SDO HMI 2014-12-01 03:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.36 | 248.22 | 63.33 | 280.65 | 3.31 | 162.66 | 63.98 | 273.27 | 0.8998 | -292.6 | -163.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.95 | 214.19 | 21.14 | 248.62 | 2.52 | 163.84 | 65.16 | 272.37 | 0.9092 | -545.4 | -204.2 | |
| 23.08 | -1.00 | 26.51 | -1.00 | 3.36 | 163.16 | 64.48 | 273.30 | 0.9042 | -566.6 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.87 | 4.26 | 162.53 | 63.85 | 274.31 | 0.8996 | -300.0 | -295.8 | |
| 1.37 | -1.00 | 1.52 | -1.00 | 3.82 | 162.13 | 63.45 | 273.83 | 0.8964 | -747.6 | 999999 | |
| 0.51 | -1.00 | 0.57 | -1.00 | 4.00 | 162.09 | 63.41 | 274.03 | 0.8961 | -553.5 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.62 | 3.91 | 160.07 | 61.39 | 273.97 | 0.8800 | -569.0 | -491.9 | |
| 0.00 | 0.60 | 0.00 | 0.61 | 3.65 | 159.48 | 60.80 | 273.69 | 0.8750 | -193.0 | -175.4 | |
| 4.19 | 6.24 | 4.26 | 6.36 | 4.48 | 159.53 | 60.85 | 274.64 | 0.8756 | 381.7 | 136.4 | |
| 0.00 | 0.60 | 0.00 | 0.58 | 4.48 | 157.97 | 59.29 | 274.67 | 0.8621 | -65.0 | -54.0 | |
| 0.00 | 0.51 | 0.00 | 0.49 | 8.03 | 157.29 | 58.61 | 278.85 | 0.8576 | 228.0 | 195.5 | |
| 0.00 | 1.20 | 0.00 | 1.12 | 5.36 | 156.55 | 57.87 | 275.76 | 0.8495 | 298.0 | 259.2 | |
| 0.34 | 1.37 | 0.32 | 1.27 | 5.57 | 156.41 | 57.73 | 276.02 | 0.8484 | 307.0 | 285.9 | |
| 1.37 | 3.33 | 1.26 | 3.08 | 5.75 | 156.10 | 57.43 | 276.25 | 0.8456 | 540.0 | 383.9 | |
| 7.78 | 16.07 | 7.06 | 14.58 | 6.29 | 155.53 | 56.85 | 276.93 | 0.8405 | 699.0 | 447.6 | |
| 0.77 | 2.74 | 0.69 | 2.45 | 4.07 | 155.05 | 56.38 | 274.29 | 0.8351 | 544.9 | 413.6 | |
| 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. | |