SDO HMI 2011-11-15 14:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.38 | 138.42 | 87.25 | 363.13 | 19.48 | 88.24 | 79.35 | 289.34 | 0.9812 | -53.7 | -128.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.12 | 56.53 | 13.83 | 196.53 | 18.92 | 90.91 | 82.02 | 288.72 | 0.9898 | -415.5 | -59.0 | |
| 4.30 | -1.00 | 15.12 | -1.00 | 19.25 | 91.29 | 82.40 | 289.05 | 0.9907 | 466.8 | 999999 | |
| 2.58 | 3.87 | 6.42 | 9.65 | 18.35 | 87.79 | 78.90 | 288.15 | 0.9811 | 149.4 | 95.9 | |
| 0.00 | 2.41 | 0.00 | 5.31 | 18.20 | 86.16 | 77.27 | 288.04 | 0.9755 | 156.0 | 100.4 | |
| 2.58 | 24.23 | 5.64 | 51.35 | 18.71 | 86.05 | 77.16 | 288.56 | 0.9752 | -420.6 | -288.6 | |
| 2.15 | -5.00 | 4.60 | -5.00 | 19.10 | 85.79 | 76.90 | 288.96 | 0.9742 | -433.3 | 999999 | |
| 1.29 | -5.00 | 2.79 | -5.00 | 19.38 | 85.79 | 76.90 | 289.25 | 0.9743 | -489.3 | 999999 | |
| 0.00 | 2.49 | 0.00 | 5.42 | 20.26 | 85.90 | 77.01 | 290.15 | 0.9748 | -382.0 | -348.3 | |
| 0.00 | 0.52 | 0.00 | 0.94 | 19.60 | 83.14 | 74.25 | 289.57 | 0.9635 | 380.0 | 396.5 | |
| 3.01 | 48.37 | 6.08 | 93.93 | 20.88 | 84.81 | 75.92 | 290.83 | 0.9707 | -621.5 | -253.2 | |
| 2.49 | -10.00 | 5.06 | -10.00 | 21.26 | 84.87 | 75.98 | 291.21 | 0.9710 | -460.1 | 999999 | |
| 10.22 | -10.00 | 18.93 | -10.00 | 20.50 | 83.38 | 74.49 | 290.50 | 0.9648 | 423.4 | 999999 | |
| 4.64 | -10.00 | 8.78 | -10.00 | 20.74 | 83.71 | 74.82 | 290.73 | 0.9662 | -393.0 | 999999 | |
| 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. | |