| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.30 | 187.82 | 35.47 | 118.38 | 34.01 | 267.68 | 10.13 | 346.35 | 0.6210 | 49.8 | -92.4 | |
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back to the solar disc SDO HMI 2010-12-31 19:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.89 | 107.76 | 13.19 | 68.05 | 33.67 | 269.55 | 12.00 | 343.80 | 0.6224 | -1129.5 | -355.3 | |
| 1.19 | -1.00 | 0.75 | -1.00 | 33.51 | 268.99 | 11.43 | 344.44 | 0.6183 | -848.1 | 999999 | |
| 0.00 | 0.93 | 0.00 | 0.59 | 34.14 | 268.79 | 11.23 | 345.02 | 0.6257 | -490.0 | -383.9 | |
| 0.00 | 2.63 | 0.00 | 1.67 | 34.17 | 268.43 | 10.87 | 345.49 | 0.6248 | -466.0 | -478.7 | |
| 0.00 | 1.27 | 0.00 | 0.79 | 33.09 | 266.75 | 9.19 | 347.17 | 0.6050 | 539.0 | 463.5 | |
| 0.00 | 1.61 | 0.00 | 1.02 | 34.41 | 266.83 | 9.27 | 347.64 | 0.6230 | -747.0 | -616.5 | |
| 0.00 | 1.53 | 0.00 | 0.95 | 33.20 | 266.48 | 8.92 | 347.58 | 0.6057 | 649.0 | 531.8 | |
| 0.00 | 0.93 | 0.00 | 0.59 | 34.60 | 266.63 | 9.07 | 347.97 | 0.6248 | -609.0 | -462.5 | |
| 1.70 | 61.82 | 1.06 | 38.78 | 33.48 | 265.65 | 8.09 | 348.81 | 0.6072 | 781.1 | 549.4 | |
| 0.00 | 1.70 | 0.00 | 1.08 | 35.45 | 265.26 | 7.70 | 350.02 | 0.6326 | 430.0 | 381.5 | |
| 9.00 | -9.00 | 5.64 | -9.00 | 34.14 | 265.07 | 7.51 | 349.83 | 0.6146 | 846.8 | 999999 | |
| 2.55 | 7.64 | 1.62 | 4.86 | 35.26 | 264.95 | 7.39 | 350.35 | 0.6293 | 740.0 | 566.1 | |
| 20.97 | -9.00 | 13.21 | -9.00 | 34.62 | 264.78 | 7.23 | 350.36 | 0.6204 | 873.7 | 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. | |