SDO HMI 2014-12-11 11:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.03 | 270.31 | 31.76 | 171.43 | -3.98 | 1.11 | 38.58 | 264.17 | 0.6276 | 883.3 | 321.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.43 | 1.87 | 0.27 | 1.19 | -1.58 | 1.47 | 38.94 | 268.01 | 0.6309 | -770.8 | -658.8 | |
| 34.51 | 251.90 | 21.99 | 160.02 | -4.16 | 1.38 | 38.85 | 263.92 | 0.6315 | 1073.6 | 333.3 | |
| 0.26 | -2.00 | 0.16 | -2.00 | -3.57 | 1.20 | 38.67 | 264.84 | 0.6284 | 886.3 | 999999 | |
| 12.87 | -2.00 | 8.13 | -2.00 | -3.92 | 0.80 | 38.27 | 264.22 | 0.6233 | 1279.0 | 999999 | |
| 0.51 | 4.01 | 0.32 | 2.52 | -2.74 | 0.37 | 37.84 | 266.09 | 0.6165 | 887.7 | 705.5 | |
| 0.00 | 1.11 | 0.00 | 0.69 | -2.56 | 0.25 | 37.72 | 266.37 | 0.6147 | 621.0 | 492.4 | |
| 0.00 | 1.53 | 0.00 | 0.95 | -2.68 | 359.55 | 37.02 | 266.12 | 0.6050 | 376.0 | 324.7 | |
| 0.00 | 0.94 | 0.00 | 0.58 | -2.77 | 359.26 | 36.72 | 265.94 | 0.6010 | 664.0 | 560.0 | |
| 0.00 | 1.02 | 0.00 | 0.63 | -3.28 | 359.13 | 36.59 | 265.09 | 0.5996 | 577.0 | 509.5 | |
| 0.00 | 1.45 | 0.00 | 0.89 | -3.57 | 359.03 | 36.50 | 264.58 | 0.5985 | 456.0 | 597.9 | |
| 1.11 | 1.96 | 0.68 | 1.20 | -1.98 | 358.68 | 36.15 | 267.24 | 0.5924 | 751.4 | 616.1 | |
| 0.34 | 2.47 | 0.21 | 1.51 | -2.60 | 358.51 | 35.98 | 266.17 | 0.5905 | -661.0 | -506.2 | |
| 0.00 | 2.05 | 0.00 | 1.25 | -3.34 | 358.07 | 35.53 | 264.86 | 0.5848 | -747.0 | -587.6 | |
| 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. | |