SDO HMI 2011-06-14 11:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.34 | 125.09 | 20.25 | 64.47 | -15.08 | 246.01 | 0.95 | 183.51 | 0.2789 | 53.1 | 21.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.65 | -14.88 | 248.45 | 3.38 | 191.84 | 0.2792 | 878.0 | 667.4 | |
| 7.61 | 14.87 | 3.92 | 7.66 | -14.78 | 247.97 | 2.91 | 190.28 | 0.2761 | 1128.1 | 747.7 | |
| 0.00 | 6.25 | 0.00 | 3.23 | -15.26 | 247.76 | 2.69 | 189.25 | 0.2834 | 742.0 | 615.2 | |
| 3.90 | 41.88 | 2.00 | 21.52 | -14.46 | 247.62 | 2.56 | 189.26 | 0.2699 | 1023.1 | 915.9 | |
| 9.88 | -4.00 | 5.08 | -4.00 | -14.53 | 247.37 | 2.31 | 188.33 | 0.2703 | 1149.0 | 999999 | |
| 0.00 | 4.17 | 0.00 | 2.15 | -15.32 | 247.28 | 2.22 | 187.62 | 0.2832 | 666.0 | 573.2 | |
| 4.17 | -4.00 | 2.14 | -4.00 | -14.15 | 247.18 | 2.11 | 187.84 | 0.2635 | 1203.4 | 999999 | |
| 1.99 | -4.00 | 1.03 | -4.00 | -14.59 | 247.09 | 2.02 | 187.29 | 0.2707 | 836.6 | 999999 | |
| 0.00 | 1.09 | 0.00 | 0.56 | -14.94 | 246.33 | 1.27 | 184.49 | 0.2752 | 726.0 | 575.1 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -13.27 | 245.79 | 0.73 | 182.90 | 0.2464 | 895.0 | 709.1 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -13.64 | 245.20 | 0.14 | 180.53 | 0.2525 | -801.0 | -507.3 | |
| 8.25 | 22.93 | 4.26 | 11.85 | -15.64 | 245.01 | -0.05 | 179.82 | 0.2861 | -978.2 | -815.1 | |
| 0.00 | 2.36 | 0.00 | 1.21 | -14.18 | 244.64 | -0.43 | 178.41 | 0.2616 | -937.0 | -730.8 | |
| 2.54 | -12.00 | 1.31 | -12.00 | -15.67 | 244.60 | -0.46 | 178.44 | 0.2867 | -1060.6 | 999999 | |
| 1.00 | 1.99 | 0.51 | 1.03 | -15.10 | 244.57 | -0.49 | 178.27 | 0.2771 | -983.8 | -906.3 | |
| 0.00 | 1.63 | 0.00 | 0.84 | -15.86 | 244.38 | -0.68 | 177.72 | 0.2900 | -849.0 | -706.2 | |
| 0.00 | 1.81 | 0.00 | 0.93 | -14.94 | 244.35 | -0.71 | 177.48 | 0.2746 | -1099.0 | -906.7 | |
| 0.00 | 0.73 | 0.00 | 0.38 | -18.91 | 243.63 | -1.44 | 176.00 | 0.3413 | 746.0 | 478.1 | |
| 0.00 | 2.99 | 0.00 | 1.55 | -16.15 | 243.46 | -1.61 | 174.76 | 0.2959 | -900.0 | -693.2 | |
| 0.00 | 5.08 | 0.00 | 2.62 | -15.64 | 243.34 | -1.73 | 174.18 | 0.2876 | -1036.0 | -848.9 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -16.40 | 243.17 | -1.89 | 173.92 | 0.3006 | -898.0 | -656.9 | |
| 0.00 | 1.99 | 0.00 | 1.03 | -15.89 | 243.14 | -1.92 | 173.64 | 0.2921 | -1016.0 | -801.9 | |
| 0.00 | 2.08 | 0.00 | 1.08 | -16.08 | 242.82 | -2.24 | 172.68 | 0.2960 | -934.0 | -748.4 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -15.64 | 242.73 | -2.33 | 172.18 | 0.2888 | -1066.0 | -941.7 | |
| 0.00 | 4.26 | 0.00 | 2.21 | -16.34 | 242.63 | -2.43 | 172.18 | 0.3006 | -933.0 | -768.6 | |
| 0.00 | 1.00 | 0.00 | 0.52 | -15.45 | 242.61 | -2.45 | 171.67 | 0.2859 | -957.0 | -733.9 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -15.92 | 242.54 | -2.52 | 171.69 | 0.2940 | -828.0 | -670.6 | |
| 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. | |