SDO HMI 2011-10-04 05:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.77 | 319.72 | 35.98 | 257.86 | 23.04 | 156.26 | -51.47 | 65.83 | 0.7912 | -682.6 | -254.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.72 | 25.98 | 156.14 | -51.59 | 62.21 | 0.7985 | -426.0 | -314.3 | |
| 0.00 | 1.06 | 0.00 | 0.87 | 25.90 | 155.98 | -51.76 | 62.35 | 0.7998 | -371.0 | -279.6 | |
| 0.00 | 1.32 | 0.00 | 1.07 | 24.90 | 156.36 | -51.37 | 63.49 | 0.7940 | 285.0 | 224.5 | |
| 0.00 | 0.79 | 0.00 | 0.65 | 25.30 | 156.13 | -51.60 | 63.05 | 0.7971 | -487.0 | -489.1 | |
| 11.52 | 251.00 | 9.15 | 200.59 | 22.52 | 156.93 | -50.80 | 66.35 | 0.7838 | -1009.6 | -297.3 | |
| 24.37 | -5.00 | 19.55 | -5.00 | 22.96 | 156.50 | -51.23 | 65.88 | 0.7889 | -883.3 | 999999 | |
| 0.26 | 57.10 | 0.22 | 47.48 | 24.21 | 155.48 | -52.25 | 64.53 | 0.8010 | -803.0 | -188.0 | |
| 1.58 | -5.00 | 1.26 | -5.00 | 22.14 | 156.61 | -51.12 | 66.89 | 0.7863 | -697.8 | 999999 | |
| 4.40 | -7.00 | 3.64 | -7.00 | 24.06 | 155.19 | -52.54 | 64.78 | 0.8034 | -885.2 | 999999 | |
| 1.23 | -5.00 | 0.99 | -5.00 | 22.38 | 156.12 | -51.61 | 66.68 | 0.7915 | -244.7 | 999999 | |
| 1.41 | -7.00 | 1.17 | -7.00 | 23.90 | 154.85 | -52.89 | 65.04 | 0.8063 | -627.6 | 999999 | |
| 0.00 | 2.73 | 0.00 | 2.22 | 20.08 | 155.38 | -52.35 | 69.69 | 0.7952 | 629.0 | 523.9 | |
| 0.00 | 1.14 | 0.00 | 0.94 | 20.82 | 154.86 | -52.88 | 68.84 | 0.8014 | -92.0 | -130.1 | |
| 0.00 | 1.85 | 0.00 | 1.62 | 23.73 | 152.54 | -55.19 | 65.67 | 0.8271 | 630.0 | 493.8 | |
| 0.00 | 0.97 | 0.00 | 0.85 | 23.26 | 152.37 | -55.36 | 66.26 | 0.8280 | 562.0 | 395.9 | |
| 0.00 | 0.88 | 0.00 | 0.85 | 26.90 | 148.86 | -58.87 | 62.55 | 0.8623 | 447.0 | 362.6 | |
| 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. | |