SDO HMI 2014-09-16 02:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.24 | 243.09 | 53.19 | 294.46 | 15.52 | 88.55 | 66.95 | 283.82 | 0.9148 | 488.5 | 228.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.80 | 0.00 | 1.04 | 16.87 | 90.29 | 68.69 | 285.32 | 0.9260 | 303.0 | 342.7 | |
| 28.43 | 166.51 | 34.70 | 202.44 | 14.87 | 88.70 | 67.10 | 283.11 | 0.9159 | 601.0 | 272.6 | |
| 0.00 | 0.80 | 0.00 | 1.03 | 17.01 | 90.14 | 68.54 | 285.48 | 0.9251 | 606.0 | 491.4 | |
| 0.00 | 1.24 | 0.00 | 1.59 | 17.19 | 89.94 | 68.34 | 285.67 | 0.9237 | 558.0 | 500.8 | |
| 0.00 | 0.98 | 0.00 | 1.12 | 12.84 | 86.93 | 65.32 | 280.82 | 0.9038 | -286.0 | -217.8 | |
| 2.84 | 27.72 | 3.53 | 34.41 | 16.81 | 89.14 | 67.54 | 285.25 | 0.9186 | -1.6 | 25.4 | |
| 0.00 | 1.24 | 0.00 | 1.50 | 17.07 | 88.26 | 66.66 | 285.52 | 0.9126 | 238.0 | 203.3 | |
| 0.00 | 2.84 | 0.00 | 3.54 | 18.57 | 89.18 | 67.57 | 287.17 | 0.9187 | -93.0 | -85.5 | |
| 0.00 | 1.24 | 0.00 | 1.55 | 18.91 | 89.29 | 67.68 | 287.53 | 0.9195 | -325.0 | -207.9 | |
| 1.42 | 23.10 | 1.68 | 27.41 | 17.55 | 87.89 | 66.29 | 286.05 | 0.9101 | 354.2 | 137.7 | |
| 4.71 | -10.00 | 5.52 | -10.00 | 17.33 | 87.65 | 66.05 | 285.80 | 0.9084 | 595.9 | 999999 | |
| 4.44 | 11.37 | 5.11 | 13.03 | 16.51 | 87.09 | 65.49 | 284.90 | 0.9045 | 464.4 | 450.9 | |
| 2.40 | 4.09 | 2.65 | 4.51 | 15.65 | 85.88 | 64.28 | 283.93 | 0.8957 | 517.1 | 394.1 | |
| 0.00 | 0.89 | 0.00 | 1.00 | 17.42 | 86.33 | 64.73 | 285.90 | 0.8990 | 457.0 | 366.6 | |
| 0.00 | 0.27 | 0.00 | 0.29 | 16.94 | 85.00 | 63.40 | 285.38 | 0.8890 | 444.0 | 399.0 | |
| 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. | |