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imported>Hhudson (The timing of the BOT (about 07:30 UT). Upper panel: Fluxes of X-ray emission detected by GOES in two spectral channels and the smoothed time derivative of X-ray flux in the 1-8 A channel. Middle panel: Temperature of the flare plasma estimated from the G) |
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Latest revision as of 14:35, 1 November 2024
The timing of the BOT (about 07:30 UT). Upper panel: Fluxes of X-ray emission detected by GOES in two spectral channels and the smoothed time derivative of X-ray flux in the 1-8 A channel. Middle panel: Temperature of the flare plasma estimated from the GOES data, and flux density of solar radio emission detected by Nobeyama Radio Polarimeter at 17 GHz. Bottom panel: Emission measure of the flare plasma estimated from the GOES data and count rates from the ACS SPI. Lines (a, b, c and d) mark the moments presented in Figure 2.
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