SDO HMI 2014-10-11 21:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.69 | 0.00 | 9.22 | 12.73 | 58.14 | 16.89 | 293.89 | 0.3115 | 243.5 | 161.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.40 | 0.00 | 0.77 | 11.66 | 66.98 | 25.73 | 284.10 | 0.4403 | -673.0 | -588.2 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 11.95 | 66.47 | 25.22 | 284.98 | 0.4334 | -755.0 | -624.1 | |
| 0.00 | 1.58 | 0.00 | 0.84 | 8.08 | 63.63 | 22.39 | 276.38 | 0.3811 | -677.0 | -449.7 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 18.26 | 60.79 | 19.55 | 304.22 | 0.3859 | -779.0 | -640.8 | |
| 0.00 | 1.58 | 0.00 | 0.84 | 17.29 | 60.42 | 19.17 | 302.45 | 0.3732 | -849.0 | -655.7 | |
| 0.00 | 0.79 | 0.00 | 0.41 | 12.74 | 59.70 | 18.45 | 291.33 | 0.3329 | 865.0 | 734.3 | |
| 0.00 | 1.23 | 0.00 | 0.63 | 13.59 | 55.40 | 14.16 | 299.25 | 0.2737 | 859.0 | 713.3 | |
| 0.00 | 1.40 | 0.00 | 0.72 | 13.77 | 55.29 | 14.04 | 300.04 | 0.2735 | 738.0 | 607.2 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 13.11 | 55.25 | 14.00 | 297.91 | 0.2679 | 898.0 | 740.5 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 13.83 | 54.47 | 13.22 | 301.64 | 0.2620 | 767.0 | 519.8 | |
| 0.00 | 1.84 | 0.00 | 0.93 | 10.90 | 53.63 | 12.38 | 292.14 | 0.2283 | 700.0 | 592.3 | |
| 0.00 | 1.75 | 0.00 | 0.89 | 11.05 | 53.48 | 12.23 | 293.01 | 0.2269 | 743.0 | 731.2 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 13.14 | 52.98 | 11.73 | 302.12 | 0.2349 | 811.0 | 564.5 | |
| 0.00 | 0.70 | 0.00 | 0.35 | 10.64 | 52.77 | 11.53 | 292.41 | 0.2134 | 761.0 | 499.1 | |
| 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. | |