SDO HMI 2011-10-25 03:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.37 | 233.76 | 36.16 | 170.58 | -21.71 | 331.56 | 39.76 | 233.95 | 0.7370 | -454.0 | -311.1 | |
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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 |
| 0.00 | 1.39 | 0.00 | 1.12 | -19.73 | 338.43 | 46.62 | 240.09 | 0.7915 | 477.0 | 349.2 | |
| 0.00 | 0.61 | 0.00 | 0.49 | -19.43 | 338.27 | 46.46 | 240.37 | 0.7888 | 443.0 | 373.1 | |
| 0.00 | 1.13 | 0.00 | 0.90 | -19.12 | 338.06 | 46.26 | 240.63 | 0.7855 | 468.0 | 412.0 | |
| 0.00 | 0.70 | 0.00 | 0.56 | -19.29 | 338.08 | 46.27 | 240.45 | 0.7864 | 313.0 | 330.2 | |
| 0.00 | 0.70 | 0.00 | 0.55 | -18.95 | 337.91 | 46.10 | 240.76 | 0.7833 | 535.0 | 480.5 | |
| 0.00 | 1.04 | 0.00 | 0.83 | -19.07 | 337.82 | 46.01 | 240.57 | 0.7830 | 586.0 | 531.0 | |
| 3.65 | 11.21 | 2.86 | 8.77 | -19.00 | 337.20 | 45.39 | 240.36 | 0.7768 | 663.1 | 549.8 | |
| 2.26 | -7.00 | 1.76 | -7.00 | -18.73 | 336.97 | 45.16 | 240.57 | 0.7734 | 745.5 | 999999 | |
| 0.96 | 1.65 | 0.74 | 1.28 | -18.52 | 336.81 | 45.00 | 240.73 | 0.7710 | 679.8 | 594.5 | |
| 0.00 | 1.48 | 0.00 | 1.15 | -19.18 | 336.95 | 45.14 | 240.02 | 0.7752 | 688.0 | 532.5 | |
| 0.00 | 2.09 | 0.00 | 1.63 | -19.59 | 336.82 | 45.02 | 239.47 | 0.7759 | 474.0 | 447.7 | |
| 0.00 | 1.13 | 0.00 | 0.87 | -19.14 | 336.40 | 44.59 | 239.79 | 0.7698 | 817.0 | 642.8 | |
| 0.00 | 0.96 | 0.00 | 0.73 | -23.04 | 333.94 | 42.14 | 233.90 | 0.7664 | -462.0 | -312.7 | |
| 5.65 | 209.67 | 4.10 | 151.70 | -21.41 | 331.31 | 39.51 | 234.19 | 0.7326 | -826.2 | -396.4 | |
| 3.56 | -14.00 | 2.59 | -14.00 | -21.80 | 331.15 | 39.34 | 233.63 | 0.7334 | -624.2 | 999999 | |
| 33.29 | -14.00 | 24.11 | -14.00 | -22.15 | 330.76 | 38.96 | 232.97 | 0.7318 | -995.5 | 999999 | |
| 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. | |