SDO HMI 2011-11-24 11:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.21 | 39.58 | 10.63 | 29.05 | 16.29 | 297.90 | 46.00 | 290.67 | 0.7401 | -467.0 | -191.5 | |
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back to the solar disc SDO HMI 2011-11-24 11:58:57 UT
See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.50 | 16.53 | 9.38 | 12.39 | 16.01 | 299.17 | 47.27 | 289.92 | 0.7533 | -652.4 | -292.1 | |
| 0.00 | 1.46 | 0.00 | 1.08 | 15.47 | 298.78 | 46.88 | 289.32 | 0.7477 | -535.0 | -390.3 | |
| 0.00 | 0.94 | 0.00 | 0.70 | 15.42 | 298.45 | 46.55 | 289.33 | 0.7440 | -661.0 | -550.8 | |
| 0.00 | 1.46 | 0.00 | 1.07 | 15.70 | 297.95 | 46.05 | 289.85 | 0.7392 | -783.0 | -620.6 | |
| 0.00 | 1.80 | 0.00 | 1.31 | 15.62 | 297.79 | 45.89 | 289.77 | 0.7372 | -796.0 | -638.3 | |
| 1.71 | 3.08 | 1.25 | 2.26 | 16.23 | 297.80 | 45.89 | 290.59 | 0.7388 | 477.2 | 300.2 | |
| 0.00 | 2.06 | 0.00 | 1.49 | 15.87 | 297.21 | 45.30 | 290.29 | 0.7313 | -803.0 | -610.0 | |
| 0.00 | 4.11 | 0.00 | 3.02 | 17.77 | 297.62 | 45.71 | 292.67 | 0.7411 | 779.0 | 582.5 | |
| 0.00 | 1.88 | 0.00 | 1.34 | 16.26 | 296.18 | 44.28 | 291.12 | 0.7209 | -567.0 | -472.0 | |
| 0.00 | 1.03 | 0.00 | 0.73 | 16.39 | 295.96 | 44.06 | 291.37 | 0.7187 | -495.0 | -425.6 | |
| 0.00 | 1.80 | 0.00 | 1.29 | 17.43 | 296.10 | 44.20 | 292.73 | 0.7234 | 636.0 | 544.2 | |
| 0.00 | 1.11 | 0.00 | 0.79 | 16.30 | 295.72 | 43.82 | 291.33 | 0.7158 | -641.0 | -552.2 | |
| 0.00 | 0.86 | 0.00 | 0.59 | 17.44 | 294.22 | 42.32 | 293.41 | 0.7022 | -563.0 | -444.2 | |
| 0.00 | 1.46 | 0.00 | 0.99 | 16.91 | 292.99 | 41.09 | 293.14 | 0.6862 | -617.0 | -556.9 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |