SDO HMI 2014-01-12 19:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 82.58 | 479.21 | 44.65 | 259.47 | -16.46 | 13.36 | -20.83 | 122.32 | 0.4051 | 1071.7 | 394.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.02 | 0.00 | 0.53 | -13.78 | 19.83 | -14.37 | 124.73 | 0.2945 | 877.0 | 754.5 | |
| 1.19 | 3.14 | 0.63 | 1.65 | -14.47 | 17.03 | -17.16 | 122.19 | 0.3392 | 1149.5 | 881.8 | |
| 0.00 | 1.78 | 0.00 | 0.95 | -14.71 | 15.44 | -18.75 | 120.68 | 0.3632 | -849.0 | -661.2 | |
| 50.55 | 462.32 | 27.26 | 250.07 | -16.54 | 13.99 | -20.20 | 123.16 | 0.3972 | 1396.4 | 419.0 | |
| 6.63 | -4.00 | 3.60 | -4.00 | -16.66 | 12.99 | -21.21 | 122.28 | 0.4117 | 1234.5 | 999999 | |
| 0.00 | 1.61 | 0.00 | 0.87 | -15.82 | 13.06 | -21.14 | 120.51 | 0.4046 | 253.0 | 313.2 | |
| 0.00 | 1.53 | 0.00 | 0.83 | -15.12 | 12.97 | -21.23 | 118.86 | 0.4009 | 704.0 | 567.4 | |
| 24.21 | -4.00 | 13.16 | -4.00 | -16.29 | 12.57 | -21.62 | 121.02 | 0.4146 | 1298.3 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.58 | -16.19 | 6.71 | -27.49 | 115.79 | 0.4944 | -819.0 | -612.1 | |
| 0.00 | 2.55 | 0.00 | 1.49 | -18.98 | 4.71 | -29.49 | 119.42 | 0.5366 | -675.0 | -699.4 | |
| 0.00 | 2.12 | 0.00 | 1.26 | -18.26 | 3.44 | -30.76 | 117.35 | 0.5489 | -777.0 | -657.3 | |
| 0.00 | 1.10 | 0.00 | 0.65 | -18.59 | 3.38 | -30.82 | 117.88 | 0.5516 | -716.0 | -634.9 | |
| 0.00 | 1.02 | 0.00 | 0.59 | -12.46 | 3.16 | -31.04 | 106.84 | 0.5282 | -821.0 | -671.9 | |
| 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. | |