The top documents tagged [coronal magnetic field]

Nonlinear Force-Free Field Modeling AIA/HMI Science Team Meeting Session C2 14 February 2006 Marc DeRosa on behalf of the “NLFFF Consortium” (Karel Schrijver,
Documents Nonlinear Force-Free Field Modeling AIA/HMI Science Team Meeting Session C2 14 February 2006 Marc DeRosa on behalf of the “NLFFF Consortium” (Karel Schrijver,

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Modeling the Dynamic Evolution of the Solar Atmosphere: C4: HMI-AIA Team Meeting: 2-14-06 Bill Abbett SSL, UC Berkeley
Documents Modeling the Dynamic Evolution of the Solar Atmosphere: C4: HMI-AIA Team Meeting: 2-14-06 Bill Abbett SSL, UC Berkeley

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Investigation Overview, Scherrer, Page 1SDO Science Writers Workshop – 16 Dec 2009 HMI Investigation Overview Philip Scherrer HMI Principal Investigator
Documents Investigation Overview, Scherrer, Page 1SDO Science Writers Workshop – 16 Dec 2009 HMI Investigation Overview Philip Scherrer HMI Principal Investigator

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How Does Free Magnetic Energy Enter the Corona? Brian Welsch, Space Sciences Lab, UC Berkeley Free magnetic energy, equivalent to departures of the coronal
Documents How Does Free Magnetic Energy Enter the Corona? Brian Welsch, Space Sciences Lab, UC Berkeley Free magnetic energy, equivalent to departures of the coronal

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Coronal expansion and solar wind The large solar corona Coronal and interplanetary temperatures Coronal expansion and solar wind The heliosphere Origin
Documents Coronal expansion and solar wind The large solar corona Coronal and interplanetary temperatures Coronal expansion and solar wind The heliosphere Origin

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Coronal Heating of an Active Region Observed by XRT on May 5, 2010 A Look at Quasi-static vs Alfven Wave Heating of Coronal Loops Amanda Persichetti Aad
Documents Coronal Heating of an Active Region Observed by XRT on May 5, 2010 A Look at Quasi-static vs Alfven Wave Heating of Coronal Loops Amanda Persichetti Aad

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The Sun as a Particle Accelerator S.A. Matthews 1, D.R. Williams 1, L.M. Green 1, L. Fletcher 2, E. Kontar 2, I. Hannah 2, A.L. MacKinnon 2, V. Nakariakov
Documents The Sun as a Particle Accelerator S.A. Matthews 1, D.R. Williams 1, L.M. Green 1, L. Fletcher 2, E. Kontar 2, I. Hannah 2, A.L. MacKinnon 2, V. Nakariakov

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How Does Free Magnetic Energy Enter the Corona?
Documents How Does Free Magnetic Energy Enter the Corona?

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MSU
Documents MSU

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PPARC/Mallorca September 2006 1 Solar Flares Lyndsay Fletcher University of Glasgow Introduction Part 1: Observations energy build-up impulsive phase atmospheric
Documents PPARC/Mallorca September 2006 1 Solar Flares Lyndsay Fletcher University of Glasgow Introduction Part 1: Observations energy build-up impulsive phase atmospheric

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Simultaneous VLA and UVCS/SOHO Observations of the Solar Corona Steven R. Spangler (University of Iowa), Mari Paz Miralles, Steven R. Cranmer, and John
Documents Simultaneous VLA and UVCS/SOHO Observations of the Solar Corona Steven R. Spangler (University of Iowa), Mari Paz Miralles, Steven R. Cranmer, and John

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I. INTRODUCTION Gas Pressure Magnetic Tension Coronal loops are thin and bright structure of hot plasma emitting intense radiation in X-ray and EUV. (1)
Documents I. INTRODUCTION Gas Pressure Magnetic Tension Coronal loops are thin and bright structure of hot plasma emitting intense radiation in X-ray and EUV. (1)

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