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If neutron star is born with a strong magnetic field
If neutron star is born with a strong magnetic field

Document
Document

Talk
Talk

The Magnetic Universe
The Magnetic Universe

... Although the rotation of a star can meaning that each parcel of light has a starlight polarisation has allowed us to amplify an existing magnetic field in the random orientation. However, Hiltner build up a picture of the magnetic field in object’s interior, this can only work if one and Hall clearl ...
Toward a Global Description of the Nucleus
Toward a Global Description of the Nucleus

Evolution of Neutron Star Magnetic Fields
Evolution of Neutron Star Magnetic Fields

... could be expected both due to spontaneous evolution and due to accretion. A physical model of field evolution should satisfy the observational constraints that relatively little magnetic field decay should take place in isolated radio pulsar population (dominated by neutron stars in the age range 10 ...
Energy conservation and Poynting`s theorem
Energy conservation and Poynting`s theorem

Quantum mechanical model for the study of pressure
Quantum mechanical model for the study of pressure

... Abstract. The knowledge of plasma equation of state and photoabsorption requires suitable and realistic models for the description of ions. The number of relevant electronic configurations of ions in hot dense plasmas can be immense (increasing with atomic number Z). In such cases, calculations rely ...
SOLID-STATE PHYSICS II 2007 O. Entin-Wohlman
SOLID-STATE PHYSICS II 2007 O. Entin-Wohlman

**** 1
**** 1

...  Measurement of the magnetic field using Zeeman broadening ~ λ In most atoms, there exist several electron configurations with the same energy, so that transitions between these configurations and another correspond to a single spectral line. The presence of a magnetic field breaks this degeneracy, ...
File
File

... amounts of X-rays. Solar flares are often associated with coronal mass ejections. ...
Sun
Sun

Does the Sun rotate?
Does the Sun rotate?

Dissipation and heating in solar wind turbulence: from the macro to
Dissipation and heating in solar wind turbulence: from the macro to

Could planting trees in the desert mitigate climate change?
Could planting trees in the desert mitigate climate change?

REPORTS Terahertz Magnetic Response from Artificial Materials
REPORTS Terahertz Magnetic Response from Artificial Materials

Order-of-Magnitude Physics – Solution Set 4
Order-of-Magnitude Physics – Solution Set 4

1 Planetary-Spin heat, Jupiter- Saturn-Solar Tidal
1 Planetary-Spin heat, Jupiter- Saturn-Solar Tidal

... It was good for the Earth. If we assumed that all planets were similar to ours, they would have to be mostly rock and have an iron core, some water and an atmosphere. As we know, that is not true. Each planet and moon is very different and we can not superimpose our earth’s history on the other plan ...
A regular period for Saturn’s magnetic field that  G. Giampieri
A regular period for Saturn’s magnetic field that G. Giampieri

... modulation of the radio source20. On the other hand, the magnetic field signal, which we have only studied over the much shorter time span of the Cassini mission, shows no obvious variations in period, phase or amplitude, and can well be used to define an improved rotation rate of the planetary sour ...
DUNE: The Deep Underground Neutrino Experiment
DUNE: The Deep Underground Neutrino Experiment

Fig. 1 - Experimental set-up - Estudo Geral
Fig. 1 - Experimental set-up - Estudo Geral

poster
poster

PPT file
PPT file

THEORETICAL STUDY OF THE SOLAR MAGNETIC CYCLE AND
THEORETICAL STUDY OF THE SOLAR MAGNETIC CYCLE AND

... Thesis Summary of Bidya Binay Karak Indian Institute of Science, Bangalore Sunspots are the seats of large-scale strong magnetic field on the surface of the Sun. The number of sunspots on the face of the Sun is observed to vary cyclically with an average period of about 11 years. However the solar c ...
HEA_Pulsars
HEA_Pulsars

< 1 ... 22 23 24 25 26 27 28 29 30 ... 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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