Solar storm effects on humans
Solar storms The sun continuously emits a stream of charged particles (“solar wind”) in all directions. The wind blows radially away from the sun, its speed and density are highly variable, and it contains a magnetic field that is also highly variable in magnitude and direction. When the sun is relatively calm, the only manifestation of solar wind may be the auroras (Northern or Southern Lights), caused by the excitation of atmospheric oxygen and nitrogen by the wind’s energetic electrons (Lenz, 2004). A geomagnetic storm, or solar storm, is caused by a solar wind shock wave that strikes Earth's magnetic field, resulting in a worldwide temporary disturbance of Earth's magnetosphere, distinct from regular diurnal variations. This only occurs if the shock wave travels in a direction toward Earth. During a geomagnetic storm, “portions of the solar wind's energy are transferred to the magnetosphere, causing Earth's magnetic field to change rapidly in directi...