SDO HMI 2011-10-29 09:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.14 | 97.99 | 26.62 | 112.27 | 12.83 | 300.51 | 64.73 | 282.02 | 0.9023 | 280.7 | 62.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.99 | 4.42 | 2.97 | 6.60 | 12.86 | 306.88 | 71.10 | 282.00 | 0.9444 | -527.8 | -291.6 | |
| 0.95 | 2.08 | 1.42 | 3.10 | 13.19 | 306.91 | 71.14 | 282.35 | 0.9446 | -280.5 | -294.2 | |
| 0.00 | 2.43 | 0.00 | 3.42 | 12.79 | 305.72 | 69.94 | 281.92 | 0.9378 | -482.0 | -355.6 | |
| 1.04 | 7.46 | 1.33 | 9.56 | 11.43 | 303.50 | 67.73 | 280.45 | 0.9240 | -551.7 | -329.9 | |
| 1.99 | 3.56 | 2.39 | 4.26 | 11.93 | 301.78 | 66.01 | 280.99 | 0.9123 | 362.3 | 240.4 | |
| 0.00 | 6.94 | 0.00 | 8.19 | 13.33 | 301.36 | 65.58 | 282.54 | 0.9095 | -127.0 | -5.0 | |
| 0.00 | 0.52 | 0.00 | 0.61 | 13.58 | 301.20 | 65.42 | 282.82 | 0.9083 | 281.0 | 286.8 | |
| 0.00 | 4.68 | 0.00 | 5.37 | 12.93 | 300.57 | 64.79 | 282.11 | 0.9037 | -316.0 | -352.5 | |
| 0.52 | 61.65 | 0.57 | 66.55 | 12.88 | 299.48 | 63.70 | 282.08 | 0.8956 | -351.3 | 228.0 | |
| 0.00 | 1.21 | 0.00 | 1.34 | 13.58 | 299.54 | 63.76 | 282.86 | 0.8962 | 153.0 | 139.4 | |
| 0.00 | 1.04 | 0.00 | 1.14 | 13.44 | 299.33 | 63.55 | 282.71 | 0.8946 | 252.0 | 172.1 | |
| 12.05 | -9.00 | 13.03 | -9.00 | 13.05 | 298.87 | 63.09 | 282.29 | 0.8910 | 597.2 | 999999 | |
| 4.60 | -9.00 | 4.91 | -9.00 | 12.62 | 298.47 | 62.70 | 281.81 | 0.8878 | 677.5 | 999999 | |
| 0.00 | 1.13 | 0.00 | 1.22 | 13.69 | 298.83 | 63.05 | 283.01 | 0.8908 | 428.0 | 388.2 | |
| 0.00 | 0.87 | 0.00 | 0.91 | 13.88 | 297.97 | 62.20 | 283.25 | 0.8842 | 453.0 | 365.1 | |
| 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. | |