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Large-scale magnetic flux concentrations from turbulent stresses 331 A. Brandenburg , N. Kleeorin
Large-scale magnetic flux concentrations from turbulent stresses 331 A. Brandenburg , N. Kleeorin

Neutron star to strange star - Institute of Physics, Bhubaneswar
Neutron star to strange star - Institute of Physics, Bhubaneswar

Spectroscopic study of the decomposition process of
Spectroscopic study of the decomposition process of

... also detected in the examined mixtures. When tetramethylsilane was introduced into the discharge zone, in the 200 – 300 nm region, strong spectrum of silicon was observed (see Fig. 2c). Similar spectrum of Si I was identified in the mixture containing methyltrichlorosilane [16] and tetrachlorosilane ...
ppt
ppt

... From the ratio of radio to TeV emission: a same distribution of electrons produces synchrotron (radio, X-ray) and TeV (IC) but synchrotron depends directly on field while IC and pion decays do not. From sharp outer X-ray edges seen in several young SNRs (Kepler, Cas A, Tycho, SN1006). Shock front co ...
PHY418 Particle Astrophysics - Particle Physics and Particle
PHY418 Particle Astrophysics - Particle Physics and Particle

... Detection of cosmic rays • Cosmic rays are strongly interacting • primary cosmic rays shower high in the atmosphere • Therefore, two approaches to detection: • detect primary particle at high altitude • requires balloon-borne or space-based experiment ...
Does the Sun rotate?
Does the Sun rotate?

High-Energy Astrophysics
High-Energy Astrophysics

ppt
ppt

High energy universe – Satellite missions
High energy universe – Satellite missions

2 - BYU Physics and Astronomy
2 - BYU Physics and Astronomy

... (ii) the pattern which would be seen by an observer looking parallel to the field lines, and (iii) the pattern which would be seen by an observer looking normally across the field lines. (f) Is this example a case of the “normal” or “anomalous” Zeeman effect? (½) (g) Suppose the total separation bet ...
2 - BYU Physics and Astronomy
2 - BYU Physics and Astronomy

Conceptual steps towards exploring the fundamental nature of our Sun
Conceptual steps towards exploring the fundamental nature of our Sun

GRA VIT A TIONAL
GRA VIT A TIONAL

... In the accretion phase, the in ow speed is accelerated at least to (4 0 5) 2 cs and as a result magnetic eld lines are strongly dragged and squeezed to the center (see Fig. 1c of Tomisaka 1996b). Beside these, the rotation speed is accelerated as the infall proceeds. Just after the state shown in F ...
Acta Polytechnica
Acta Polytechnica

... both with own plasma, created by itself with impact ionization, and with HVGD plasma, which develops this electron beam (Fig. 5). Analyzing the results of PBD formation mechanism in LGEG operation, it is possible to report on the following. Having certain parameters of EB and neutral gas pressure, t ...
Model Answers for CE Physics Questions
Model Answers for CE Physics Questions

... A: The average kinetic energy of molecules is a measure of temperature. During evaporation, the faster moving molecules near the liquid surface escape, leaving the relatively slower molecules in the liquid. As a result, the average kinetic energy is decreased, and hence the temperature is lower. Q: ...
2 Solar magnetic fields. - High Altitude Observatory
2 Solar magnetic fields. - High Altitude Observatory

... The effects of magnetic fields in spectra of astronomical plasmas are generally more subtle, because bright objects are usually hot and so spectral lines are broadened by thermal motions. Only when magnetic fields are strong can one use spectroscopy alone. More generally, one must also use “plasma po ...
the magnetic field reversal as a to a mechanism of the origin
the magnetic field reversal as a to a mechanism of the origin

PowerPoint
PowerPoint

... radioactive dating, by comparing the intensity left over after a given time to that predicted by the half life of the isotope. • Positron emitters can be used for PET scanning of isotope distribution inside a human/animal body. ...
Spectral-Type Trends: Absorption
Spectral-Type Trends: Absorption

... But stellar winds are stronger and denser for hotter and more luminous stars, so an X-ray hardness trend governed by wind attenuation is expected.) To explore the effect of wind absorption, we have developed a radiation transport model of thermal X-ray emission from plasma embedded within an extende ...
Zeeman observations: Measuring magnetic fields in the atomic and
Zeeman observations: Measuring magnetic fields in the atomic and

... are also used as a tracers of the Galactic magnetic field [21]. The Galactic ASKAP Survey (GASKAP, [12]) will already provide an unbiased, flux-limited survey of OH masers associated with high-mass star forming regions. This survey will serve as base to carry OH Zeeman observations with SKA1 towards ...
P3 Further Physics - The Thomas Cowley High School
P3 Further Physics - The Thomas Cowley High School

... Electromagnetic induction - generators • When a wire cuts through magnetic field lines a potential difference is induced in the wire. • If the wire is part of a complete circuit a current will flow. • The current is increased by moving the wire faster or using stronger magnets. ...
Current Systems in Planetary Magnetospheres and Ionospheres
Current Systems in Planetary Magnetospheres and Ionospheres

Full text - terrapub
Full text - terrapub

... the center in the draped field geometry (E × B drift) giving rise to the plasma sheet ion population. Dubinin et al. (1993a) have shown that magnetic shear stresses (i.e. j × B force) might be important for the ion dynamics. Lichtenegger et al. (1995) tried to take into consideration this force by i ...
Sun Test Answers
Sun Test Answers

Acoustic Waves - The Evergreen State College
Acoustic Waves - The Evergreen State College

... The surface of the Sun is around 5800 Kelvin (K), yet between 103 and 104 km from the surface there is a dramatic spike in the temperature of the corona, to more than 1 million K. One source of this heating probably involves the transformation of acoustic waves to magnetic waves. Acoustic waves are ...
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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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