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Voyager
Voyager

... spacecraft, you and your design team are going to work together, by brainstorming, revising your plans, building your design and then presenting to the class. ...
AMPTE:  NOTES  ON  THE  INITIAL ... WORK  IN  PROGRESS _ _ _ _ _... _
AMPTE: NOTES ON THE INITIAL ... WORK IN PROGRESS _ _ _ _ _... _

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Baby-Quiz

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... time to circle the Earth--a few minutes. View from North Pole ...
Mass vs. Weight
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... Gravity is a force among all objects in the universe. Within our solar system, every object is attracted to every other object due to gravity. The closer objects are and the more mass they have, the stronger the attraction. Gravitational forces among objects in the solar system cause distinct charac ...
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Fundamental nuclear symmetries meet classical electrodynamic

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... Every planet has its own unique features and characteristics. The solar system can be divided into two distinct planetary groups: – the inner planets, also called terrestrial, or Earth-like, planets; – the outer planets, or Jovian (in reference to Jupiter), planets. The terrestrial planets tend to b ...
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PYTS/ASTR 206 – Solar System Scales

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... called the corona. The temperature of the corona can be several million degrees. • Magnetic fields are thought to be responsible for these very high temperatures. • The corona is so hot it expands outward along with the Sun’s magnetic field and streams through the Solar System. This is known as the ...
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PDF file of Lecture 9a - Planet Jupiter

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Age of the Earth III - PowerPoint Lecture Notes

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Chapter 6 Our Solar System and Its Origin

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5th grade Solar System Test
5th grade Solar System Test

... location and the tilt of the earth. The order of the planets from the sun is Mercury, Venus, Earth, Mars, Jupiter, Saturn and Neptune. Therefore, Mercury, Venus, Earth, and Mars are the inner planets. The solar system has an elliptical orbit which means the orbit is oval or egg-shaped. ...
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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.
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