| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.96 | 259.53 | 59.70 | 267.17 | 17.71 | 61.02 | -61.01 | 71.87 | 0.8765 | -214.1 | -127.5 | |
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back to the solar disc SDO HMI 2011-11-07 00:58:59 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.21 | 0.00 | 1.15 | 17.92 | 63.88 | -58.14 | 71.30 | 0.8553 | -371.0 | -255.8 | |
| 1.64 | 183.84 | 1.56 | 174.44 | 17.11 | 63.82 | -58.21 | 72.25 | 0.8550 | -513.1 | -310.9 | |
| 29.78 | -2.00 | 28.21 | -2.00 | 16.71 | 63.84 | -58.19 | 72.71 | 0.8545 | -811.0 | 999999 | |
| 3.80 | -2.00 | 3.69 | -2.00 | 16.66 | 62.91 | -59.12 | 72.88 | 0.8625 | -370.2 | 999999 | |
| 1.12 | -2.00 | 1.10 | -2.00 | 16.92 | 62.59 | -59.44 | 72.61 | 0.8653 | -120.3 | 999999 | |
| 4.83 | 6.39 | 4.88 | 6.45 | 17.39 | 61.65 | -60.38 | 72.17 | 0.8735 | -452.9 | -266.1 | |
| 0.00 | 2.50 | 0.00 | 2.53 | 17.05 | 61.64 | -60.38 | 72.56 | 0.8732 | 262.0 | 127.0 | |
| 0.00 | 2.07 | 0.00 | 2.13 | 17.26 | 61.01 | -61.01 | 72.38 | 0.8785 | 420.0 | 304.0 | |
| 0.00 | 3.19 | 0.00 | 3.32 | 17.18 | 60.67 | -61.36 | 72.50 | 0.8811 | 162.0 | 68.8 | |
| 0.00 | 1.38 | 0.00 | 1.52 | 17.38 | 58.79 | -63.24 | 72.45 | 0.8956 | 439.0 | 369.7 | |
| 1.55 | 30.81 | 1.91 | 38.71 | 19.83 | 55.92 | -66.11 | 69.99 | 0.9171 | 689.1 | 422.2 | |
| 0.00 | 0.78 | 0.00 | 1.01 | 21.14 | 54.60 | -67.43 | 68.68 | 0.9261 | 370.0 | 314.3 | |
| 0.00 | 1.47 | 0.00 | 1.82 | 19.69 | 55.64 | -66.39 | 70.17 | 0.9188 | 574.0 | 515.6 | |
| 8.20 | -11.00 | 10.39 | -11.00 | 20.01 | 55.13 | -66.90 | 69.86 | 0.9222 | 616.5 | 999999 | |
| 0.00 | 0.86 | 0.00 | 1.11 | 19.98 | 54.66 | -67.37 | 69.93 | 0.9252 | 170.0 | 183.1 | |
| 6.04 | 24.43 | 7.96 | 32.20 | 20.14 | 54.18 | -67.85 | 69.79 | 0.9282 | 341.8 | 134.4 | |
| 0.00 | 0.60 | 0.00 | 0.78 | 19.47 | 54.60 | -67.43 | 70.48 | 0.9253 | 212.0 | 167.3 | |
| 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. | |