SDO HMI 2014-01-15 17:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 82.02 | 388.82 | 43.25 | 205.16 | -16.30 | 12.47 | 16.67 | 233.13 | 0.3456 | 1077.3 | 408.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.72 | -14.91 | 13.36 | 17.56 | 237.93 | 0.3456 | -569.0 | -465.4 | |
| 33.23 | 225.56 | 17.62 | 119.62 | -16.56 | 13.35 | 17.55 | 233.87 | 0.3594 | 1321.2 | 417.5 | |
| 5.95 | -2.00 | 3.15 | -2.00 | -16.57 | 12.96 | 17.16 | 233.28 | 0.3544 | 1408.0 | 999999 | |
| 5.27 | -2.00 | 2.79 | -2.00 | -16.70 | 12.62 | 16.82 | 232.46 | 0.3511 | 1139.7 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -16.02 | 12.21 | 16.41 | 233.46 | 0.3394 | 226.0 | 161.0 | |
| 0.00 | 2.21 | 0.00 | 1.16 | -14.88 | 11.86 | 16.06 | 235.82 | 0.3247 | 688.0 | 600.2 | |
| 1.36 | 152.73 | 0.71 | 80.03 | -15.39 | 11.71 | 15.91 | 234.24 | 0.3272 | 1013.7 | 437.0 | |
| 36.21 | -7.00 | 18.98 | -7.00 | -15.88 | 11.53 | 15.73 | 232.70 | 0.3292 | 1328.9 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -14.38 | 11.29 | 15.49 | 236.25 | 0.3125 | -560.0 | -458.2 | |
| 0.00 | 1.53 | 0.00 | 0.81 | -18.97 | 11.51 | 15.71 | 225.56 | 0.3601 | 956.0 | 805.0 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -17.07 | 6.99 | 11.19 | 220.47 | 0.2872 | -821.0 | -652.3 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -17.63 | 6.08 | 10.28 | 216.88 | 0.2847 | -686.0 | -622.6 | |
| 0.00 | 0.93 | 0.00 | 0.48 | -19.14 | 4.34 | 8.54 | 209.11 | 0.2896 | -861.0 | -737.6 | |
| 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. | |