Search results
Results from the WOW.Com Content Network
A rendering of the magnetic field lines of the magnetosphere of the Earth. In astronomy and planetary science, a magnetosphere is a region of space surrounding an astronomical object in which charged particles are affected by that object's magnetic field. [1] [2] It is created by a celestial body with an active interior dynamo.
A gameplay screenshot showing the protagonist shining their flashlight down the left hallway. Five Nights at Freddy's 4 is a point-and-click survival horror game. [1] Like previous games in the series, the player is tasked with surviving from midnight to 6:00 a.m. against homicidal animatronics.
Artistic representation of Earth's magnetosphere. The plasma sheet is highlighted in yellow. In the magnetosphere, the plasma sheet is a sheet-like region of denser (0.3-0.5 ions/cm 3 versus 0.01-0.02 in the lobes) [citation needed] hot plasma and lower magnetic field located on the magnetotail and near the equatorial plane, between the magnetosphere's north and south lobes.
Five Nights at Freddy's (FNaF) is an American multimedia horror franchise created and owned by Scott Cawthon. The franchise began with the release of its first video game on 8 August 2014. Three sequels were released up to July 2015, setting a Guinness World Record for "most video game sequels released in a year".
The magnetosheath is the region of space between the magnetopause and the bow shock of a planet's magnetosphere.The regularly organized magnetic field generated by the planet becomes weak and irregular in the magnetosheath due to interaction with the incoming solar wind, and is incapable of fully deflecting the highly charged particles.
Main page; Contents; Current events; Random article; About Wikipedia; Contact us; Help; Learn to edit; Community portal; Recent changes; Upload file
1964 - IMP-1 (Interplanetary Monitoring Platform 1) reports a large bow shock formed in the solar wind ahead of the magnetosphere, and a long magnetic tail on the night side of the Earth. 1964 - Syun-Ichi Akasofu (Japan-U.S.) and Sydney Chapman revive and expand Birkeland's notion of a "polar magnetic storm", now named "magnetic substorm."
This opening is called the dayside reconnection and occurs on the side of the magnetosphere facing the solar wind source. In the second stage, the flux travels in the direction of the solar wind across the magnetosphere. In the third stage, at the magnetotail, reconnection closes the open flux, allowing for a new cycle to begin. This ...