• Study Resource
  • Explore
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
university of california, san diego
university of california, san diego

SOFIA Polarimetry: Recent Musings
SOFIA Polarimetry: Recent Musings

bution of Solar Proton Events Affecting the Earth E
bution of Solar Proton Events Affecting the Earth E

Inhomogeneous cloud coverage through the Coulomb explosion of
Inhomogeneous cloud coverage through the Coulomb explosion of

Cosmic Rays near Proxima Centauri b
Cosmic Rays near Proxima Centauri b

Geophysical Turbulence Program
Geophysical Turbulence Program

...  Stream function perturbations with a prescribed kinetic energy spectrum: ...
Periodic Spectral Line Asymmetries In Solar Coronal Structures From Slow Magnetoacoustic Waves
Periodic Spectral Line Asymmetries In Solar Coronal Structures From Slow Magnetoacoustic Waves

... will symmetric in number density, temperature and1atvelocity, The coronal volume element isamodelled asGaussian profile at any giv line be emission , respectively. (3)local ...
The Solar Tachocline: A Self-Consistent Model of Magnetic
The Solar Tachocline: A Self-Consistent Model of Magnetic

Attitude Determination and Orbital Estimation Using Earth Position
Attitude Determination and Orbital Estimation Using Earth Position

Telescope Bernard Lyot/Narval The Observatory of Stellar Magnetism
Telescope Bernard Lyot/Narval The Observatory of Stellar Magnetism

Studies of an inductively coupled negative hydrogen ion radio
Studies of an inductively coupled negative hydrogen ion radio

2008 HSC Exam Paper - Physics
2008 HSC Exam Paper - Physics

... Which statement best explains how induction cooktops heat food? (A) Eddy currents generated in the water in the food produce heat. (B) Eddy currents generated in the base of the saucepan produce heat. (C) Resistance in the glass of the cooktop produces heat. (D) Resistance in the element beneath ...
Winds from accretion disks driven by the radiation and
Winds from accretion disks driven by the radiation and

Can a Fast-Mode EUV Wave Generate a Stationary Front?
Can a Fast-Mode EUV Wave Generate a Stationary Front?

Full-Text PDF
Full-Text PDF

AS Physics Contents Guide
AS Physics Contents Guide

on the rotational dynamics of magnetically threaded disks around
on the rotational dynamics of magnetically threaded disks around

Ion-supported tori: a thermal bremsstrahlung model for the X
Ion-supported tori: a thermal bremsstrahlung model for the X

9 core formulas - Universal Healing Tao Switzerland
9 core formulas - Universal Healing Tao Switzerland

Matter in strong magnetic fields - the Max Planck Institute for the
Matter in strong magnetic fields - the Max Planck Institute for the

... characteristics of the thermal emission, proper interpretations of the observations require a detailed understanding of the physical properties of the neutron star envelope in the presence of intense magnetic fields (B ⲏ1012 G). B. Laboratory physics motivation ...
STELLAR ABLATION OF PLANETARY ATMOSPHERES
STELLAR ABLATION OF PLANETARY ATMOSPHERES

constraints on primordial magnetic fields with cmb anisotropies
constraints on primordial magnetic fields with cmb anisotropies

... One of the possible interpretations of this lack of photons is the presence of a diffuse magnetic field not associated with existing structures. Assuming a model for the background light and the Blazar emission it is possible to derive hypothetical lower limits on the field amplitude. Current limits ...
PDF only - at www.arxiv.org.
PDF only - at www.arxiv.org.

Correlation Between Nitrogen and Oxygen Content in Planetary
Correlation Between Nitrogen and Oxygen Content in Planetary

... Discussion ...
Relationship between solar wind dynamic pressure and amplitude
Relationship between solar wind dynamic pressure and amplitude

< 1 ... 3 4 5 6 7 8 9 10 11 ... 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.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report