SDO HMI 2011-11-14 07:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.13 | 66.68 | 38.51 | 70.79 | 19.54 | 87.40 | 61.50 | 290.58 | 0.8863 | -224.0 | -172.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.29 | 29.08 | 1.46 | 32.35 | 19.40 | 89.35 | 63.44 | 290.17 | 0.9007 | 202.9 | -354.8 | |
| 16.60 | -1.00 | 18.44 | -1.00 | 19.30 | 88.85 | 62.95 | 290.11 | 0.8970 | -658.9 | 999999 | |
| 0.00 | 1.20 | 0.00 | 1.26 | 18.63 | 87.13 | 61.22 | 289.57 | 0.8835 | -547.0 | -481.2 | |
| 8.09 | 12.82 | 8.22 | 13.02 | 18.26 | 86.14 | 60.23 | 289.29 | 0.8754 | 548.2 | 192.6 | |
| 1.29 | 2.67 | 1.32 | 2.72 | 19.26 | 86.22 | 60.32 | 290.41 | 0.8771 | 291.3 | 303.0 | |
| 0.00 | 1.63 | 0.00 | 1.69 | 19.94 | 86.46 | 60.55 | 291.14 | 0.8797 | 262.0 | 216.2 | |
| 0.00 | 0.69 | 0.00 | 0.68 | 18.49 | 85.20 | 59.30 | 289.68 | 0.8681 | 376.0 | 280.2 | |
| 0.00 | 1.38 | 0.00 | 1.43 | 20.81 | 86.52 | 60.62 | 292.12 | 0.8812 | 75.0 | 59.0 | |
| 3.18 | 12.65 | 3.33 | 13.16 | 21.34 | 86.69 | 60.79 | 292.69 | 0.8831 | -600.9 | -489.2 | |
| 0.00 | 0.95 | 0.00 | 0.93 | 18.78 | 84.94 | 59.03 | 290.05 | 0.8662 | 284.0 | 292.1 | |
| 3.36 | -9.00 | 3.47 | -9.00 | 21.33 | 86.29 | 60.38 | 292.74 | 0.8800 | -702.3 | 999999 | |
| 2.32 | 2.75 | 2.27 | 2.69 | 19.74 | 84.57 | 58.67 | 291.20 | 0.8644 | 370.2 | 315.4 | |
| 0.00 | 0.86 | 0.00 | 0.86 | 20.87 | 85.22 | 59.31 | 292.39 | 0.8711 | 143.0 | 195.5 | |
| 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. | |