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Physics News in 2007 - Physik Uni
Physics News in 2007 - Physik Uni

IOSR Journal of Mathematics (IOSR-JM)
IOSR Journal of Mathematics (IOSR-JM)

... of Laplace transform. More to this, Ram et al (1984) have analyzed Hall effects on heat and mass transfer flow through porous media. Soundelgekar and Abdulla Ali (1986) studied the flow of viscous incompressible electrically conducting fluid past an impulsively started infinite vertical isothermal p ...
RES7_phys_glossary
RES7_phys_glossary

Protoplanetary Disk Gap Behavior as a Function
Protoplanetary Disk Gap Behavior as a Function

Fluid Instabilities
Fluid Instabilities

6. Solar wind acceleration
6. Solar wind acceleration

... Color contours show the velocity-space density, normalized in each panel to the maximum value at the origin. At left is the initial, isotropic distribution. Adjacent panels show the time development for three later times, where τ is proportional to the normalized wave intensity. ...
causes of solar activity - The National Academies of Sciences
causes of solar activity - The National Academies of Sciences

study of planetary magnetic fields
study of planetary magnetic fields

... of 24 hours generates enough movement of the liquid to stimulate a magnetic field. The other planets in our solar system, except for Venus and Mars, all have magnetic fields or traces of magnetism that differ from Earth’s in various ways. Mars: Mars does not have a conventional magnetic field--one t ...
PPT - JMMC
PPT - JMMC

M.Sc._Physics_sem_IV.pdf
M.Sc._Physics_sem_IV.pdf

... Radiations by moving charges: LienardWeinchert potentials and field for a point charge, total power radiated by an accelerated charge (Larmor’s Formula and its relativistic generalization). Angular distribution and frequency spectrum of the radiation power.Covariant formulation of electromagnetic th ...
Fusion Reactors – a dream that can never come true
Fusion Reactors – a dream that can never come true

Magnetic fields generated by r-modes in accreting quark stars
Magnetic fields generated by r-modes in accreting quark stars

Magnetar-driven Hypernovae
Magnetar-driven Hypernovae

Vladimir_Sokolov
Vladimir_Sokolov

The magnetic hyperpolarizability anisotropy of the neon atom
The magnetic hyperpolarizability anisotropy of the neon atom

Solar-cycle variation of low density solar wind during
Solar-cycle variation of low density solar wind during

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PDF only

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Electron Firehose instability and acceleration of electrons in solar

Slide 1
Slide 1

GROUP V: Summary talk
GROUP V: Summary talk

THE MEAN ELECTROMOTIVE FORCE FOR MHD TURBULENCE
THE MEAN ELECTROMOTIVE FORCE FOR MHD TURBULENCE

... 1979; Krause and Rädler, 1980; Zeldovich et al., 1983). The crucial point of this approach is the mean electromotive force which is determined by the fluctuations of the fluid velocity and the magnetic field. It describes several physical effects like -effect, turbulent diffusion of the magnetic f ...
Lecture 4: Molecular Clouds (1)
Lecture 4: Molecular Clouds (1)

... Both HI and diffuse clouds can persist for long periods by means of pressure balance, because of the presence of a surrounding, more rarefied and warmer medium which prevents the internal (thermal) motion from dispersing the cloud. In giant molecular clouds, the main cohesive force is typically the ...
Syllabus for a Post Graduate Course in Physics(M.Sc) 1 Introduction
Syllabus for a Post Graduate Course in Physics(M.Sc) 1 Introduction

MHD seismology as a tool to diagnose the coronae of X
MHD seismology as a tool to diagnose the coronae of X

pptx
pptx

... Hydrogen fusion reactions ...
< 1 ... 14 15 16 17 18 19 20 21 22 ... 39 >

Spheromak

Not to be confused with the spherical tokamak, another topic in fusion research.A spheromak is an arrangement of plasma formed into a toroidal shape similar to a smoke ring. The spheromak contains large internal electric currents and their associated magnetic fields arranged so the magnetohydrodynamic forces within the spheromak are nearly balanced, resulting in long-lived (microsecond) confinement times without external fields. Spheromaks belong to a type of plasma configuration referred to as the compact toroids.The physics of the spheromak and their collisions is similar to a variety of astrophysical events, like coronal loops and filaments, relativistic jets and plasmoids. They are particularly useful for studying magnetic reconnection events, when two or more spheromaks collide. Spheromaks are easy to generate using a ""gun"" that ejects spheromaks off the end of an electrode into a holding area, called the flux conserver. This has made them useful in the laboratory setting, and spheromak guns are relatively common in astrophysics labs. These devices are often, confusingly, referred to simply as ""spheromaks"" as well; the term has two meanings.Spheromaks have been proposed as a magnetic fusion energy concept due to their long confinement times, which was on the same order as the best tokamaks when they were first studied. Although they had some successes during the 1970s and 80s, these small and lower-energy devices had limited performance and most spheromak research ended when fusion funding was dramatically curtailed in the late 1980s. However, in the late 1990s research demonstrated that hotter spheromaks have better confinement times, and this led to a second wave of spheromak machines. Spheromaks have also been used to inject plasma into a bigger magnetic confinement experiment like a tokamak.
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