Diagram of the solar flare activity and CME
CME, coronal material is ejected into space at high speeds magnetic field arising from the solar corona and being released into the solar wind.
A solar flare is a sudden brightness observed near the Sun‘s surface.solar flares typically occur near sunspots where magnetic field emit radiation in several bands of the electromagnetic spectrum (white light, untraviolet, x-rays, gamma rays)
A G-type main-sequence star (Spectral type: G-V), often (and imprecisely) called a yellow dwarf, or G dwarf star, is a main-sequence star (luminosity class V) of spectral type G. Such a star as the Sun is the best known (and most visible) example of a G-type main-sequence star.
A solar flare is a sudden brightness observed near the Sun‘s surface.solar flares typically occur near sunspots where magnetic field emit radiation in several bands of the electromagnetic spectrum (white light, untraviolet, x-rays, gamma rays)
A G-type main-sequence star (Spectral type: G-V), often (and imprecisely) called a yellow dwarf, or G dwarf star, is a main-sequence star (luminosity class V) of spectral type G. Such a star as the Sun is the best known (and most visible) example of a G-type main-sequence star.
Comments
Post a Comment