SDO HMI 2011-11-15 12:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.11 | 143.19 | 83.23 | 338.03 | 19.52 | 87.98 | 78.00 | 289.40 | 0.9769 | -39.6 | -148.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.78 | 55.69 | 11.83 | 171.42 | 19.27 | 91.32 | 81.34 | 289.07 | 0.9881 | 457.8 | -76.5 | |
| 6.10 | -1.00 | 18.27 | -1.00 | 19.05 | 90.81 | 80.82 | 288.84 | 0.9868 | -454.0 | 999999 | |
| 0.69 | -1.00 | 2.06 | -1.00 | 19.77 | 90.80 | 80.82 | 289.58 | 0.9868 | -274.4 | 999999 | |
| 2.66 | 4.21 | 6.12 | 9.71 | 18.28 | 87.83 | 77.84 | 288.10 | 0.9776 | 147.9 | 83.8 | |
| 0.00 | 2.84 | 0.00 | 5.80 | 18.20 | 86.16 | 76.17 | 288.06 | 0.9713 | 236.0 | 106.5 | |
| 5.24 | 26.13 | 10.66 | 51.90 | 18.64 | 86.10 | 76.11 | 288.51 | 0.9711 | -332.9 | -220.9 | |
| 1.46 | -6.00 | 2.99 | -6.00 | 18.86 | 86.13 | 76.15 | 288.73 | 0.9713 | 312.4 | 999999 | |
| 0.00 | 0.95 | 0.00 | 1.82 | 18.52 | 85.29 | 75.30 | 288.41 | 0.9678 | 306.0 | 237.9 | |
| 3.09 | -6.00 | 6.15 | -6.00 | 19.22 | 85.72 | 75.73 | 289.12 | 0.9697 | -517.4 | 999999 | |
| 0.00 | 1.12 | 0.00 | 2.12 | 20.30 | 84.82 | 74.84 | 290.28 | 0.9662 | 0.0 | -85.8 | |
| 0.00 | 2.49 | 0.00 | 4.96 | 21.31 | 85.67 | 75.68 | 291.28 | 0.9699 | 37.0 | 18.6 | |
| 0.00 | 1.12 | 0.00 | 1.90 | 19.60 | 83.00 | 73.01 | 289.63 | 0.9579 | 517.0 | 464.0 | |
| 2.84 | 48.64 | 5.36 | 88.40 | 21.22 | 84.78 | 74.79 | 291.23 | 0.9662 | -425.5 | -352.0 | |
| 9.45 | -13.00 | 16.63 | -13.00 | 20.52 | 83.57 | 73.58 | 290.56 | 0.9608 | 416.1 | 999999 | |
| 1.80 | -13.00 | 3.16 | -13.00 | 20.80 | 83.49 | 73.50 | 290.87 | 0.9605 | -281.8 | 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. | |