SDO HMI 2011-12-08 05:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.78 | 82.20 | 35.54 | 107.59 | 17.01 | 137.24 | 66.56 | 288.53 | 0.9247 | 24.9 | -37.4 | |
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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 |
| 1.62 | 42.47 | 2.34 | 60.46 | 17.18 | 139.64 | 68.96 | 288.33 | 0.9408 | 310.7 | -120.2 | |
| 11.17 | -1.00 | 15.84 | -1.00 | 16.96 | 139.29 | 68.61 | 288.14 | 0.9387 | -570.9 | 999999 | |
| 1.71 | 8.87 | 2.22 | 11.59 | 16.87 | 137.33 | 66.65 | 288.27 | 0.9269 | 122.9 | -342.1 | |
| 0.94 | -3.00 | 1.22 | -3.00 | 16.87 | 137.17 | 66.50 | 288.29 | 0.9259 | -112.5 | 999999 | |
| 0.00 | 1.19 | 0.00 | 1.52 | 16.68 | 136.65 | 65.98 | 288.16 | 0.9225 | -124.0 | -177.6 | |
| 10.66 | 17.91 | 13.35 | 22.49 | 16.37 | 136.30 | 65.62 | 287.88 | 0.9199 | 548.0 | 247.6 | |
| 0.00 | 1.19 | 0.00 | 1.52 | 17.05 | 136.60 | 65.93 | 288.57 | 0.9225 | 198.0 | 72.2 | |
| 0.00 | 2.81 | 0.00 | 3.51 | 17.02 | 136.20 | 65.53 | 288.59 | 0.9199 | 419.0 | 300.6 | |
| 0.00 | 0.94 | 0.00 | 0.83 | 21.43 | 123.70 | 53.02 | 296.16 | 0.8307 | -442.0 | -358.9 | |
| 0.68 | 3.24 | 0.57 | 2.69 | 18.19 | 121.78 | 51.10 | 292.88 | 0.8048 | 446.6 | 479.3 | |
| 0.00 | 0.85 | 0.00 | 0.73 | 21.74 | 122.19 | 51.51 | 297.00 | 0.8182 | 506.0 | 401.3 | |
| 0.00 | 1.88 | 0.00 | 1.55 | 19.84 | 121.19 | 50.51 | 295.06 | 0.8036 | 607.0 | 457.9 | |
| 0.00 | 0.85 | 0.00 | 0.70 | 20.79 | 120.53 | 49.85 | 296.41 | 0.8001 | 504.0 | 408.7 | |
| 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. | |