ABOUT THE 3RD INTEGRAL OF CHARGED-PARTICLE MOTION IN STRONGLY CURVED MAGNETIC-FIELDS

被引：16

作者：

BUCHNER, J

机构：

来源：

ASTRONOMISCHE NACHRICHTEN | 1986年 / 307卷 / 03期

关键词：

D O I：

10.1002/asna.2113070310

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：191 / 199

页数：9

共 15 条

[1] SATURNS MAGNETIC TAIL - STRUCTURE AND DYNAMICS [J].

BEHANNON, KW ;

CONNERNEY, JEP ;

NESS, NF .

NATURE, 1981, 292 (5825) :753-755

[2]

Birkhoff G.D., 1927, DYNAM SYST, VVolume 9

[3]

Broucke R., 1979, INSTABILITIES DYNAMI, P3

[4]

BUCHNER J, 1986, UNPUB J GEOPHYS RES

[5]

BUCHNER J, 1982, HHI MSP182 INT REP

[6]

GALEEV AA, 1978, J EKSPER TEORET FIZI, V70, P3133

[7] PARTICLE PITCH ANGLE DIFFUSION DUE TO NON-ADIABATIC EFFECTS IN THE PLASMA SHEET [J].

GRAY, PC ;

LEE, LC .

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1982, 87 (NA9) :7445-7452

[8] ON A PLASMA SHEATH SEPARATING REGIONS OF OPPOSITELY DIRECTED MAGNETIC FIELD [J].

HARRIS, EG .

NUOVO CIMENTO, 1962, 23 (01) :115-+

[9] APPLICABILITY OF 3 INTEGRAL OF MOTION - SOME NUMERICAL EXPERIMENTS [J].

HENON, M ;

HEILES, C .

ASTRONOMICAL JOURNAL, 1964, 69 (01) :73-&

[10] EMERGING FLUX MODEL FOR SOLAR-FLARE PHENOMENON [J].

HEYVAERTS, J ;

PRIEST, ER ;

RUST, DM .

ASTROPHYSICAL JOURNAL, 1977, 216 (01) :123-137

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