Okay, not a force field, exactly, but a gigantic magnetic field surrounding the Earth, and it acts like a force field, protecting the planet – and all the life – from space radiation. Gamma radiation emission is a nuclear process that occurs to rid an unstable nucleus of excess energy after most nuclear reactions. This intense solar radiation as it is known in physical geography originates in the sun’s core and is eventually sent to Earth after convection (the vertical movement of energy) forces it away from the sun’s core. So, the relatively small moon exerts a much stronger tidal force on Earth than the gargantuan sun because it is so much closer—on average the moon is 384,399.9 kilometers (238,855 miles) from Earth, while the sun is 149.6 million kilometers (92.92 million miles) away. Both alpha and beta particles have an electric charge and mass, and thus are quite likely to interact with other atoms in their path. Gamma (γ) radiation consists of photons with a wavelength less than 3x10 −11 meters (greater than 10 19 Hz and 41.4 keV). It takes approximately eight minutes for solar radiation to reach the Earth after leaving the sun’s surface. The data collected by NISTAR on Earth's albedo, incoming short- and long-wave radiation, and outgoing long-wave radiation has never been measured from Lagrangian point 1 (L1) position before. DSCOVR's location at the L1 observing position permits long integration times because no scanning is …
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