'Magnetic energy' presentation slideshows

E&M I

1.03k views • 37 slides

GLOBAL ENERGETICS OF FLARES

GLOBAL ENERGETICS OF FLARES. Gordon Emslie (for a large group of people). Initial Study (Emslie et al. 2004). Methodologies. Magnetic Energy U B =. Methodologies. Thermal Plasma U th = 3 n e V kT = 3 k T [EM . V] 1/2 erg

520 views • 36 slides

15.1 Energy and Its Forms

373 views • 28 slides

Casimir effect in Napoli

499 views • 27 slides

The Time Domain in Stellar Radio Astronomy

The Time Domain in Stellar Radio Astronomy. Rachel Osten STScI Radio Stars and Their Lives in the Galaxy Oct. 3, 2012. What do Studies of the Time Domain Tell Us About Stellar Astrophysics?.

466 views • 27 slides

The prompt phase of GRBs

The prompt phase of GRBs . Dimitrios Giannios Lyman Spitzer, Jr. Fellow Princeton, Department of Astrophysical Sciences Raleigh, 3/7/2011 . Structure of the talk. Main properties of the prompt emission Models for the GRB flow Fireballs Internal shocks Poynting-flux dominated flows

390 views • 24 slides

Specification of ITER disruption/VDE Thermal Loads

Update on Thermal Loads during disruptions and VDEs A. Loarte with contributions from M. Sugihara , A. Herrmann, G. Arnoux, T. Eich, G. Counsell, G. Pautasso, V. Riccardo, etc. Specification of ITER disruption/VDE Thermal Loads.

397 views • 18 slides

PIC simulations of magnetic reconnection

PIC simulations of magnetic reconnection. Cerutti et al. 2013. 3D PIC simulations of relativistic pair plasma reconnection ( Zeltron code) Includes Radiation reaction force ( Lorentz -Abraham- Dirac equation ) Guide field Results :

303 views • 16 slides

Applied Spectroscopy Guillermo Moyna

Applied Spectroscopy Guillermo Moyna. Ala-Arg-Pro-Tyr-Asn-Phe- Cpa -Leu-NH 2. Cpa. Ala. Pro. What is Spectroscopy? Without going into latin or greek, spectroscopy is the study of the interactions between light and matter .

449 views • 15 slides

Lesson 3.3:

291 views • 15 slides

Radio

Radio. Introductory Question. If you took an electrically charged ball and shook it up and down rapidly, charges in a nearby metal object would move in response. How far away could that metal object be and still respond? 1 meter 1 kilometer The other side of the universe.

254 views • 15 slides

Radio

Radio. Question:. If you took an electrically charged ball and shook it up and down rapidly, charges in a nearby metal object would move in response. How far away could that metal object be and still respond? 1 meter 1 kilometer The other side of the universe. Observations About Radio.

263 views • 14 slides

372 views • 13 slides

The Sun

322 views • 13 slides

Muscular System

217 views • 12 slides

Neutronics Parameters for Preferred Chamber Configuration with Magnetic Intervention

Neutronics Parameters for Preferred Chamber Configuration with Magnetic Intervention . Mohamed Sawan Ed Marriott, Carol Aplin UW Fusion Technology Inst. Rene Raffray UCSD. HAPL Project Meeting UW-Madison October 22-23, 2008. Blanket Configuration. Top Blanket: 5 m above target

215 views • 12 slides

Can We Harness Solar Wind As Energy?

Can We Harness Solar Wind As Energy?. By Eric Eggen, Samir El Idrissi, and Daniel Zheng. Useful Vocabulary. Sub-atomic - Smaller than an atom. Electron - Sub -atomic particle with a charge of negative energy. Atomic - Relating to an atom.

195 views • 8 slides

Magnetic Energy

Magnetic Energy. Caroline Bienkowski, Jack Felch, Veronica Manson, Kyle Elsasser. What is Magnetic Energy?.

1.47k views • 4 slides

Box Model: Core Evolution ~ 700 Myr

Geodynamo Evolution Flow Chart. Box Model: Core Evolution ~ 700 Myr. Thermodynamic Parameters. CMB Heat Flow Q(t) T(r,0), C(r,0), r ICB (0). T(r, t ) C( r,t ) r ICB (t). 3D Model: Numerical Dynamo ~ 5 Myr intervals. CMB Heat Flux Heterogeneity q( x ) W (t).

158 views • 4 slides

Madeline Hubbard (Keene High School)

Magnetic Reconnection: High Latitude Tail ward of the Cusp Events. Introduction. Madeline Hubbard (Keene High School) Matthew Shindel (Stanwich High School) Advisors: Fathima Muzamil, Dr. Charles Farrugia , Dr. Roy Torbert.

144 views • 1 slides