| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.46 | 232.01 | 54.29 | 200.48 | 7.69 | 129.62 | -54.74 | 81.38 | 0.8196 | -175.4 | -154.2 | |
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back to the solar disc SDO HMI 2011-11-29 14:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 1.17 | 5.63 | 132.57 | -51.78 | 83.71 | 0.7889 | -550.0 | -484.1 | |
| 0.00 | 1.03 | 0.00 | 0.83 | 5.42 | 132.41 | -51.95 | 83.99 | 0.7906 | -721.0 | -612.6 | |
| 18.97 | 113.48 | 15.43 | 92.21 | 7.50 | 132.05 | -52.31 | 81.40 | 0.7957 | -903.6 | -363.5 | |
| 1.20 | -3.00 | 0.98 | -3.00 | 8.69 | 131.83 | -52.53 | 79.93 | 0.7991 | 305.2 | 999999 | |
| 13.93 | 24.87 | 11.60 | 20.76 | 6.53 | 130.97 | -53.39 | 82.70 | 0.8063 | -661.2 | -4.2 | |
| 0.00 | 2.73 | 0.00 | 2.30 | 6.91 | 130.61 | -53.75 | 82.26 | 0.8102 | -381.0 | -247.6 | |
| 1.20 | 2.56 | 1.01 | 2.17 | 7.62 | 130.38 | -53.98 | 81.40 | 0.8130 | -328.4 | -235.1 | |
| 3.50 | 5.30 | 2.98 | 4.51 | 7.26 | 130.14 | -54.22 | 81.86 | 0.8152 | -496.3 | -369.1 | |
| 0.00 | 0.94 | 0.00 | 0.80 | 7.08 | 129.96 | -54.39 | 82.10 | 0.8168 | -287.0 | -227.1 | |
| 0.00 | 1.37 | 0.00 | 1.18 | 7.43 | 129.69 | -54.66 | 81.69 | 0.8197 | -362.0 | -174.4 | |
| 2.22 | 2.99 | 1.93 | 2.59 | 7.04 | 129.35 | -55.01 | 82.19 | 0.8229 | -332.6 | -226.0 | |
| 0.00 | 0.77 | 0.00 | 0.68 | 7.57 | 128.78 | -55.58 | 81.60 | 0.8288 | -452.0 | -340.4 | |
| 2.82 | 5.64 | 2.59 | 5.16 | 8.95 | 127.28 | -57.08 | 80.08 | 0.8440 | 624.0 | 351.7 | |
| 0.34 | 68.11 | 0.32 | 65.38 | 8.00 | 126.15 | -58.21 | 81.28 | 0.8536 | 508.2 | 147.1 | |
| 12.73 | -14.00 | 12.10 | -14.00 | 8.30 | 125.97 | -58.39 | 80.95 | 0.8554 | 832.7 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.74 | 7.67 | 125.71 | -58.65 | 81.71 | 0.8574 | 601.0 | 528.3 | |
| 5.55 | -14.00 | 5.35 | -14.00 | 8.32 | 125.50 | -58.86 | 80.96 | 0.8596 | 491.8 | 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. | |