SDO HMI 2014-09-02 17:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.70 | 40.77 | 9.07 | 29.47 | -17.74 | 158.22 | -40.02 | 122.75 | 0.7304 | 140.0 | 37.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.82 | 21.55 | 7.69 | 15.32 | -17.57 | 159.18 | -39.06 | 123.15 | 0.7199 | 701.8 | 508.5 | |
| 0.54 | 2.41 | 0.38 | 1.72 | -17.14 | 158.84 | -39.40 | 122.40 | 0.7207 | 510.5 | 434.2 | |
| 0.00 | 1.07 | 0.00 | 0.77 | -18.09 | 158.55 | -39.70 | 123.36 | 0.7292 | -195.0 | -178.8 | |
| 0.00 | 1.61 | 0.00 | 1.14 | -16.38 | 158.87 | -39.38 | 121.49 | 0.7161 | 623.0 | 531.2 | |
| 0.00 | 0.89 | 0.00 | 0.65 | -17.89 | 158.19 | -40.06 | 122.89 | 0.7317 | -256.0 | -217.0 | |
| 0.00 | 1.34 | 0.00 | 0.98 | -18.31 | 157.90 | -40.34 | 123.22 | 0.7369 | -240.0 | -222.1 | |
| 0.00 | 0.63 | 0.00 | 0.46 | -18.51 | 157.84 | -40.40 | 123.42 | 0.7387 | -513.0 | -403.6 | |
| 0.00 | 1.25 | 0.00 | 0.93 | -18.39 | 156.61 | -41.63 | 122.52 | 0.7500 | -723.0 | -583.1 | |
| 0.00 | 1.25 | 0.00 | 0.94 | -18.90 | 156.41 | -41.84 | 123.00 | 0.7547 | -595.0 | -449.9 | |
| 0.00 | 3.67 | 0.00 | 2.75 | -18.53 | 156.43 | -41.81 | 122.59 | 0.7524 | -632.0 | -537.4 | |
| 0.80 | 4.38 | 0.60 | 3.28 | -18.18 | 156.28 | -41.96 | 122.08 | 0.7520 | -806.2 | -626.9 | |
| 0.54 | -11.00 | 0.40 | -11.00 | -18.10 | 156.09 | -42.15 | 121.87 | 0.7534 | -608.8 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.53 | -15.60 | 155.42 | -42.82 | 118.49 | 0.7472 | 575.0 | 477.4 | |
| 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. | |