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Space Weather - Coggle Diagram

- - - - -strong and spectacular explosions of gases -attain maximum brightness within a few seconds or minutes -light from solar flares takes 8 minutes to reach Earth while the charged gas particles take tens of minutes
    - - -huge loop or arched column of glowing gases over the sunspot -Prominence that are very strong can throw out matter from the sun into space at speeds ranging from 600km/s to more than 1000km/s -The prominence plasma is typically a hundred times more luminous and denser than trhe coronal plasma
  - - - -cells of plasma -hot rising plasma in the center ,cooler plasma falling in the narrow spaces between them -1000 kilometers in diameter -lifespam -8 to 20 minutes -super granuels
    - - -region of reduced surface temperature caused by concentrations of magnetic field flux that inhibit convection - appear in pairs of opposite magnetic polarity -appear dark because their temperature lower than surroundings granules -activities varies approximately 11 year (solar cycle)
  - - - -release of plasma and the solar corona -magnetized plasma consisting primarily of electrons and protons -often follow solar flares and are normally present during a solar prominence eruptions