'Reconnection' presentation slideshows

Anti-parallel versus Component Reconnection at the Magnetopause

Anti-parallel versus Component Reconnection at the Magnetopause. K.J. Trattner Lockheed Martin Advanced Technology Center Palo Alto, CA, USA and the Polar/TIMAS, Cluster/CIS, Image/FUV teams. Outline. Reconnection: When, Where and Why Where: The Cusp for Northward IMF

567 views • 49 slides

Three-dimensional MHD simulations of emerging flux and associated magnetic reconnection

Three-dimensional MHD simulations of emerging flux and associated magnetic reconnection. Hiroaki Isobe (DAMTP, Cambridge / Tokyo) Takehiro Miyagoshi, Kazunari Shibata (Kyoto) Takaaki Yokoyama (Tokyo). 6th Solar-B Science Meeting, 8-11 November 2005, Kyoto. Outline.

550 views • 41 slides

Reconnection Exhausts Observed by Wind in March 2006

Reconnection Exhausts Observed by Wind in March 2006. Reconnection Exhausts Observed by Wind in March 2006. V. 1-hr avgs. B. . . Oppositely Directed Exhausts From a Common Reconnection X-Line. Similar signatures observed at ACE, Geotail and STEREO B.

430 views • 34 slides

Main Title

Main Title. Reconnection mini-workshop 2002.7.9. Kwasan obs. Magnetic Reconnection in Flares Yokoyama, T. (NAOJ). Introduction : Reconnection Model of a Flare Direct Observation of a Reconnection Inflow MHD Simulation of a Flare. Reconnection Model of a Flare & Yohkoh Observations.

513 views • 31 slides

EVALUATING CONTINUOUS AND PULSED RECONNECTION FROM CUSP OBSERVATIONS

EVALUATING CONTINUOUS AND PULSED RECONNECTION FROM CUSP OBSERVATIONS. K.J. Trattner, S.M. Petrinec and S.A. Fuselier Lockheed Martin ATC, Palo Alto, CA, USA. Outline. Evidence for Continuous Reconnection Evidence for Pulsed/Intermittent Reconnection Calculating the Time since Reconnection

466 views • 29 slides

Magnetic reconnection in stars: fast and slow

Magnetic reconnection in stars: fast and slow. D. J. Mullan University of Delaware, Newark DE USA. Flares in stars. Flare: a transient increase in brightness In the Sun, flares occur in magnetic regions. Flare stars are known to have strong surface fields.

414 views • 29 slides

FNMI Student Success Webinar Series: Session 1

419 views • 27 slides

Summary of Major Scientific Advancements since 2006 Roadmap

We are gathering the major scientific advances in heliophysics that have occurred since the last roadmap ... IBEX will have a strong energetic particle population to detect ...

580 views • 25 slides

S. Tanuma (Kwasan Observatory)

365 views • 24 slides

The Magnetospheric Multiscale Mission Jim Burch Southwest Research Institute San Antonio, TX

The Magnetospheric Multiscale Mission Jim Burch Southwest Research Institute San Antonio, TX 2008 Huntsville Workshop: The Physical Processes for Energy and Plasma Transport Across Magnetic Boundaries October 27, 2008. Universal Significance of Reconnection.

395 views • 24 slides

Magnetic Reconnection in the Solar Wind Gosling, Phan, et al.

Magnetic Reconnection in the Solar Wind Gosling, Phan, et al. Draping of the Ambient Field about an ICME. The ambient magnetic field ahead of a fast ICME is compressed by its interaction with an ICME and drapes about it. Magnetic Reconnection. Inflow. Outflow. Outflow. Inflow.

334 views • 23 slides

HOW TO CREATE A CORONA

HOW TO CREATE A CORONA. need to heat the coronal plasma to several million degrees... and then prevent this plasma from escaping i.e. need closed magnetic loops solar corona requires a heat input of 10 7 ergs cm -2 s -1 (=10 4 Wm -1 ) to maintain its X-ray surface brightness

304 views • 18 slides

Hantao Ji Princeton Plasma Physics Laboratory

Hantao Ji Princeton Plasma Physics Laboratory. Experimentalist Laboratory astrophysics Reconnection, angular momentum transport, dynamo effect… Center for Magnetic Self-organization (CMSO, a NSF Physics Frontier Center) Current main research projects (>~10%)

412 views • 16 slides

Current Sheet Formation and Reconnection in CMEs/Flares

Current Sheet Formation and Reconnection in CMEs/Flares. Current Sheet Formation and Reconnection in CMEs/Flares. S. K. Antiochos, J. T. Karpen (GSFC), C. R. DeVore (NRL), (from Karpen et al 2011). Understand CME onset, acceleration, flare impulsive phase

255 views • 16 slides

264 views • 15 slides

SOLAR FLARES

425 views • 14 slides

A Comparison of 2D PIC simulations of Reconnection

Michael Harrison Thomas Neukirch Michael Hesse 5 th Cambridge Workshop on Magnetic Reconnection Bad Honnef August 17-22, 2008. A Comparison of 2D PIC simulations of Reconnection. Motivation.

486 views • 12 slides

High Latitude Magnetopause Current Sheet

High Latitude Magnetopause Current Sheet. Hui Zhang , Q.- G. Zong, T. A. Fritz (BU) S. Y. Fu (PKU) M. G. G. T. Taylor (ESA) S. Schaefer, K. H. Glassmeier (TUBraunschweig) P. W. Daly (MPA) H. Reme (CESR, France) A. Balogh (Imperial College, UK). Background.

207 views • 11 slides

Housing Justice Conference Night Shelters: Now is the Time

Housing Justice Conference Night Shelters: Now is the Time. The Local Authority/Sub Regional Perspective Margaret Williams East London Housing Partnership. East London Housing Partnership. Barking and Dagenham City of London Hackney Havering Newham Redbridge Tower hamlets

200 views • 8 slides

AOGS 2009 - Singapore

204 views • 8 slides