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Uses and limitations of the Tsyganenko magnetic field models. / Stern, David P.; Tsyganenko, Nikolai A.

In: Eos, Transactions American Geophysical Union, Vol. 73, No. 46, 01.01.1992, p. 489-494.

Research output: Contribution to journalArticlepeer-review

Harvard

Stern, DP & Tsyganenko, NA 1992, 'Uses and limitations of the Tsyganenko magnetic field models', Eos, Transactions American Geophysical Union, vol. 73, no. 46, pp. 489-494. https://doi.org/10.1029/91EO00359

APA

Stern, D. P., & Tsyganenko, N. A. (1992). Uses and limitations of the Tsyganenko magnetic field models. Eos, Transactions American Geophysical Union, 73(46), 489-494. https://doi.org/10.1029/91EO00359

Vancouver

Stern DP, Tsyganenko NA. Uses and limitations of the Tsyganenko magnetic field models. Eos, Transactions American Geophysical Union. 1992 Jan 1;73(46):489-494. https://doi.org/10.1029/91EO00359

Author

Stern, David P. ; Tsyganenko, Nikolai A. / Uses and limitations of the Tsyganenko magnetic field models. In: Eos, Transactions American Geophysical Union. 1992 ; Vol. 73, No. 46. pp. 489-494.

BibTeX

@article{78cebcd8683b4803836ae9dab8f83baa,
title = "Uses and limitations of the Tsyganenko magnetic field models",
abstract = "When exploring a new country, one needs a good map. The Earth's magnetosphere is such a country, and its “maps” are models of the geomagnetic field. In essence they are mathematical prescriptions implemented by computer which, given (x,y,z) of a point and other supporting information, return the point's expected magnetic components (Bx, By, Bz) [Tsyganenko, 1990]. At present, the empirical magnetic field models by Tsyganenko [1987, 1989a, c; denoted henceforth as T87 and T89] are often used in various studies of the Earth's magnetosphere. Stern [1990] has devised modifications of T87 with current‐free tail lobes and with a plasma sheet that warps in response to dipole tilt [Peredo and Stern, 1991].",
keywords = "magnetosphere, models, SPACECRAFT DATA",
author = "Stern, {David P.} and Tsyganenko, {Nikolai A.}",
year = "1992",
month = jan,
day = "1",
doi = "10.1029/91EO00359",
language = "English",
volume = "73",
pages = "489--494",
journal = "Trans Amer Geophys Union",
issn = "0096-3941",
publisher = "American Geophysical Union",
number = "46",

}

RIS

TY - JOUR

T1 - Uses and limitations of the Tsyganenko magnetic field models

AU - Stern, David P.

AU - Tsyganenko, Nikolai A.

PY - 1992/1/1

Y1 - 1992/1/1

N2 - When exploring a new country, one needs a good map. The Earth's magnetosphere is such a country, and its “maps” are models of the geomagnetic field. In essence they are mathematical prescriptions implemented by computer which, given (x,y,z) of a point and other supporting information, return the point's expected magnetic components (Bx, By, Bz) [Tsyganenko, 1990]. At present, the empirical magnetic field models by Tsyganenko [1987, 1989a, c; denoted henceforth as T87 and T89] are often used in various studies of the Earth's magnetosphere. Stern [1990] has devised modifications of T87 with current‐free tail lobes and with a plasma sheet that warps in response to dipole tilt [Peredo and Stern, 1991].

AB - When exploring a new country, one needs a good map. The Earth's magnetosphere is such a country, and its “maps” are models of the geomagnetic field. In essence they are mathematical prescriptions implemented by computer which, given (x,y,z) of a point and other supporting information, return the point's expected magnetic components (Bx, By, Bz) [Tsyganenko, 1990]. At present, the empirical magnetic field models by Tsyganenko [1987, 1989a, c; denoted henceforth as T87 and T89] are often used in various studies of the Earth's magnetosphere. Stern [1990] has devised modifications of T87 with current‐free tail lobes and with a plasma sheet that warps in response to dipole tilt [Peredo and Stern, 1991].

KW - magnetosphere

KW - models

KW - SPACECRAFT DATA

UR - http://www.scopus.com/inward/record.url?scp=84984503235&partnerID=8YFLogxK

U2 - 10.1029/91EO00359

DO - 10.1029/91EO00359

M3 - Article

AN - SCOPUS:84984503235

VL - 73

SP - 489

EP - 494

JO - Trans Amer Geophys Union

JF - Trans Amer Geophys Union

SN - 0096-3941

IS - 46

ER -

ID: 33902934