The Earth's magnetic field redirects the Sun's particle radiation (such as alpha and beta particles); it doesn't exactly shield it. Some of it will break around the Earth's magnetosphere, like water breaking around the bow of a ship. But some of it does end up travelling down the magnetic field lines until it collides with particles in our atmosphere, ionizing them. This is what produces the aurora. In sufficient quantities, this ionizing process can also produce electromagnetic interference, sufficient to disrupt radio communications or even overload and burn out circuitry. These days, electrical companies pay very close attention to the space weather forecast.<br /><br />The molecules of our atmosphere block a lot of the high energy electromagnetic radiation, such as gamma rays. (And famously, the ozone layer blocks a significant amount of the ultraviolet radiation.) It has its limits (a sufficiently large burst will make it through) but because it shields us so well, if astronomers want to do x-ray astronomy or study gamma ray bursts, they generally have to do it with either space telescopes or airplane-mounted telescopes. <div class="Discussion_UserSignature"> <p> </p><p><font color="#666699"><em>"People assume that time is a strict progression of cause to effect, but actually from a non-linear, non-subjective viewpoint it's more like a big ball of wibbly wobbly . . . timey wimey . . . stuff."</em> -- The Tenth Doctor, "Blink"</font></p> </div>