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SID Sudden Ionospheric Disturbance is a phenomenon that occurs when x-ray flares
from the sun ionize the D layer of the Ionosphere “which is about 60 KM up”. The
ionization of this region of the Ionosphere briefly causes signals to bounce off that layer
allowing signals to be received from over the horizon that normally could not be received
during the day. By monitoring distant stations we can study the affects of solar flaring on
the Ionosphere. Below are graphs from my monitoring station that are updated once a day
@ 00:00 UTC. For more info about SID monitoring visit Stanford University’s SOLAR
Center web site @
Stanford University SOLAR Center
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