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Dusty AGN Tori
Dusty AGN Tori

Document
Document

1 Pc2 EMIC waves generated high off the equator in the dayside 2
1 Pc2 EMIC waves generated high off the equator in the dayside 2

... [15] We now consider whether the wave packets are reflected from the bi-ion hybrid frequency location in the magnetosphere [Perraut et al., 1984; Guglielmi et al., 2001]. Choosing this location at 15 MLat, the field line length between the two conjugate bi-ion frequency locations is around 5  104 ...
Relaxation of Blazar Induced Pair Beams in Cosmic Voids
Relaxation of Blazar Induced Pair Beams in Cosmic Voids

... In this paper, we reanalyze the stability of blazars induced ultra-relativistic pair beams. In particular, we use a Monte Carlo model of the electromagnetic shower to quantify the beam properties at various distances from the blazar, and analyze the stability of the produced beam following the work ...
Yield of Ozone, Nitrite Nitrogen and Hydrogen Peroxide Versus
Yield of Ozone, Nitrite Nitrogen and Hydrogen Peroxide Versus

The  on­ quilibrium  ISIS
The  on­ quilibrium  ISIS

... Characteristics of our spectral code  (Ji PhD thesis 2006)   based on the updated atomic data (CHIANTI , APED) the atomic data and the code are  separate                                                                      ...
Higher Order Drifts and the Parallel Equation of Motion
Higher Order Drifts and the Parallel Equation of Motion

So if you look at it, this is exactly the structure of
So if you look at it, this is exactly the structure of

... The total of fields come together which pull together just like putting hand and your hold hands together, is called gravity and you pull each other together. And then a bunch of there who pull away from you to try to pull outwards, we call this magnetic fields or magnetical fields which is the repu ...
The Cosmic Rays and Our Galaxy
The Cosmic Rays and Our Galaxy

Magnetic quenching of turbulent diffusivity - Andrés Muñoz
Magnetic quenching of turbulent diffusivity - Andrés Muñoz

PHY418 Particle Astrophysics
PHY418 Particle Astrophysics

... • relative velocities of objects in Galactic disc are only 10s of km/s, so fractional energy gain per reflection is only ~10−8 • There is no obvious reason why different sources should ...
Accreting neutron stars: strong gravity and type I bursts - UvA-DARE
Accreting neutron stars: strong gravity and type I bursts - UvA-DARE

disks surviving the radiation pressure of radio pulsars
disks surviving the radiation pressure of radio pulsars

Cosmological dynamics with non-minimally coupled scalar field and
Cosmological dynamics with non-minimally coupled scalar field and

... 1/ Introduction The so-called CDM new standard model of cosmology has reached a robustness level comparable to the one of the standard model of particle physics. However these two standard models are in conflict about the issue of the dark matter, an outcome of the cosmological standard model that ...
Accretion to Stars with Non
Accretion to Stars with Non

Full Paper - PDF - Armagh Observatory
Full Paper - PDF - Armagh Observatory

Document
Document

McConnell XGPolarimetry SSE
McConnell XGPolarimetry SSE

... photon energy and absorption depth) to the magnetic field, rotation of polarization position angle with pulse phase provides a probe of the magnetic-field geometry. The existence of a non-dipolar field [12] would support other evidence for such fields in some accreting pulsars [13], due perhaps to t ...
Conceptual Design of the International Axion Observatory (IAXO)
Conceptual Design of the International Axion Observatory (IAXO)

... A third-generation experiment, the CERN Axion Solar Telescope (CAST), began data collection in 2003. The experiment uses a Large Hadron Collider (LHC) dipole prototype magnet with a magnetic field of up to 9 T over a length of 9.3 m [25]. Like Sumico, CAST is able to follow the Sun for several hours ...
Effects of neutron-star superconductivity on
Effects of neutron-star superconductivity on

1 LOCAL HELIOSEISMOLOGY OF NEAR
1 LOCAL HELIOSEISMOLOGY OF NEAR

No Slide Title
No Slide Title

Nature of Gravitation
Nature of Gravitation

... absolute zero the thermal radiation, and with it the Casimir force, should disappear. But actual experiments in 1958 by Sparnaay revealed that instead a "residual" attractive force persisted even at absolute zero [15]. Therefore the "vacuum" even at absolute zero temperature is not completely empty ...
PPT
PPT

... trans-field direction (perpendicular to poloidal field line) is balanced and solve (poloidal) field aligned flow. • If we consider more realistic situation in 2D, we need to solve additional equation, so-called Grad-Shafranov equation (trans-field equation) which describing force balance perpendicul ...
PDF only
PDF only

... determined by the Little Effect. Furthermore, novel orbital dynamics driven by transient magnetic states for both ferromagnetic and paramagnetic systems under external, strong magnetic environments are embraced by the Little Effect. The Little Effect determines that strong magnetic environments frus ...
< 1 ... 5 6 7 8 9 10 11 12 13 ... 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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