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Solar flares are likely to affect the electrojet current more strongly as a result of the absorption, in the lower E-region, of the shorter wavelength solar X-rays flare spectrum.
It is reasonable to distinguish among four different mechanisms responsible for absorption: regular absorption due to solar UV illumination, absorption associated with energetic particles precipitation, absorption connected with X-rays flare and additional absorption in Auroral oval area.
Then the orbiting telescope got smacked in the eye by an x-ray flare.
Then, in early 2014, a bright x-ray flare erupted from close to Sgr A*.
Observers say this x-ray flare makes the black hole virtually a certainty.
The x-ray flare is large in extent, has fine strulctuire, and follows a neutral magnetic line.
The most intense X-ray flare from this active region was X15 at 1350 UT on March 6.
In 1996 they observed a large x-ray flare that lasted a few minutes using an x-ray detector aboard the Compton Gamma Ray Observatory satellite.
Flare spectra are taken as power laws, with the logarithmic slope a parameter based on the observed statistics of the most energetic hard X-ray flare spectra.
Each flare has different spectral characteristics, strong narrow line flare, broad line flare and continuum gamma-ray flare.
(1) The 1998 September 9 event was an impulsive hard X-ray flare and CME was not observed.
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