| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.63 | 180.27 | 35.55 | 113.23 | 34.03 | 267.71 | 9.05 | 347.76 | 0.6178 | -9.7 | -47.3 | |
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back to the solar disc SDO HMI 2010-12-31 17:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.93 | 102.24 | 0.59 | 64.31 | 33.93 | 270.05 | 11.38 | 344.71 | 0.6234 | -540.6 | -355.3 | |
| 24.12 | -1.00 | 15.16 | -1.00 | 33.70 | 269.51 | 10.85 | 345.28 | 0.6185 | -1114.2 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.86 | 34.25 | 268.78 | 10.12 | 346.47 | 0.6232 | -521.0 | -411.3 | |
| 0.00 | 0.76 | 0.00 | 0.48 | 34.02 | 268.47 | 9.80 | 346.78 | 0.6193 | -461.0 | -352.3 | |
| 0.00 | 1.87 | 0.00 | 1.18 | 34.28 | 268.39 | 9.72 | 346.99 | 0.6224 | -710.0 | -531.0 | |
| 0.00 | 0.76 | 0.00 | 0.48 | 34.65 | 268.14 | 9.48 | 347.47 | 0.6265 | -527.0 | -448.3 | |
| 0.00 | 1.36 | 0.00 | 0.84 | 33.09 | 266.83 | 8.16 | 348.56 | 0.6019 | 800.0 | 580.2 | |
| 0.00 | 0.59 | 0.00 | 0.37 | 33.38 | 266.43 | 7.76 | 349.21 | 0.6048 | 412.0 | 398.6 | |
| 1.61 | 3.57 | 1.00 | 2.21 | 33.56 | 265.91 | 7.24 | 349.98 | 0.6059 | 510.7 | 378.5 | |
| 3.74 | 55.28 | 2.33 | 34.59 | 33.89 | 265.26 | 6.59 | 350.96 | 0.6089 | 899.4 | 606.1 | |
| 5.60 | -10.00 | 3.50 | -10.00 | 34.18 | 265.17 | 6.51 | 351.16 | 0.6127 | 936.4 | 999999 | |
| 2.80 | 11.38 | 1.77 | 7.21 | 35.15 | 265.14 | 6.48 | 351.49 | 0.6257 | 791.1 | 551.9 | |
| 0.00 | 1.10 | 0.00 | 0.70 | 35.60 | 265.03 | 6.37 | 351.76 | 0.6316 | 389.0 | 293.9 | |
| 17.83 | -10.00 | 11.20 | -10.00 | 34.55 | 264.91 | 6.25 | 351.62 | 0.6172 | 904.6 | 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. | |