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The Sun, with some sunspots visible, during solar cycle 22 (1992).
The Sun, with some sunspots visible, during solar cycle 22 (1992).
Artist's depiction of solar wind colliding with Earth's magnetosphere.
Artist's depiction of solar wind colliding with Earth's magnetosphere.
Image artifacts (diffraction spikes and vertical streaks) appearing in a CCD image of a major solar flare due to the excess incident radiation
Image artifacts (diffraction spikes and vertical streaks) appearing in a CCD image of a major solar flare due to the excess incident radiation
An X3.2-class solar flare observed in different wavelengths. Clockwise from top left: 304, 335, 131, and 193 Å
An X3.2-class solar flare observed in different wavelengths. Clockwise from top left: 304, 335, 131, and 193 Å
Electric currents in Earth's dayside ionosphere can be strengthened during a large solar flare.
Electric currents in Earth's dayside ionosphere can be strengthened during a large solar flare.
Richard Carrington's sketch of the first recorded solar flare (A and B mark the initial bright points which moved over the course of five minutes to C
Richard Carrington's sketch of the first recorded solar flare (A and B mark the initial bright points which moved over the course of five minutes to C and D before disappearing.)