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Dressing the Coronal Magnetic Extrapolations of Active Regions with a Parameterized Thermal Structure. / Nita, Gelu M.; Viall, Nicholeen M.; Klimchuk, James A.; Loukitcheva, Maria A.; Gary, Dale E.; Kuznetsov, Alexey A.; Fleishman, Gregory D.

в: Astrophysical Journal, Том 853, № 1, 66, 20.01.2018.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Nita, GM, Viall, NM, Klimchuk, JA, Loukitcheva, MA, Gary, DE, Kuznetsov, AA & Fleishman, GD 2018, 'Dressing the Coronal Magnetic Extrapolations of Active Regions with a Parameterized Thermal Structure', Astrophysical Journal, Том. 853, № 1, 66. https://doi.org/10.3847/1538-4357/aaa4bf

APA

Nita, G. M., Viall, N. M., Klimchuk, J. A., Loukitcheva, M. A., Gary, D. E., Kuznetsov, A. A., & Fleishman, G. D. (2018). Dressing the Coronal Magnetic Extrapolations of Active Regions with a Parameterized Thermal Structure. Astrophysical Journal, 853(1), [66]. https://doi.org/10.3847/1538-4357/aaa4bf

Vancouver

Nita GM, Viall NM, Klimchuk JA, Loukitcheva MA, Gary DE, Kuznetsov AA и пр. Dressing the Coronal Magnetic Extrapolations of Active Regions with a Parameterized Thermal Structure. Astrophysical Journal. 2018 Янв. 20;853(1). 66. https://doi.org/10.3847/1538-4357/aaa4bf

Author

Nita, Gelu M. ; Viall, Nicholeen M. ; Klimchuk, James A. ; Loukitcheva, Maria A. ; Gary, Dale E. ; Kuznetsov, Alexey A. ; Fleishman, Gregory D. / Dressing the Coronal Magnetic Extrapolations of Active Regions with a Parameterized Thermal Structure. в: Astrophysical Journal. 2018 ; Том 853, № 1.

BibTeX

@article{589d871abb284db2990096bac998f49f,
title = "Dressing the Coronal Magnetic Extrapolations of Active Regions with a Parameterized Thermal Structure",
abstract = "The study of time-dependent solar active region (AR) morphology and its relation to eruptive events requires analysis of imaging data obtained in multiple wavelength domains with differing spatial and time resolution, ideally in combination with 3D physical models. To facilitate this goal, we have undertaken a major enhancement of our IDL-based simulation tool, GX-Simulator, previously developed for modeling microwave and X-ray emission from flaring loops, to allow it to simulate quiescent emission from solar ARs. The framework includes new tools for building the atmospheric model and enhanced routines for calculating emission that include new wavelengths. In this paper, we use our upgraded tool to model and analyze an AR and compare the synthetic emission maps with observations. We conclude that the modeled magneto-thermal structure is a reasonably good approximation of the real one.",
keywords = "acceleration of particles, diffusion, Sun: flares, Sun: magnetic fields, Sun: radio radiation, turbulence",
author = "Nita, {Gelu M.} and Viall, {Nicholeen M.} and Klimchuk, {James A.} and Loukitcheva, {Maria A.} and Gary, {Dale E.} and Kuznetsov, {Alexey A.} and Fleishman, {Gregory D.}",
year = "2018",
month = jan,
day = "20",
doi = "10.3847/1538-4357/aaa4bf",
language = "English",
volume = "853",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "IOP Publishing Ltd.",
number = "1",

}

RIS

TY - JOUR

T1 - Dressing the Coronal Magnetic Extrapolations of Active Regions with a Parameterized Thermal Structure

AU - Nita, Gelu M.

AU - Viall, Nicholeen M.

AU - Klimchuk, James A.

AU - Loukitcheva, Maria A.

AU - Gary, Dale E.

AU - Kuznetsov, Alexey A.

AU - Fleishman, Gregory D.

PY - 2018/1/20

Y1 - 2018/1/20

N2 - The study of time-dependent solar active region (AR) morphology and its relation to eruptive events requires analysis of imaging data obtained in multiple wavelength domains with differing spatial and time resolution, ideally in combination with 3D physical models. To facilitate this goal, we have undertaken a major enhancement of our IDL-based simulation tool, GX-Simulator, previously developed for modeling microwave and X-ray emission from flaring loops, to allow it to simulate quiescent emission from solar ARs. The framework includes new tools for building the atmospheric model and enhanced routines for calculating emission that include new wavelengths. In this paper, we use our upgraded tool to model and analyze an AR and compare the synthetic emission maps with observations. We conclude that the modeled magneto-thermal structure is a reasonably good approximation of the real one.

AB - The study of time-dependent solar active region (AR) morphology and its relation to eruptive events requires analysis of imaging data obtained in multiple wavelength domains with differing spatial and time resolution, ideally in combination with 3D physical models. To facilitate this goal, we have undertaken a major enhancement of our IDL-based simulation tool, GX-Simulator, previously developed for modeling microwave and X-ray emission from flaring loops, to allow it to simulate quiescent emission from solar ARs. The framework includes new tools for building the atmospheric model and enhanced routines for calculating emission that include new wavelengths. In this paper, we use our upgraded tool to model and analyze an AR and compare the synthetic emission maps with observations. We conclude that the modeled magneto-thermal structure is a reasonably good approximation of the real one.

KW - acceleration of particles

KW - diffusion

KW - Sun: flares

KW - Sun: magnetic fields

KW - Sun: radio radiation

KW - turbulence

UR - http://www.scopus.com/inward/record.url?scp=85041140268&partnerID=8YFLogxK

U2 - 10.3847/1538-4357/aaa4bf

DO - 10.3847/1538-4357/aaa4bf

M3 - Article

AN - SCOPUS:85041140268

VL - 853

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 1

M1 - 66

ER -

ID: 41428626