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Earth`s Magnetic Field
Earth`s Magnetic Field

... Currents in the molten part of Earth beneath the crust provide a better explanation for Earth’s magnetic field. Most geologists think that moving charges looping around within Earth create its magnetic field. Because of Earth’s great size, the speed of charges would have to be less than one millimet ...
declination - Troop 233, Bethesda, MD
declination - Troop 233, Bethesda, MD

... needle would not rotate freely, and hence would not work properly. The Earth's magnetic field, as measured by a magnetic sensor on or above the Earth's surface, is actually the sum of magnetic fields generated by a variety of sources. These fields are superimposed on each other and through inductive ...
Populating the asteroid belt from two parent source - SwRI
Populating the asteroid belt from two parent source - SwRI

... migration of Jupiter and Saturn brings them inwards to 1.5 AU, truncating the disk of planetesimals in the terrestrial planet region, before migrating outwards toward their current locations. This model, informally titled ‘‘The Grand Tack,’’ examines the planetary dynamics of the solar system bodies ...
Gamma-ray absorption and pair echos at very high
Gamma-ray absorption and pair echos at very high

Magnetism Lesson 2
Magnetism Lesson 2

Earths Layer Model
Earths Layer Model

Simultaneous observation of the electron acceleration and ion deceleration
Simultaneous observation of the electron acceleration and ion deceleration

Solar chromospheric flares: energy release, transport and radiation
Solar chromospheric flares: energy release, transport and radiation

Chiral ratio of the compressional and shear velocity for the
Chiral ratio of the compressional and shear velocity for the

Credit: X-ray: NASA/CXC/UMass/D. Wang et al.; Optical: Caltech/SSC/S.Stolovy
Credit: X-ray: NASA/CXC/UMass/D. Wang et al.; Optical: Caltech/SSC/S.Stolovy

Chapter 22: Magnetism
Chapter 22: Magnetism

S3P2. Students will investigate magnets and how they affect other
S3P2. Students will investigate magnets and how they affect other

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

Lecture 8 Plasma shaping and vertical stability
Lecture 8 Plasma shaping and vertical stability

Model Atmosphere Results (Kurucz 1979, ApJS, 40, 1)
Model Atmosphere Results (Kurucz 1979, ApJS, 40, 1)

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

A Solar Polar Imager Concept - The National Academies of
A Solar Polar Imager Concept - The National Academies of

magnetic field
magnetic field

Full text - terrapub
Full text - terrapub

Greenstone - Miami University
Greenstone - Miami University

... imparts color to a mineral by its presence in the structure) in the earth. When iron is in its divalent oxidation state (Fe2+), as is found in such minerals as olivine, pyroxenes, amphiboles, chlorites, and epidote, it typically imparts a green color. Exceptions to this do exist and include, for exa ...
Lecture 10: Tokamak continued
Lecture 10: Tokamak continued

Pole Shift (magnetic)
Pole Shift (magnetic)

Understanding Magnetism - The Physics of Bruce Harvey
Understanding Magnetism - The Physics of Bruce Harvey

Stellar Atmospheres
Stellar Atmospheres

Observation of the Bastille day flare on 2000 July 14
Observation of the Bastille day flare on 2000 July 14

< 1 ... 6 7 8 9 10 11 12 13 14 ... 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.
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