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Tutorial 3 Magnetostatics
Tutorial 3 Magnetostatics

Unit 4: Formation of the Earth
Unit 4: Formation of the Earth

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Week one: Space Physics and Aeronomy (pdf, 1.3 MB)

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... Step 2: Write down the new number without the zeros. Step 3: Write "x 10" after the number. Step 4: Write the number of times you moved the decimal as the power of 10. Note: If you moved the decimal to the left the exponent is positive, if you moved it to the right it is negative. Try it with these ...
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... atmosphere to balance the amount of energy coming from the Sun. At that point the surface stops heating up. However its temperature is higher than it would be if no greenhouse gases were present and infrared radiation could simply escape into space. 6. Clearly the larger the amount of greenhouse gas ...
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Teacher - Challenger Learning Center

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Chapter 7: Air-Sea Interaction Study Guide

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UV SURFACE ENVIRONMENT OF EARTH

... affects the surface UV environment for Earth-like planets through geological time and therefore the conditions for the origin and evolution of life. Depending on the intensity, UV radiation can be both useful and harmful to life as we know it. UV radiation can inhibit photosynthesis and cause damage ...
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Lecture #5: Evolution of the Earth`s Atmosphere

MAKE-UP ACTIVITY/QUIZ NAME: Date: SHORT ANSWERS: Are all
MAKE-UP ACTIVITY/QUIZ NAME: Date: SHORT ANSWERS: Are all

he Magnetosphere/Solar
he Magnetosphere/Solar

Kein Folientitel
Kein Folientitel

Origin and Structure of the Earth
Origin and Structure of the Earth

magnet Any material that attracts iron and materials that contain iron
magnet Any material that attracts iron and materials that contain iron

< 1 ... 40 41 42 43 44 45 46 47 >

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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