Animati3


Forfatter/Opretter:
Dr. Nikolai Tsyganenko, USRA/NASA/GSFC
Kredit:
http://modelweb.gsfc.nasa.gov/magnetos/data-based/modeling.html, http://modelweb.gsfc.nasa.gov/magnetos/data-based/animati3.gif
Shortlink:
https://dkwiki.dk/b/22f3f
kilde:
Wikimedia Commons
størrelse:
560 x 510 Pixel (811368 Bytes)
beskrivelse:
Simulation of Earth's magnetic field in interaction with (solar) interplanetar magnetic field (IMF): The animation illustrates the dynamical changes of the global magnetic field in the course of a disturbance: a temporary compression of the magnetosphere by enhanced flow of the solar wind is followed by a tailward stretching of the field lines. Eventually, the increase of the tail magnetic field results in a sudden collapse of the nightside field (a substorm ) and a gradual recovery of the magnetosphere to its pre-storm configuration.
Licens:
Public domain

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