'Emerging flux' presentation slideshows

3D simulations of solar emerging flux

3D simulations of solar emerging flux. ISOBE Hiroaki Plasma seminar 2004/04/28. What is emerging flux?. Magnetic field: origin of solar activities such as sunspots, active regions, coronal heating, flares, coronal mass ejections, jets etc..

536 views • 41 slides

Solar-B Science Objectives - Overview of the Mission -

394 views • 39 slides

MHD simulations on eruption triggered by flux emergence

FEW2011 2011.8.22-25 Berkeley, USA. MHD simulations on eruption triggered by flux emergence. T. Yokoyama University of Tokyo Collaborators K. Nagashima (Stanford U.), S. Notoya, T. Kaneko (U. Tokyo) Based on the papers Notoya, 2006, master degree thesis, U. Tokyo

478 views • 37 slides

Solar Flares

Solar Flares. Phillip Chamberlin University of Colorado Laboratory for Atmospheric and Space Physics (LASP) Phil.Chamberlin@lasp.colorado.edu (303)492-9318. Outline. Solar Atmosphere Flux Tubes Two Ribbon Flare Cartoons Movies Irradiance Measurements of Flares VUV White Light TSI.

795 views • 31 slides

Solar Flares

Solar Flares. Phillip Chamberlin University of Colorado Laboratory for Atmospheric and Space Physics (LASP) Phil.Chamberlin@lasp.colorado.edu (303)492-9318. Outline. Solar Atmosphere Flux Tubes Two Ribbon Flare Cartoons Movies Irradiance Measurements of Flares VUV White Light TSI.

653 views • 28 slides

Evolution of Emerging Flux and Associated Active Phenomena

Evolution of Emerging Flux and Associated Active Phenomena. Takehiro Miyagoshi (GUAS , Japan) Takaaki Yokoyama (NRO , Japan). Studies of Coronal Magnetic Structure Formed by Isolated Twisted Emerging Flux by MHD Numerical Simulations. Upper Convection Zone --- Corona.

291 views • 20 slides

Evolution of Emerging Flux and Associated Active Phenomena

Evolution of Emerging Flux and Associated Active Phenomena. Takehiro Miyagoshi (GUAS , Japan) Takaaki Yokoyama (NRO , Japan). Studies of Coronal Magnetic Structure Formed by Isolated Twisted Emerging Flux by MHD Numerical Simulations. Upper Convection Zone --- Corona.

204 views • 20 slides

Sub-Surface Meridional Flow, Vorticity and the Life Time of Solar Active Regions

Sub-Surface Meridional Flow, Vorticity and the Life Time of Solar Active Regions. Maurya, R., A., & Ambastha, A. 2010, arXiv1003.5273. April 19, 2010 short talk in Solar Seminar Tetsu Anan. Abstract. 1/15. Global Oscillation Network Group (GONG)

315 views • 19 slides

Magnetic connection between the photosphere and the corona

Magnetic connection between the photosphere and the corona. S. Kamio Solar Seminar 2003.12.15. Introduction. Magnetic field must play an important role in the connection between photosphere and corona may be related to surge, macro spicule, or EUV blinker?.

264 views • 16 slides

The process of the filament formation and eruption triggered by the emerging flux

The process of the filament formation and eruption triggered by the emerging flux. S.Notoya T.Yokoyama. Plane: temperature. Arrows:direction of the magnetic field. 6*10^4 (km). corona. convection zone and chromospheres. Corona arcade field.

215 views • 10 slides