SDO HMI 2013-10-17 21:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.35 | 56.68 | 15.64 | 56.88 | -22.16 | 153.75 | 54.63 | 240.33 | 0.8685 | 279.9 | 160.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.81 | 35.32 | 11.69 | 38.28 | -22.43 | 156.48 | 57.36 | 241.15 | 0.8906 | 590.8 | 196.7 | |
| 0.00 | 1.48 | 0.00 | 1.58 | -22.55 | 155.96 | 56.84 | 240.84 | 0.8873 | 795.0 | 661.5 | |
| 1.40 | 9.07 | 1.23 | 7.97 | -21.30 | 148.93 | 49.81 | 239.41 | 0.8290 | 553.1 | 484.7 | |
| 0.78 | -3.00 | 0.69 | -3.00 | -21.37 | 148.62 | 49.49 | 239.19 | 0.8266 | 708.3 | 999999 | |
| 0.35 | -3.00 | 0.31 | -3.00 | -21.50 | 148.58 | 49.45 | 239.03 | 0.8268 | 595.8 | 999999 | |
| 0.00 | 1.22 | 0.00 | 1.05 | -20.92 | 147.97 | 48.85 | 239.40 | 0.8193 | -555.0 | -438.7 | |
| 0.96 | 2.18 | 0.84 | 1.92 | -22.32 | 148.41 | 49.29 | 238.05 | 0.8287 | 559.6 | 434.5 | |
| 1.05 | 4.36 | 0.88 | 3.68 | -20.67 | 147.23 | 48.11 | 239.35 | 0.8119 | -593.8 | -502.6 | |
| 0.00 | 0.61 | 0.00 | 0.51 | -22.34 | 146.14 | 47.02 | 236.94 | 0.8096 | -420.0 | -420.1 | |
| 0.00 | 0.44 | 0.00 | 0.34 | -22.32 | 142.27 | 43.15 | 234.91 | 0.7755 | -527.0 | -444.8 | |
| 0.00 | 0.61 | 0.00 | 0.49 | -24.65 | 142.19 | 43.07 | 232.25 | 0.7872 | -371.0 | -308.7 | |
| 0.00 | 0.87 | 0.00 | 0.67 | -23.26 | 140.83 | 41.70 | 233.00 | 0.7677 | -544.0 | -510.1 | |
| 0.00 | 0.52 | 0.00 | 0.39 | -21.42 | 139.99 | 40.87 | 234.60 | 0.7496 | -566.0 | -505.8 | |
| 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. | |