Solar X-rays: Geomagnetic Field: |
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Since computers operate with magnetic storage devices and flowing electrons magnetic interference is common. Below are charts that are updated approx every ten minutes to show the electronic flux and X-Ray radiation that is present in the earths atmosphere. |
The fluctuations in the atmosphere can effect data line transmissions, computer processors , short term memory storage (RAM) and magnetic hard drive storage. You may also experience blurred CRT screens and possible obtain a spot on the screen. These may be removed by using the degauss option on the monitor configuring buttons. Slow data transmissions may occur across long distance transmission lines (telephone or data lines) as these charged electrons are traveling through the physical cable a magnetic charge may erase the arrangement of these particles causing the sending source to resend the packets excessively creating a false Denial of Service (DOS) effect. |
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Normal: Solar X-ray flux is quiet (< 1.00e-6 W/m^2) |
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Active: Solar X-ray flux is active (>= 1.00e-6 W/m^2) |
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M Class Flare: An M Class flare has occurred (X-ray flux >= 1.00e-5 W/m^2) |
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X Class Flare: An X Class flare has occurred (X-ray flux >= 1.00e-4 W/m^2) |
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Quiet: the Geomagnetic Field is quiet (Kp < 4) |
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Active: the Geomagnetic Field has been unsettled (Kp=4) |
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Storm: A Geomagnetic Storm has occurred (Kp>4) |
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X-Ray Flux | Satellite Environment (combined) | Electron Flux |
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Magnetometer | Estimated Kp Index | GOES 8 Proton Flux |
Special thanks to the NOAA Space Environment Center for the data and plots.
Visit their Today's Space Weather site (the source of these plots)