File:195f1.png
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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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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 21:24, 22 February 2013 | | 1,484×1,415 (653 KB) | Hhudson (Talk | contribs) | (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) |
| 21:16, 22 February 2013 |  | 1,417×709 (195 KB) | Hhudson (Talk | contribs) | (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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