'Van ballegooijen' presentation slideshows

Current Sheet Formation Along Magnetic Separators in 3d

Current Sheet Formation Along Magnetic Separators in 3d. Dana Longcope Montana State University. Thanks: I. Klapper, A.A. van Ballegooijen NSF-ATM. The Coronal Field. 8/11/01 9:25. 1 MK plasma (TRACE 171A). Corona : complex inter-connections between sources. B z =0. Lower boundary :

661 views • 57 slides

Current sheets formation along magnetic separators in 3d

Current sheets formation along magnetic separators in 3d. Dana Longcope Montana State University. Thanks: I Klapper, A.A. Van Ballegooijen NSF-ATM. The Coronal Field. 8/11/01 9:25. 1 MK plasma (TRACE 171A). Corona : complex inter-connections between sources. B z =0. Lower boundary :

684 views • 56 slides

Magnetic Shear in Two-ribbon Solar Flares

Magnetic Shear in Two-ribbon Solar Flares. Yingna Su 1,2 Advisors: Leon Golub 1 , Guangli Huang 2 Collaborators: A. A. Van Ballegooijen 1 , E. E. Deluca 1 , J. McCaughey 1 , K. K. Reeves 1 , and M. Gros 3 1. Harvard-Smithsonian Center for Astrophysics, USA

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378 views • 25 slides

Applications of MHD Turbulence: from SUMER to Ulysses! Steven R. Cranmer, Harvard-Smithsonian CfA

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Helicity Condensation: T he Origin of Coronal/Heliospheric Structure

Helicity Condensation: T he Origin of Coronal/Heliospheric Structure. S. K. Antiochos, C. R. DeVore , et al NASA/GSFC. Key features of the corona and wind Laminar loops Sheared filament channels Non-steady slow wind. TRACE: Title et al VAULT: Vourlidas et al

173 views • 9 slides

Validating Models of the Corona and Inner Heliosphere

Validating Models of the Corona and Inner Heliosphere. Discussion Leaders Bart Van Der Holst, Peter MacNeice. Objective.

200 views • 8 slides

M. G. Bobra 1 , A. A. van Ballegooijen 1 , E. E. DeLuca 1 , J. L. Sandell 2

Modeling Non-Potential Magnetic Fields in Solar Active Regions.

78 views • 1 slides