aligned potential drops. They convert energy stored in magnetic shear stresses into kinetic energy. A good fraction of this energy is carried by runaway electrons and ions out of the acceleration region. The paper emphasizes the analogy with mechanical fractures. Simple expressions for the energy conversion rate and the parallel potential drop are derived, the two being linked by the critical current density needed for instability. The origin of the currents (generator) lies mostly in a region remote from that of energy conversion (fracture zone). The transmission of shear stresses and energy from the generator plasma, where the primary forces are applied to the fracture zone is also considered. A closed set of relations allows quantitative evaluation of the energetic particle production efficiency. The decoupling of the plasma on either side of the fracture zone which allows fast stress relief is described in detail, as well as a stationary model for the Alfven wave interaction between fracture zone and generator plasma. A simple concept of the nature of the anomalous resistivity generated by the unstable current leads to an expression for the magnetic diffusivity inside the fracture zone and an estimate of the latter's extent parallel to the magnetic field, whereas its width and length transverse to B follow from the macroscopic relations. Finally and as an example, the theory is applied to the problem of fast electron (and ion) acceleration well above 1 MeV seen to occur in many solar flares. It is obvious that this process belongs to the most powerful production processes of high-energy particles in stellar magnetic fields.
引用
收藏
页码:765 / 774
页数:10
相关论文
共 31 条
[1]  
Alfven H., 1963, COSMICAL ELECTRODYNA
[2]   AURORAL ARC THICKNESSES AS PREDICTED BY VARIOUS THEORIES [J].
BOROVSKY, JE .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1993, 98 (A4) :6101-6138
[3]   CHARACTERISTICS OF SOLITARY WAVES AND WEAK DOUBLE-LAYERS IN THE MAGNETOSPHERIC PLASMA [J].
BOSTROM, R ;
GUSTAFSSON, G ;
HOLBACK, B ;
HOLMGREN, G ;
KOSKINEN, H ;
KINTNER, P .
PHYSICAL REVIEW LETTERS, 1988, 61 (01) :82-85
[4]   ROCKET-BASED MAGNETIC OBSERVATIONS OF AURORAL BIRKELAND CURRENTS IN ASSOCIATION WITH A STRUCTURED AURORAL ARC [J].
CASSERLY, RT ;
CLOUTIER, PA .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1975, 80 (16) :2165-2168
[5]   PHENOMENOLOGICAL MODEL OF SOLAR-FLARES [J].
COLGATE, SA .
ASTROPHYSICAL JOURNAL, 1978, 221 (03) :1068-+
[6]   AURORAL ELECTROMAGNETIC DISTURBANCES AT ALTITUDES OF 900 KM - ALFVEN-WAVE TURBULENCE [J].
DUBININ, EM ;
VOLOKITIN, AS ;
ISRAELEVICH, PL ;
NIKOLAEVA, NS .
PLANETARY AND SPACE SCIENCE, 1988, 36 (10) :949-962
[7]   RELATIONSHIP BETWEEN AURORAL ELECTRONS FLUXES AND FIELD ALIGNED ELECTRIC-POTENTIAL DIFFERENCE [J].
FRIDMAN, M ;
LEMAIRE, J .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1980, 85 (NA2) :664-670
[8]   PULSAR ELECTRODYNAMICS [J].
GOLDREICH, P ;
JULIAN, WH .
ASTROPHYSICAL JOURNAL, 1969, 157 (2P1) :869-+
[9]   THE DISTRIBUTION OF ION-BEAMS AND CONICS BELOW 8000 KM [J].
GORNEY, DJ ;
CLARKE, A ;
CROLEY, D ;
FENNELL, J ;
LUHMANN, J ;
MIZERA, P .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1981, 86 (NA1) :83-89
[10]  
Gurnett D., 1972, CRITICAL PROBLEMS MA, P123