EQUILIBRIUM PITCH-ANGLE DISTRIBUTION FUNCTIONS OF ENERGETIC PARTICLES IN NONADIABATIC SCATTERING ON THE CURRENT SHEET OF THE MAGNETOSPHERIC TAIL.

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EQUILIBRIUM PITCH-ANGLE DISTRIBUTION FUNCTIONS OF ENERGETIC PARTICLES IN NONADIABATIC SCATTERING ON THE CURRENT SHEET OF THE MAGNETOSPHERIC TAIL. / Tsyganenko, N. A.

в: Cosmic Research (English translation of Kosmicheskie Issledovaniya), Том 21, № 4, 01.01.1983, стр. 453-456.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

BibTeX

@article{95555fc9c1754dbe9e1bfe5f2ced811b,

title = "EQUILIBRIUM PITCH-ANGLE DISTRIBUTION FUNCTIONS OF ENERGETIC PARTICLES IN NONADIABATIC SCATTERING ON THE CURRENT SHEET OF THE MAGNETOSPHERIC TAIL.",

abstract = "The pitch-angle scattering of energetic particles in a magnetic field containing a current sheet, analogous to that observed in the region of the magnetospheric tail, is studied by numerical methods. Calculations of a large number of trajectories (about 20,000 for each variant of the model) permitted the construction of a matrix of pitch-angle scattering and the kernel of the integral equation for the equilibrium particle distribution function. The results obtained can be used to interpret observations of the spatial distribution of fluxes of energetic particles in the near region of the magnetospheric tail and at the outer boundary of the belt of trapped radiation.",

author = "Tsyganenko, {N. A.}",

year = "1983",

month = jan,

day = "1",

language = "English",

volume = "21",

pages = "453--456",

journal = "Cosmic Research",

issn = "0010-9525",

publisher = "МАИК {"}Наука/Интерпериодика{"}",

number = "4",

}

RIS

TY - JOUR

T1 - EQUILIBRIUM PITCH-ANGLE DISTRIBUTION FUNCTIONS OF ENERGETIC PARTICLES IN NONADIABATIC SCATTERING ON THE CURRENT SHEET OF THE MAGNETOSPHERIC TAIL.

AU - Tsyganenko, N. A.

PY - 1983/1/1

Y1 - 1983/1/1

N2 - The pitch-angle scattering of energetic particles in a magnetic field containing a current sheet, analogous to that observed in the region of the magnetospheric tail, is studied by numerical methods. Calculations of a large number of trajectories (about 20,000 for each variant of the model) permitted the construction of a matrix of pitch-angle scattering and the kernel of the integral equation for the equilibrium particle distribution function. The results obtained can be used to interpret observations of the spatial distribution of fluxes of energetic particles in the near region of the magnetospheric tail and at the outer boundary of the belt of trapped radiation.

AB - The pitch-angle scattering of energetic particles in a magnetic field containing a current sheet, analogous to that observed in the region of the magnetospheric tail, is studied by numerical methods. Calculations of a large number of trajectories (about 20,000 for each variant of the model) permitted the construction of a matrix of pitch-angle scattering and the kernel of the integral equation for the equilibrium particle distribution function. The results obtained can be used to interpret observations of the spatial distribution of fluxes of energetic particles in the near region of the magnetospheric tail and at the outer boundary of the belt of trapped radiation.

UR - http://www.scopus.com/inward/record.url?scp=0020777439&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:0020777439

VL - 21

SP - 453

EP - 456

JO - Cosmic Research

JF - Cosmic Research

SN - 0010-9525

IS - 4

ER -

ID: 33903190