WBL6_Lecture_Ch19
... The closer together (that is, the denser) the B field lines, the stronger the magnetic field. At any location, the direction of the magnetic field is tangent to the field line, or equivalently, the way the north end of a compass points. ...
... The closer together (that is, the denser) the B field lines, the stronger the magnetic field. At any location, the direction of the magnetic field is tangent to the field line, or equivalently, the way the north end of a compass points. ...
Latitudinal and radial gradients of galactic cosmic ray protons in the
... a combination of temporal and spatial variations. Ulysses was launched first towards Jupiter. Following the fly-by of Jupiter in February 1992, the spacecraft has been traveling in an elliptical, Sun-focused orbit inclined at 80.2 degrees to the solar equator. The characteristics of the Ulysses traj ...
... a combination of temporal and spatial variations. Ulysses was launched first towards Jupiter. Following the fly-by of Jupiter in February 1992, the spacecraft has been traveling in an elliptical, Sun-focused orbit inclined at 80.2 degrees to the solar equator. The characteristics of the Ulysses traj ...
Physics - Magnetism
... _a=1 NASA provides an explanation of the Earth's magnetosphere as well as magnetic field lines. This site also includes links to learn more about each topic covered. Www-istp.gsfc.nasa.gov,. 'Magnetism'. N.p., 2015. Web. 16 June 2015. Retrieved from http://www-istp.gsfc.nasa.gov/Education/Imagnet.ht ...
... _a=1 NASA provides an explanation of the Earth's magnetosphere as well as magnetic field lines. This site also includes links to learn more about each topic covered. Www-istp.gsfc.nasa.gov,. 'Magnetism'. N.p., 2015. Web. 16 June 2015. Retrieved from http://www-istp.gsfc.nasa.gov/Education/Imagnet.ht ...
File
... • Draw lines through and around the magnet to show the magnetic field. • Describe what happens to the strength of the magnetic fields as you go further away from the magnets. • “As the magnets move further away from each other, the ...
... • Draw lines through and around the magnet to show the magnetic field. • Describe what happens to the strength of the magnetic fields as you go further away from the magnets. • “As the magnets move further away from each other, the ...
Device for Controlled Distribution of FePt
... tumours, infections, blood clots, for local hyperthermia and other [1 – 10]. Such administration can reduce unwanted distribution of drugs thus minimizing side effects such as caused by systematically administered chemotherapy [6]. The distance from the magnets to the locations where particles are s ...
... tumours, infections, blood clots, for local hyperthermia and other [1 – 10]. Such administration can reduce unwanted distribution of drugs thus minimizing side effects such as caused by systematically administered chemotherapy [6]. The distance from the magnets to the locations where particles are s ...
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.