SDO HMI 2011-11-26 05:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.53 | 37.49 | 19.47 | 51.95 | 16.90 | 297.28 | 68.46 | 287.57 | 0.9338 | 36.5 | 130.6 | |
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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 |
| 1.03 | 11.22 | 1.71 | 18.46 | 16.40 | 301.19 | 72.37 | 286.71 | 0.9559 | 145.2 | -29.9 | |
| 0.00 | 1.28 | 0.00 | 2.06 | 16.01 | 300.54 | 71.72 | 286.34 | 0.9525 | -372.0 | -279.3 | |
| 5.65 | -1.00 | 9.23 | -1.00 | 16.47 | 300.85 | 72.03 | 286.80 | 0.9542 | -381.0 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.95 | 16.11 | 300.42 | 71.60 | 286.45 | 0.9519 | -426.0 | -366.6 | |
| 0.00 | 0.77 | 0.00 | 1.08 | 16.30 | 297.62 | 68.80 | 286.86 | 0.9366 | -422.0 | -434.2 | |
| 0.00 | 1.28 | 0.00 | 1.61 | 16.11 | 294.97 | 66.15 | 286.90 | 0.9201 | 260.0 | 215.6 | |
| 0.34 | 2.40 | 0.43 | 2.98 | 16.30 | 294.86 | 66.04 | 287.12 | 0.9195 | 398.0 | 309.9 | |
| 0.00 | 1.71 | 0.00 | 2.13 | 16.89 | 294.72 | 65.90 | 287.77 | 0.9190 | 322.0 | 277.6 | |
| 2.23 | 3.68 | 2.80 | 4.64 | 17.41 | 295.01 | 66.19 | 288.30 | 0.9212 | 359.7 | 298.8 | |
| 0.00 | 1.71 | 0.00 | 2.12 | 17.20 | 294.55 | 65.74 | 288.13 | 0.9181 | 417.0 | 367.5 | |
| 0.00 | 0.43 | 0.00 | 0.54 | 17.81 | 294.99 | 66.17 | 288.74 | 0.9214 | 287.0 | 209.8 | |
| 0.00 | 1.20 | 0.00 | 1.47 | 16.90 | 294.27 | 65.45 | 287.83 | 0.9160 | -372.0 | -286.5 | |
| 4.28 | 10.10 | 5.30 | 12.56 | 17.67 | 294.58 | 65.76 | 288.63 | 0.9186 | 603.9 | 449.9 | |
| 0.00 | 1.11 | 0.00 | 1.35 | 18.02 | 293.85 | 65.03 | 289.11 | 0.9140 | -127.0 | -115.8 | |
| 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. | |