• Study Resource
  • Explore Categories
    • 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
talk-tutorial - Helioseismic and Magnetic Imager
talk-tutorial - Helioseismic and Magnetic Imager

Probability Distribution Function
Probability Distribution Function

The force-free magnetosphere of a rotating black hole
The force-free magnetosphere of a rotating black hole

INTERSTELLAR TRANSFER OF PLANETARY MICROBIOTA
INTERSTELLAR TRANSFER OF PLANETARY MICROBIOTA

Formation of Active Regions on the Rising Slope of the 23rd Solar
Formation of Active Regions on the Rising Slope of the 23rd Solar

... can only be done purely by empirical-statistical methods based on large uniform sequences of observations of different solar structures (mainly relative sunspot numbers). Solar activity forecast tasks are divided into three groups, depending on the task: short-term - of the order of a few days (but ...
The sun and the solar corona
The sun and the solar corona

... established by purely theoretical considerations, based on the measured energy output (luminosity), radius and mass, using of course all the applicable laws of physics. Making some simplifying assumptions, such as spherical symmetry, no rotation and no magnetic fields, basic models of the Sun’s inte ...
Conceptual steps towards exploring the fundamental nature of our Sun
Conceptual steps towards exploring the fundamental nature of our Sun

2 Gamma-Ray Production and Absorption Processes
2 Gamma-Ray Production and Absorption Processes

The Kuiper Belt: What We Know and What We Don`t - UCLA
The Kuiper Belt: What We Know and What We Don`t - UCLA

... (“irregular” means that the orbit around the planet is large and eccentric and, in this case, the orbital motion is opposite to the direction of Saturn’s spin). Phoebe was captured from elsewhere in the Solar system but the source region and the mechanism of capture remain unknown. One possible sour ...
Document
Document

Can We Successfully Apply A Solar Thin-Flux
Can We Successfully Apply A Solar Thin-Flux

...  Spin up to different  (0.25, 1, 4, 10, 25, 63, rigid rot. profile). Mainly PMS-stars, a few (sub)giants for comparison. ...
South Magnetic Pole - Maritime Museum Education
South Magnetic Pole - Maritime Museum Education

Geomagnetism - Brock University
Geomagnetism - Brock University

Geomagnetism. - Brock University
Geomagnetism. - Brock University

... magnetic poles at the time of rock formation). 3. The inclination of the RMS (the inclination of the Earth's field which reflects the latitude at which the rock ...
Answers for Student notes page
Answers for Student notes page

... • Where is the motion of electric charges in a common bar magnet? • The magnet as a whole may be stationary, but it is composed of atoms whose electrons are in constant motion about atomic nuclei. • This moving charge constitutes a tiny current and produces a magnetic field. Most substances are not ...
Tracing the release sites of the energy stored in the twisted coronal
Tracing the release sites of the energy stored in the twisted coronal

Kinetic aspects of the vortex-induced
Kinetic aspects of the vortex-induced

... magnetosheath components not distinguished) ...
Magnetic Field Variations - West Virginia University
Magnetic Field Variations - West Virginia University

Significance of the Kuiper Belt
Significance of the Kuiper Belt

... (“irregular” means that the orbit around the planet is large and eccentric and, in this case, the orbital motion is opposite to the direction of Saturn’s spin). Phoebe was captured from elsewhere in the Solar system but the source region and the mechanism of capture remain unknown. One possible sour ...
Magnets and Magnetism
Magnets and Magnetism

... Ferromagnets – magnets made with metals Electromagnets – produced by an electric current. Temporary magnets – made from materials that are easy to magnetize, but they lose their magnetization easily too. Permanent magnets – difficult to magnetize, but retain their magnetic properties better. ...
satellites
satellites

Hewitt/Lyons/Suchocki/Yeh, Conceptual Integrated Science
Hewitt/Lyons/Suchocki/Yeh, Conceptual Integrated Science

... • The electric force between any two charged particles depends on the product of their charges and their distance of separation, as specified in Coulomb’s law. • If the charged particles are moving with respect to each other, there is an additional force between them, called the magnetic force. • Th ...
Hewitt/Lyons/Suchocki/Yeh, Conceptual Integrated Science
Hewitt/Lyons/Suchocki/Yeh, Conceptual Integrated Science

... • Earth is itself a huge magnet. • The magnetic poles of Earth are widely separated from the geographic poles. • The magnetic field of Earth is not due to a giant magnet in its interior—it is due to electric currents. • Most Earth scientists think that moving charges looping around within the molten ...
Primary science goal: map geothermal heat flux under an ice sheet
Primary science goal: map geothermal heat flux under an ice sheet

Magnetism - SchoolRack
Magnetism - SchoolRack

< 1 ... 9 10 11 12 13 14 15 16 17 ... 48 >

Van Allen radiation belt



A radiation belt is a layer of energetic charged particles that is held in place around a magnetized planet, such as the Earth, by the planet's magnetic field. The Earth has two such belts and sometimes others may be temporarily created. The discovery of the belts is credited to James Van Allen and as a result the Earth's belts bear his name. The main belts extend from an altitude of about 1,000 to 60,000 kilometers above the surface in which region radiation levels vary. Most of the particles that form the belts are thought to come from solar wind and other particles by cosmic rays. The belts are located in the inner region of the Earth's magnetosphere. The belts contain energetic electrons that form the outer belt and a combination of protons and electrons that form the inner belt. The radiation belts additionally contain less amounts of other nuclei, such as alpha particles. The belts endanger satellites, which must protect their sensitive components with adequate shielding if their orbit spends significant time in the radiation belts. In 2013, NASA reported that the Van Allen Probes had discovered a transient, third radiation belt, which was observed for four weeks until destroyed by a powerful, interplanetary shock wave from the Sun.
  • studyres.com © 2026
  • DMCA
  • Privacy
  • Terms
  • Report