3-D Modelling of cosmetic-ray transport in the heliosphere: Toward solar maximum

Research output: Contribution to journalArticle

11 Citations (Scopus)

Abstract

We present preliminary results from new developments in our 3-D time-dependent numerical codes modeling the diffusive transport of galactic and anomalous cosmic rays in the heliosphere, including drift, diffusion, and adiabatic cooling and acceleration. Our existing 3-D codes are modified to achieve a better description of solar maximum conditions. More complex structures of the current sheet are considered, including multiple current sheets during periods of high solar activity. Latitudinal and recurrent time-variations are discussed. The role of the variation of the magnetic field strength is briefly addressed.

Original languageEnglish (US)
Pages (from-to)529-534
Number of pages6
JournalAdvances in Space Research
Volume27
Issue number3
DOIs
StatePublished - 2001

Fingerprint

Cosmetics
Cosmic rays
heliosphere
current sheets
rays
Magnetic fields
Cooling
solar activity
cosmic ray
modeling
cosmic rays
field strength
magnetic field
cooling
magnetic fields
code

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

3-D Modelling of cosmetic-ray transport in the heliosphere : Toward solar maximum. / Kóta, J.; Jokipii, J. Randy.

In: Advances in Space Research, Vol. 27, No. 3, 2001, p. 529-534.

Research output: Contribution to journalArticle

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