Validation of two MHD models of the solar corona with rotational tomography

We demonstrate a validation of two 3D MHD models of the corona by comparing density values from solar rotational tomography (SRT) to densities and morphological properties of the two MHD solutions for CR 2029 (2005 April 21-May 18). The two MHD models are given by the Stanford and Michigan models, a...

Descripción completa

Guardado en:

Detalles Bibliográficos
Autores principales:	Vasquez, A.M., Frazin, R.A., Hayashi, K., Sokolov, I.V., Cohen, O., Manchester IV, W.B., Kamalabadi, F.
Formato:	JOUR
Materias:	Methods: numerical Solar wind Sun: corona Sun: magnetic fields Techniques: image processing
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_0004637X_v682_n2_p1328_Vasquez
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

Ejemplares similares

The solar minimum corona from differential emission measure tomography
por: Vásquez, A.M., et al.

Validation of two MHD models of the solar corona with rotational tomography
Publicado: (2008)

Quantitative, three-dimensional analysis of the global corona with multi-spacecraft differential emission measure tomography
por: Frazin, R.A., et al.

The solar minimum corona from differential emission measure tomography
Publicado: (2010)

Tomography of the Solar Corona with Multiple Instruments: First Steps
por: Lloverás, D.G., et al.
Publicado: (2019)

The 3D solar corona Cycle 24 rising phase from SDO/AIA tomography
por: Nuevo, F.A., et al.

The effect of proton temperature anisotropy on the solar minimum corona and wind
por: Vásquez, A.M., et al.

The 3D solar minimum with differential emission measure tomography
por: Vásquez, A.M., et al.

Evolution of the global temperature structure of the solar corona during the minimum between solar cycles 23 and 24
por: Manchester IV, W.B., et al.
Publicado: (2013)

Evolution of the global temperature structure of the solar corona during the minimum between solar cycles 23 and 24
por: Manchester IV, W.B., et al.

Evolution of the global temperature structure of the solar corona during the minimum between solar cycles 23 and 24
por: Manchester IV, W.B., et al.
Publicado: (2013)

Reconstrucción tomográfica y modelado MHD de la baja corona para la rotación CR2223 de la campaña WHPI
por: Lloveras, D. G., et al.
Publicado: (2021)

Reconstrucción tridimensional de la velocidad del viento solar mediante tomografía Lyman-α
por: Nuevo, F.A., et al.
Publicado: (2023)

Quantitative, three-dimensional analysis of the global corona with multi-spacecraft differential emission measure tomography
Publicado: (2009)

Oxygen abundance in coronal streamers
por: Vásquez, A.M., et al.

The effect of proton temperature anisotropy on the solar minimum corona and wind
Publicado: (2003)

A global two-temperature corona and inner heliosphere model: A comprehensive validation study
por: Jin, M., et al.
Publicado: (2012)

A global two-temperature corona and inner heliosphere model: A comprehensive validation study
por: Jin, M., et al.

A global two-temperature corona and inner heliosphere model: A comprehensive validation study
por: Jin, M., et al.
Publicado: (2012)

Energy input flux in the global quiet-sun corona
por: Mac Cormack, C., et al.

Multimodal differential emission measure in the solar corona
por: Nuevo, F.A., et al.

Newly discovered global temperature structures in the quiet sun at solar minimum
por: Huang, Z., et al.

Oxygen abundance in coronal streamers
Publicado: (2005)

A global two-temperature corona and inner heliosphere model: A comprehensive validation study
por: Vasquez, Alberto Marcos
Publicado: (2012)

Nonlocal heat transport in the solar wind
por: Canullo, M.V., et al.

The 3D solar corona Cycle 24 rising phase from SDO/AIA tomography
Publicado: (2011)

The counterkink rotation of a non-hale active region
Publicado: (2000)

The counterkink rotation of a non-hale active region
por: López Fuentes, M.C., et al.

Nonlocal heat transport in the solar wind
Publicado: (1996)

Energy input flux in the global quiet-sun corona
por: Vasquez, Alberto Marcos, et al.
Publicado: (2017)

A data-driven, two-temperature solar wind model with alfvén waves
por: Van Der Holst, B., et al.
Publicado: (2010)

A data-driven, two-temperature solar wind model with alfvén waves
por: Van Der Holst, B., et al.

A data-driven, two-temperature solar wind model with alfvén waves
por: Van Der Holst, B., et al.
Publicado: (2010)

Multimodal differential emission measure in the solar corona
por: Nuevo, Federico Alberto, et al.
Publicado: (2015)

Coronal transients during two solar minima: Their source regions and interplanetary counterparts
por: Mandrini, Cristina Hemilse, et al.
Publicado: (2011)

Coronal transients during two solar minima: Their source regions and interplanetary counterparts
por: Cremades, H., et al.
Publicado: (2011)

Coronal transients during two solar minima: Their source regions and interplanetary counterparts
por: Cremades, H., et al.

Coronal transients during two solar minima: Their source regions and interplanetary counterparts
por: Cremades, H., et al.
Publicado: (2011)

Evolution of the global temperature structure of the solar corona during the minimum between solar cycles 23 and 24
por: Nuevo, Federico Alberto, et al.
Publicado: (2013)

Distribution of electric currents in sunspots from photosphere to corona
Publicado: (2014)