Ribut geomagnetik - Wikipedia Bahasa Melayu, ensiklopedia bebas

Ribut geomagnetik adalah ganguan sementara pada magnetosfera yang disebabkan oleh gelombang kejutan angin suria dan/atau awan medan magnet yang bertindak balas dengan medan mangnet bumi. Peningkatan pada tekanan angin suria pada awalnya menekan magnetosfera dan medan magnet angin suria bertindak balas dengan medan mangnet Bumi dan memindahkan peningkatan tenaga pada magnetosfera. Kedua tindak balas menyebabkan peningkatan pada pergerakan plasma melalui magnetosfera (didorong oleh peningkatan medan eletrik dalam magnetosfera) dan peningkatan arus eletrik pada magnetosfera dan ionosfera.

Rujukan

Bacaan lanjut

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Laman web berkait

Websites relating to coping with or measuring solar storms

Solar Cycle 24 and VHF Aurora Website (www.solarcycle24.com)
Live solar and geomagnetic activity data (www.spaceweatherlive.com)
The warp and woof of a geomagnetic storm — NASA's Space Science News.
NOAA Space Weather Scales Diarkibkan 2008-05-16 di Wayback Machine — NOAA.
NOAA Space Weather Prediction Center Diarkibkan 2012-08-06 di Wayback Machine - NOAA.
NOAA Space Weather Alerts — NOAA.
NASA — Carrington Super Flare Diarkibkan 2009-08-01 di Wayback Machine NASA May 6, 2008
Ionosphere and thermosphere response to geomagnetic storm simulated by a Coupled Magnetosphere Ionosphere Thermosphere model
SSC automatic alert system Diarkibkan 2013-04-29 di Wayback Machine (experimental, broadcast on Twitter)
AirSatOne:Recent Geophysical Alert Messages Diarkibkan 2012-12-17 di archive.today

Aurora Watch, at Lancaster University, gives email warnings of coronal mass ejections and geomagnetic storms for aurora watching enthusiasts:

http://aurorawatch.lancs.ac.uk/
http://geomag.usgs.gov
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Power grid related links