SDO HMI 2014-11-25 11:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.68 | 69.45 | 8.57 | 35.71 | 4.77 | 158.18 | -15.20 | 77.77 | 0.2686 | 148.2 | -7.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.60 | 2.91 | 0.30 | 1.48 | 4.06 | 160.92 | -12.46 | 78.57 | 0.2206 | -1060.9 | -824.8 | |
| 3.08 | 4.80 | 1.57 | 2.44 | 4.38 | 160.86 | -12.53 | 77.19 | 0.2229 | -1150.2 | -867.5 | |
| 0.00 | 3.17 | 0.00 | 1.61 | 4.41 | 160.37 | -13.02 | 77.52 | 0.2311 | -520.0 | -487.7 | |
| 1.37 | 3.25 | 0.70 | 1.66 | 4.73 | 160.12 | -13.27 | 76.38 | 0.2364 | -981.9 | -805.7 | |
| 2.48 | 6.17 | 1.27 | 3.14 | 4.32 | 159.89 | -13.50 | 78.31 | 0.2389 | -1068.2 | -865.5 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 4.40 | 159.09 | -14.30 | 78.58 | 0.2524 | -706.0 | -517.7 | |
| 1.28 | 6.08 | 0.66 | 3.11 | 5.20 | 159.04 | -14.35 | 75.53 | 0.2560 | -1079.0 | -801.4 | |
| 0.00 | 2.48 | 0.00 | 1.27 | 4.40 | 158.78 | -14.61 | 78.81 | 0.2575 | -676.0 | -419.0 | |
| 0.00 | 0.60 | 0.00 | 0.31 | 4.90 | 158.59 | -14.80 | 77.05 | 0.2624 | -737.0 | -500.1 | |
| 1.28 | 3.00 | 0.66 | 1.54 | 5.14 | 158.52 | -14.87 | 76.22 | 0.2643 | -925.3 | -569.3 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 3.89 | 158.21 | -15.18 | 81.08 | 0.2657 | 680.0 | 517.3 | |
| 0.51 | 1.97 | 0.26 | 1.01 | 4.69 | 158.10 | -15.29 | 78.19 | 0.2697 | 870.7 | 654.2 | |
| 0.00 | 3.77 | 0.00 | 1.94 | 5.40 | 157.96 | -15.43 | 75.74 | 0.2745 | -742.0 | -683.4 | |
| 0.00 | 2.31 | 0.00 | 1.19 | 4.28 | 157.77 | -15.62 | 79.92 | 0.2739 | 146.0 | 210.9 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 4.89 | 157.26 | -16.13 | 78.05 | 0.2841 | 994.0 | 726.2 | |
| 1.20 | 2.57 | 0.62 | 1.33 | 5.07 | 157.20 | -16.19 | 77.48 | 0.2858 | 1026.8 | 833.0 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 5.72 | 156.84 | -16.55 | 75.55 | 0.2940 | 758.0 | 663.5 | |
| 3.00 | 4.54 | 1.55 | 2.35 | 5.93 | 156.80 | -16.59 | 74.89 | 0.2954 | 1082.2 | 869.4 | |
| 0.00 | 1.97 | 0.00 | 1.02 | 5.66 | 156.56 | -16.83 | 75.97 | 0.2983 | 917.0 | 759.6 | |
| 0.00 | 0.86 | 0.00 | 0.44 | 4.00 | 156.38 | -17.00 | 81.60 | 0.2962 | 769.0 | 715.9 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 5.33 | 156.29 | -17.10 | 77.23 | 0.3015 | 952.0 | 812.7 | |
| 0.00 | 2.65 | 0.00 | 1.38 | 4.80 | 156.15 | -17.24 | 79.07 | 0.3021 | 931.0 | 794.3 | |
| 0.00 | 3.34 | 0.00 | 1.74 | 4.35 | 156.00 | -17.38 | 80.60 | 0.3033 | 930.0 | 808.3 | |
| 0.00 | 0.86 | 0.00 | 0.45 | 4.65 | 155.90 | -17.48 | 79.69 | 0.3057 | 882.0 | 727.7 | |
| 1.88 | 3.25 | 0.98 | 1.69 | 4.53 | 155.69 | -17.70 | 80.19 | 0.3090 | 967.2 | 779.2 | |
| 0.00 | 1.71 | 0.00 | 0.89 | 4.47 | 155.44 | -17.95 | 80.51 | 0.3129 | 899.0 | 797.7 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 4.23 | 155.32 | -18.07 | 81.31 | 0.3143 | 802.0 | 695.9 | |
| 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. | |