Application of an analytical MHD wind model with latitudinal dependences to the solar wind

JJG Lima; C Sauty; N Iro; K Tsinganos; Eric Ronald Priest

Application of an analytical MHD wind model with latitudinal dependences to the solar wind

JJG Lima, C Sauty, N Iro, K Tsinganos, Eric Ronald Priest

Applied Mathematics

Research output: Other contribution

Abstract

The non-spherical character of the solar wind is modelled using an analytical MHD wind model in which the latitudinal dependences were obtained via separation of the variables (Lima, Priest & Tsinganos 2001). Ulysses data is used to constrain the parameters that control the various latitudinal profiles. The solution is then reconstructed all the way back to the base of the corona. The applicability of this model with open field lines is compared to the applicability of another model which relaxes that assumption (Sauty, Tsinganos & Trussoni 1999).

Original language	English
Publication status	Published - 2001

Keywords

solar wind
magnetohydrodynamics
NONPOLYTROPIC ASTROPHYSICAL OUTFLOWS
JETS

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title = "Application of an analytical MHD wind model with latitudinal dependences to the solar wind",

abstract = "The non-spherical character of the solar wind is modelled using an analytical MHD wind model in which the latitudinal dependences were obtained via separation of the variables (Lima, Priest & Tsinganos 2001). Ulysses data is used to constrain the parameters that control the various latitudinal profiles. The solution is then reconstructed all the way back to the base of the corona. The applicability of this model with open field lines is compared to the applicability of another model which relaxes that assumption (Sauty, Tsinganos & Trussoni 1999).",

keywords = "solar wind, magnetohydrodynamics, NONPOLYTROPIC ASTROPHYSICAL OUTFLOWS, JETS",

author = "JJG Lima and C Sauty and N Iro and K Tsinganos and Priest, {Eric Ronald}",

note = "Solar Encounter: the First Solar Orbiter Workshop, ESA SP-493",

year = "2001",

language = "English",

type = "Other",

}

TY - GEN

T1 - Application of an analytical MHD wind model with latitudinal dependences to the solar wind

AU - Lima, JJG

AU - Sauty, C

AU - Iro, N

AU - Tsinganos, K

AU - Priest, Eric Ronald

N1 - Solar Encounter: the First Solar Orbiter Workshop, ESA SP-493

PY - 2001

Y1 - 2001

N2 - The non-spherical character of the solar wind is modelled using an analytical MHD wind model in which the latitudinal dependences were obtained via separation of the variables (Lima, Priest & Tsinganos 2001). Ulysses data is used to constrain the parameters that control the various latitudinal profiles. The solution is then reconstructed all the way back to the base of the corona. The applicability of this model with open field lines is compared to the applicability of another model which relaxes that assumption (Sauty, Tsinganos & Trussoni 1999).

AB - The non-spherical character of the solar wind is modelled using an analytical MHD wind model in which the latitudinal dependences were obtained via separation of the variables (Lima, Priest & Tsinganos 2001). Ulysses data is used to constrain the parameters that control the various latitudinal profiles. The solution is then reconstructed all the way back to the base of the corona. The applicability of this model with open field lines is compared to the applicability of another model which relaxes that assumption (Sauty, Tsinganos & Trussoni 1999).

KW - solar wind

KW - magnetohydrodynamics

KW - NONPOLYTROPIC ASTROPHYSICAL OUTFLOWS

KW - JETS

M3 - Other contribution

ER -

Application of an analytical MHD wind model with latitudinal dependences to the solar wind

Abstract

Keywords

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