SDO HMI 2014-09-09 10:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.17 | 63.78 | 9.46 | 39.72 | 9.58 | 147.30 | 37.66 | 276.33 | 0.6080 | -3.4 | -78.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.19 | 11.95 | 2.73 | 7.78 | 9.52 | 150.53 | 40.88 | 276.19 | 0.6516 | -750.1 | -560.2 | |
| 0.00 | 1.43 | 0.00 | 0.92 | 9.65 | 150.06 | 40.42 | 276.40 | 0.6455 | -654.0 | -550.4 | |
| 1.16 | 2.68 | 0.73 | 1.68 | 9.99 | 148.08 | 38.44 | 276.97 | 0.6190 | -674.5 | -518.4 | |
| 0.00 | 1.25 | 0.00 | 0.78 | 9.55 | 147.90 | 38.26 | 276.26 | 0.6165 | -367.0 | -381.0 | |
| 0.00 | 1.52 | 0.00 | 0.95 | 10.01 | 147.77 | 38.13 | 277.02 | 0.6148 | -587.0 | -494.0 | |
| 1.61 | 12.84 | 1.00 | 8.02 | 9.97 | 147.53 | 37.89 | 276.96 | 0.6115 | -964.8 | -720.1 | |
| 0.00 | 1.78 | 0.00 | 1.11 | 9.36 | 147.14 | 37.49 | 275.96 | 0.6061 | 618.0 | 454.7 | |
| 1.25 | 2.68 | 0.77 | 1.66 | 9.02 | 146.87 | 37.22 | 275.39 | 0.6023 | -789.0 | -645.4 | |
| 0.00 | 1.34 | 0.00 | 0.83 | 9.76 | 146.77 | 37.12 | 276.62 | 0.6010 | -123.0 | -107.3 | |
| 0.00 | 3.39 | 0.00 | 2.08 | 9.32 | 146.10 | 36.45 | 275.90 | 0.5916 | 612.0 | 521.3 | |
| 1.25 | 19.62 | 0.76 | 11.91 | 9.61 | 145.49 | 35.84 | 276.41 | 0.5831 | 638.4 | 628.0 | |
| 5.71 | -11.00 | 3.47 | -11.00 | 9.32 | 145.30 | 35.65 | 275.91 | 0.5805 | 916.4 | 999999 | |
| 0.00 | 3.30 | 0.00 | 2.00 | 9.79 | 145.13 | 35.48 | 276.73 | 0.5782 | 892.0 | 764.3 | |
| 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. | |