SDO HMI 2014-12-02 06:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.87 | 128.14 | 20.09 | 73.68 | -19.20 | 107.40 | 23.54 | 227.85 | 0.5102 | 41.1 | -60.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.33 | 7.43 | 1.98 | 4.43 | -19.65 | 111.22 | 27.36 | 231.27 | 0.5569 | 893.5 | 627.5 | |
| 0.00 | 0.77 | 0.00 | 0.46 | -19.96 | 111.28 | 27.42 | 230.86 | 0.5602 | 553.0 | 455.1 | |
| 0.43 | 1.79 | 0.25 | 1.07 | -19.83 | 110.79 | 26.93 | 230.59 | 0.5537 | 872.0 | 755.6 | |
| 0.00 | 1.37 | 0.00 | 0.81 | -19.52 | 110.52 | 26.66 | 230.80 | 0.5480 | 763.0 | 525.7 | |
| 0.00 | 2.14 | 0.00 | 1.26 | -19.67 | 110.20 | 26.34 | 230.25 | 0.5456 | 883.0 | 707.5 | |
| 0.00 | 2.91 | 0.00 | 1.71 | -19.42 | 109.88 | 26.02 | 230.30 | 0.5398 | 974.0 | 760.0 | |
| 0.60 | 24.27 | 0.35 | 14.12 | -19.13 | 109.72 | 25.86 | 230.58 | 0.5356 | 659.7 | 669.4 | |
| 0.94 | -7.00 | 0.55 | -7.00 | -18.82 | 109.39 | 25.53 | 230.73 | 0.5291 | 943.4 | 999999 | |
| 1.03 | -7.00 | 0.60 | -7.00 | -19.04 | 109.36 | 25.50 | 230.36 | 0.5306 | 968.7 | 999999 | |
| 7.86 | -7.00 | 4.56 | -7.00 | -18.66 | 109.06 | 25.20 | 230.63 | 0.5239 | 1014.9 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.35 | -20.17 | 109.27 | 25.41 | 228.55 | 0.5396 | 819.0 | 607.6 | |
| 0.00 | 1.28 | 0.00 | 0.75 | -20.36 | 108.82 | 24.96 | 227.79 | 0.5362 | 770.0 | 598.5 | |
| 0.68 | 1.97 | 0.39 | 1.13 | -18.43 | 108.47 | 24.61 | 230.36 | 0.5152 | 972.1 | 844.1 | |
| 2.82 | 15.30 | 1.63 | 8.82 | -18.78 | 108.39 | 24.53 | 229.72 | 0.5172 | -677.2 | -335.7 | |
| 0.00 | 1.20 | 0.00 | 0.69 | -19.06 | 108.36 | 24.50 | 229.26 | 0.5195 | 173.0 | 202.6 | |
| 0.26 | -14.00 | 0.15 | -14.00 | -18.71 | 108.24 | 24.38 | 229.66 | 0.5150 | -899.0 | 999999 | |
| 3.33 | -14.00 | 1.92 | -14.00 | -18.65 | 107.99 | 24.13 | 229.49 | 0.5116 | -621.5 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -18.46 | 107.86 | 24.00 | 229.64 | 0.5084 | 166.0 | 267.0 | |
| 0.00 | 1.97 | 0.00 | 1.14 | -20.32 | 108.08 | 24.22 | 227.04 | 0.5279 | 807.0 | 534.7 | |
| 0.00 | 2.14 | 0.00 | 1.22 | -18.36 | 107.50 | 23.64 | 229.39 | 0.5034 | 920.0 | 790.9 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -17.30 | 107.08 | 23.23 | 230.65 | 0.4889 | -526.0 | -489.2 | |
| 0.00 | 2.91 | 0.00 | 1.64 | -17.27 | 106.91 | 23.05 | 230.50 | 0.4866 | -1024.0 | -804.1 | |
| 0.00 | 0.77 | 0.00 | 0.44 | -18.82 | 106.08 | 22.22 | 226.98 | 0.4916 | -658.0 | -577.4 | |
| 0.00 | 2.91 | 0.00 | 1.65 | -18.73 | 105.86 | 22.00 | 226.86 | 0.4882 | -792.0 | -688.4 | |
| 0.00 | 1.97 | 0.00 | 1.12 | -19.26 | 105.60 | 21.74 | 225.70 | 0.4906 | -731.0 | -686.5 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -18.98 | 105.49 | 21.63 | 226.01 | 0.4866 | -772.0 | -643.9 | |
| 13.59 | 51.53 | 7.71 | 29.22 | -19.57 | 105.24 | 21.38 | 224.76 | 0.4898 | -1060.1 | -508.9 | |
| 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. | |