Published 2017 | Version v1
Miscellaneous Open

Usage of magnetic field of magnetosphere paraboloid model as initial approximation at hybrid numerical simulation of solar wind interaction with Mercury magnetosphere

  • 1. NIIYaF MGU, Moscow (Russian Federation)
  • 2. Space Research Inst., Austrian Acad. Sci., Graz (Austria)
  • 3. Aalto Univ., Helsinki (Finland)

Description

no abstract available

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Part of:
The Twelfth annual conference Plasma physics in Solar system. Abstracts

Additional details

Additional titles

Original title (Russian)
Использование магнитного поля параболоидной модели магнитосферы в качестве начального приближения при гибридном численном моделировании взаимодействия солнечного ветра с магнитосферой Меркурия

Publishing Information

Publisher
IKI RAN
Imprint Place
Moscow (Russian Federation)
Imprint Title
The Twelfth annual conference Plasma physics in Solar system. Abstracts
Imprint Pagination
325 p.
Journal Page Range
p. 267
Report number
INIS-RU--603

Conference

Title
12. annual conference plasma physics in solar system
Original Conference Title
Dvenadtsataya ezhegodnaya konferentsiya Fizika plazmy v Solnechnoj sisteme
Dates
6-10 Feb 2017
Place
Moscow (Russian Federation)

INIS

Country of Publication
Russian Federation
Country of Input or Organization
Russian Federation
INIS RN
49053571
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
No Abstract, Conference
Descriptors DEI
COMPUTERIZED SIMULATION; CORRELATIONS; ELECTRONS; IONS; MATHEMATICAL MODELS; MERCURY PLANET; SOLAR WIND
Descriptors DEC
CHARGED PARTICLES; ELEMENTARY PARTICLES; FERMIONS; LEPTONS; PLANETS; SIMULATION; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR WINDS

Optional Information

Notes
Imprint:Dvenadtsataya ezhegodnaya konferentsiya Fizika plazmy v Solnechnoj sisteme. Tezisy