Standard

NUMERICAL-MODELS OF QUIET AND DISTURBED GEOMAGNETIC-FIELD IN THE CISLUNAR PART OF THE MAGNETOSPHERE. / TSYGANENKO, NA.

In: Annales de geophysique, Vol. 37, No. 3, 1981, p. 381-391.

Research output: Contribution to journal › Article › peer-review

Harvard

TSYGANENKO, NA 1981, 'NUMERICAL-MODELS OF QUIET AND DISTURBED GEOMAGNETIC-FIELD IN THE CISLUNAR PART OF THE MAGNETOSPHERE', Annales de geophysique, vol. 37, no. 3, pp. 381-391.

APA

TSYGANENKO, NA. (1981). NUMERICAL-MODELS OF QUIET AND DISTURBED GEOMAGNETIC-FIELD IN THE CISLUNAR PART OF THE MAGNETOSPHERE. Annales de geophysique, 37(3), 381-391.

Vancouver

TSYGANENKO NA. NUMERICAL-MODELS OF QUIET AND DISTURBED GEOMAGNETIC-FIELD IN THE CISLUNAR PART OF THE MAGNETOSPHERE. Annales de geophysique. 1981;37(3):381-391.

Author

TSYGANENKO, NA. / NUMERICAL-MODELS OF QUIET AND DISTURBED GEOMAGNETIC-FIELD IN THE CISLUNAR PART OF THE MAGNETOSPHERE. In: Annales de geophysique. 1981 ; Vol. 37, No. 3. pp. 381-391.

BibTeX

@article{0e1a3579099a4a8ca5570fb1c132f470,
title = "NUMERICAL-MODELS OF QUIET AND DISTURBED GEOMAGNETIC-FIELD IN THE CISLUNAR PART OF THE MAGNETOSPHERE",
abstract = "Quantitative models of the geomagnetic field are described, based on a modified and generalized version of a previously discussed model (Tsyganenko, 1976). The models provide a numerical representation of the magnetospheric magnetic field from the ionospheric level up to 60 earth radii, using the geodipole tilt angle as an input parameter. Six sets of coefficients are calculated, which correspond to different magnetospheric conditions ranging from a super-quiet state to a strong storm situation. The model is developed in the form of a FORTRAN-IV subroutine, which can be used to compute the geomagnetic field components in the solar magnetospheric coordinate system for any geodipole tilt angle.",
keywords = "magnetosphere, geomagnetic field, modeling, magnetosphere, geomagnetic field, modeling",
author = "NA TSYGANENKO",
year = "1981",
language = "English",
volume = "37",
pages = "381--391",
journal = "Annales de geophysique",
issn = "0003-4029",
publisher = "Centre Nationale de la Recherche Scientifique",
number = "3",

}

RIS

TY - JOUR

T1 - NUMERICAL-MODELS OF QUIET AND DISTURBED GEOMAGNETIC-FIELD IN THE CISLUNAR PART OF THE MAGNETOSPHERE

AU - TSYGANENKO, NA

PY - 1981

Y1 - 1981

N2 - Quantitative models of the geomagnetic field are described, based on a modified and generalized version of a previously discussed model (Tsyganenko, 1976). The models provide a numerical representation of the magnetospheric magnetic field from the ionospheric level up to 60 earth radii, using the geodipole tilt angle as an input parameter. Six sets of coefficients are calculated, which correspond to different magnetospheric conditions ranging from a super-quiet state to a strong storm situation. The model is developed in the form of a FORTRAN-IV subroutine, which can be used to compute the geomagnetic field components in the solar magnetospheric coordinate system for any geodipole tilt angle.

AB - Quantitative models of the geomagnetic field are described, based on a modified and generalized version of a previously discussed model (Tsyganenko, 1976). The models provide a numerical representation of the magnetospheric magnetic field from the ionospheric level up to 60 earth radii, using the geodipole tilt angle as an input parameter. Six sets of coefficients are calculated, which correspond to different magnetospheric conditions ranging from a super-quiet state to a strong storm situation. The model is developed in the form of a FORTRAN-IV subroutine, which can be used to compute the geomagnetic field components in the solar magnetospheric coordinate system for any geodipole tilt angle.

KW - magnetosphere

KW - geomagnetic field

KW - modeling

KW - magnetosphere

KW - geomagnetic field

KW - modeling

M3 - Article

VL - 37

SP - 381

EP - 391

JO - Annales de geophysique

JF - Annales de geophysique

SN - 0003-4029

IS - 3

ER -

ID: 27874374