Yup Bobbywhy's links back up what I said in my earlier post...
I'm not aware of the magnetic fields of individual spots, even when they snap, having much effect at any great distance from the sun.
The overall magnetic field of the sun is a different thing.
But for some reason I have never heard of those waves. One usually only hears of disturbances of the solar wind when it suddenly increases from a usual 300 km/s to 600 km/s or so, just like you describe. So I want to know more about the other waves that go at light speed, 1000 times faster than normal solar wind. My question is how strong such disturbances are by the the time they arrive at the earth, that is 8 minutes later, and in what way they interact with the geomagnetic field.
well from the flares you have a burst of light, radio waves, Xrays all that get here in that 8 and a bit minute period
Its the X-rays that cause the main initial effects namely shortwave ( 1 - 30 MHz ) black outs (SW fadeouts)
This is caused by enhancement of the D layer of the Ionosphere by the incoming X-Rays, it enhances VLF propagation but stops the HF (~ 1 - 30MHz) signals from reaching and being reflected by the F1/F2 layers.
The term for this phenomena is called a SID, Sudden Ionospheric Disturbance.
the other event that is directly related to this is a PCA, a Polar Cap Absorption. This affects HF radio signals using the polar paths...
A polar cap absorption event results from the ionisation of the D-layer of the polar ionosphere by high energy protons ( X-rays). A PCA causes a HF radio blackout for trans polar circuits (polar paths) and can last several days. PCAs are almost always preceded by a major solar flare with the time between the flare event and the onset of the PCA ranging from few minutes to several hours.
Solar activity is one of my fav subjects and has been for some 40 years since I first started observing and drawing sunspot groups. Then went on to giving lectures on solar activity, aurora and also the effects of those on radio propagation
cheers
Dave