Dynamic magnetography of solar flaring loops

Gregory Fleishman; Gelu Nita; Dale Gary

doi:10.1088/0004-637X/698/2/L183

Dynamic magnetography of solar flaring loops

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

Abstract

We develop a practical forward fitting method based on the SIMPLEX algorithm with shaking, which allows the derivation of the magnetic field and other parameters along a solar flaring loop using microwave imaging spectroscopy of gyrosynchrotron emission. We illustrate the method using a model loop with spatially varying magnetic field, filled with uniform ambient density and an evenly distributed fast electron population with an isotropic, power-law energy distribution.

Original language	English (US)
Pages (from-to)	L183-L187
Journal	Astrophysical Journal
Volume	698
Issue number	2
DOIs	https://doi.org/10.1088/0004-637X/698/2/L183
State	Published - Jun 20 2009

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

Sun: corona
Sun: flares
Sun: magnetic fields
Sun: radio radiation

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10.1088/0004-637X/698/2/L183

Cite this

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title = "Dynamic magnetography of solar flaring loops",

abstract = "We develop a practical forward fitting method based on the SIMPLEX algorithm with shaking, which allows the derivation of the magnetic field and other parameters along a solar flaring loop using microwave imaging spectroscopy of gyrosynchrotron emission. We illustrate the method using a model loop with spatially varying magnetic field, filled with uniform ambient density and an evenly distributed fast electron population with an isotropic, power-law energy distribution.",

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T1 - Dynamic magnetography of solar flaring loops

AU - Fleishman, Gregory

AU - Nita, Gelu

AU - Gary, Dale

PY - 2009/6/20

Y1 - 2009/6/20

N2 - We develop a practical forward fitting method based on the SIMPLEX algorithm with shaking, which allows the derivation of the magnetic field and other parameters along a solar flaring loop using microwave imaging spectroscopy of gyrosynchrotron emission. We illustrate the method using a model loop with spatially varying magnetic field, filled with uniform ambient density and an evenly distributed fast electron population with an isotropic, power-law energy distribution.

AB - We develop a practical forward fitting method based on the SIMPLEX algorithm with shaking, which allows the derivation of the magnetic field and other parameters along a solar flaring loop using microwave imaging spectroscopy of gyrosynchrotron emission. We illustrate the method using a model loop with spatially varying magnetic field, filled with uniform ambient density and an evenly distributed fast electron population with an isotropic, power-law energy distribution.

KW - Sun: corona

KW - Sun: flares

KW - Sun: magnetic fields

KW - Sun: radio radiation

UR - https://www.scopus.com/pages/publications/78149265491

UR - https://www.scopus.com/pages/publications/78149265491#tab=citedBy

U2 - 10.1088/0004-637X/698/2/L183

DO - 10.1088/0004-637X/698/2/L183

M3 - Article

AN - SCOPUS:78149265491

SN - 0004-637X

VL - 698

SP - L183-L187

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

ER -

Dynamic magnetography of solar flaring loops

Abstract

All Science Journal Classification (ASJC) codes

Keywords

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