
Planet Jupiter
... liquid hydrogen. Within the planet pressure and temperature are so high that there is no clear boundary between the gas and liquid. Jupiter probably has a central core of rocky material about 1.5 times the diameter of Earth and 10 to 15 times more massive. Over this may rest an enormous mantle of li ...
... liquid hydrogen. Within the planet pressure and temperature are so high that there is no clear boundary between the gas and liquid. Jupiter probably has a central core of rocky material about 1.5 times the diameter of Earth and 10 to 15 times more massive. Over this may rest an enormous mantle of li ...
Magnetism and Electricity
... (b) Like poles of magnets always repel one another. (c) Magnetic south pole of the Earth is towards its geographic north pole. ...
... (b) Like poles of magnets always repel one another. (c) Magnetic south pole of the Earth is towards its geographic north pole. ...
1B11 Foundations of Astronomy Star names and magnitudes
... understanding the coupling between solar wind and planetary atmospheres (auroras), as well as acceleration of particles in space and astrophysical plasmas (solar flares, etc..) The frozen-in flux approximation (in the case of RM>>1) leads to a picture of space plasmas contained within separated re ...
... understanding the coupling between solar wind and planetary atmospheres (auroras), as well as acceleration of particles in space and astrophysical plasmas (solar flares, etc..) The frozen-in flux approximation (in the case of RM>>1) leads to a picture of space plasmas contained within separated re ...
Lecture 4 Sea-Floor Spreading POLAR
... for rocks of different ages from North America and Eurasia produces two curves, the so-called “polar wandering curves”. Note that as the curves get younger they converge. Fitting the continents back together results in a single curve. Nonetheless, the positions still do not correspond with the curre ...
... for rocks of different ages from North America and Eurasia produces two curves, the so-called “polar wandering curves”. Note that as the curves get younger they converge. Fitting the continents back together results in a single curve. Nonetheless, the positions still do not correspond with the curre ...
Intro to Solar System
... from east to west • planets are on smaller spheres, rotating at different speeds, east to west • Earth is motionless in the center ...
... from east to west • planets are on smaller spheres, rotating at different speeds, east to west • Earth is motionless in the center ...
Moving Charges And Magnetism Moving Charges Moving charges
... Current carrying loop as magnetic dipole Its upper face has current flowing in anti-clockwise direction. It has North polarity. Its lower face has current flowing in clockwise direction. It has South polarity. Magnetic dipole moment of current loop (M) is given by M=NIA. Magnetic dipole moment of a ...
... Current carrying loop as magnetic dipole Its upper face has current flowing in anti-clockwise direction. It has North polarity. Its lower face has current flowing in clockwise direction. It has South polarity. Magnetic dipole moment of current loop (M) is given by M=NIA. Magnetic dipole moment of a ...
Magnets - Bari Science Lab
... • Electromagnetism—the interaction between electricity and magnetism. ...
... • Electromagnetism—the interaction between electricity and magnetism. ...
The Dimensions of the Solar System
... planets, and then laying them out along a line from the Sun outward. Unfortunately, the sizes of the Sun and planets often need to be exaggerated relative to their distances to make them visible. This may seem inevitable given the huge difference in the distances versus the sizes, but we see this as ...
... planets, and then laying them out along a line from the Sun outward. Unfortunately, the sizes of the Sun and planets often need to be exaggerated relative to their distances to make them visible. This may seem inevitable given the huge difference in the distances versus the sizes, but we see this as ...
The Transport of Open Magnetic Flux on the Solar Surface and its
... electron heat flux. The electron heat flux data is now ambiguous. ...
... electron heat flux. The electron heat flux data is now ambiguous. ...
B - UConn Physics
... • I have two wires, labeled 1 and 2, carrying equal current, into the page. We know that wire 1 produces a magnetic field, and that wire 2 has moving charges. What is the force on wire 2 from wire 1 ? ...
... • I have two wires, labeled 1 and 2, carrying equal current, into the page. We know that wire 1 produces a magnetic field, and that wire 2 has moving charges. What is the force on wire 2 from wire 1 ? ...
Magnetism - effinghamschools.com
... • Early Greeks discovered a rare ore in a region of Turkey called Magnesia. • In the 12th century, the Chinese found that a single stone made of this ore if suspended will always point toward geographical north ...
... • Early Greeks discovered a rare ore in a region of Turkey called Magnesia. • In the 12th century, the Chinese found that a single stone made of this ore if suspended will always point toward geographical north ...
Magnetic separation
... • The rate of sample introduction is controlled by the angle of the feed outlet shoot and the strength of feed vibration • The speed at which material moved down the ramp is controlled by the strength of the chute ...
... • The rate of sample introduction is controlled by the angle of the feed outlet shoot and the strength of feed vibration • The speed at which material moved down the ramp is controlled by the strength of the chute ...
11129_sou05_23ste_co_wb
... . In a diagram of a magnetic field, they are magnetic field lines represented by ________________________. By convention, the lines are drawn coming out of entering into ________________________ the north pole and ________________________ the south pole of a magnet. ...
... . In a diagram of a magnetic field, they are magnetic field lines represented by ________________________. By convention, the lines are drawn coming out of entering into ________________________ the north pole and ________________________ the south pole of a magnet. ...
Solar System - Delta Education
... arc representing the Sun. ACTIVITY 9 Students use satellite models and light sources to demonstrate planetary rotation and revolution. They learn that one rotation of a planet about its axis constitutes a day and that one revolution of a planet around the Sun constitutes a year. Later, they role-pla ...
... arc representing the Sun. ACTIVITY 9 Students use satellite models and light sources to demonstrate planetary rotation and revolution. They learn that one rotation of a planet about its axis constitutes a day and that one revolution of a planet around the Sun constitutes a year. Later, they role-pla ...
Physics: Particles from Space - Advice for Practitioners (Revised
... Austrian physicist Victor Hess made measurements of radiation at high altitudes from a balloon, to try and get away from possible sources on Earth. He was surprised to find the measurements actually increased with altitude. At an altitude of 5000 m the intensity of radiation was found to be five tim ...
... Austrian physicist Victor Hess made measurements of radiation at high altitudes from a balloon, to try and get away from possible sources on Earth. He was surprised to find the measurements actually increased with altitude. At an altitude of 5000 m the intensity of radiation was found to be five tim ...
Geomagnetic storm

A geomagnetic storm is a temporary disturbance of the Earth's magnetosphere caused by a solar wind shock wave and/or cloud of magnetic field that interacts with the Earth's magnetic field. The increase in the solar wind pressure initially compresses the magnetosphere. The solar wind's magnetic field interacts with the Earth’s magnetic field and transfers an increased energy into the magnetosphere. Both interactions cause an increase in plasma movement through the magnetosphere (driven by increased electric fields inside the magnetosphere) and an increase in electric current in the magnetosphere and ionosphere.During the main phase of a geomagnetic storm, electric current in the magnetosphere creates a magnetic force that pushes out the boundary between the magnetosphere and the solar wind. The disturbance in the interplanetary medium that drives the storm may be due to a solar coronal mass ejection (CME) or a high speed stream (co-rotating interaction region or CIR) of the solar wind originating from a region of weak magnetic field on the Sun’s surface. The frequency of geomagnetic storms increases and decreases with the sunspot cycle. CME driven storms are more common during the maximum of the solar cycle, while CIR driven storms are more common during the minimum of the solar cycle.Several space weather phenomena tend to be associated with or are caused by a geomagnetic storm. These include: solar energetic Particle (SEP) events, geomagnetically induced currents (GIC), ionospheric disturbances that cause radio and radar scintillation, disruption of navigation by magnetic compass and auroral displays at much lower latitudes than normal. In 1989, a geomagnetic storm energized ground induced currents that disrupted electric power distribution throughout most of the province of Quebec and caused aurorae as far south as Texas.