SDO HMI 2011-11-13 18:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.68 | 82.02 | 11.98 | 58.35 | 8.29 | 347.27 | -45.78 | 81.41 | 0.7194 | 150.0 | 81.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.46 | 0.00 | 1.01 | 8.70 | 349.00 | -44.04 | 80.65 | 0.6988 | -559.0 | -445.6 | |
| 2.15 | 39.98 | 1.49 | 27.93 | 7.75 | 348.55 | -44.50 | 82.04 | 0.7036 | 580.2 | 47.0 | |
| 3.53 | -2.00 | 2.47 | -2.00 | 8.19 | 348.19 | -44.86 | 81.46 | 0.7083 | -440.0 | 999999 | |
| 0.00 | 6.96 | 0.00 | 4.92 | 7.84 | 347.56 | -45.49 | 82.01 | 0.7157 | -738.0 | -464.9 | |
| 1.03 | 6.19 | 0.74 | 4.41 | 9.47 | 347.22 | -45.83 | 79.77 | 0.7213 | 652.7 | 640.0 | |
| 0.00 | 1.20 | 0.00 | 0.87 | 8.99 | 346.47 | -46.58 | 80.51 | 0.7297 | 588.0 | 486.8 | |
| 0.00 | 1.38 | 0.00 | 0.99 | 7.32 | 346.59 | -46.45 | 82.80 | 0.7270 | -548.0 | -407.1 | |
| 0.00 | 1.20 | 0.00 | 0.87 | 7.43 | 346.36 | -46.69 | 82.66 | 0.7298 | -442.0 | -273.1 | |
| 1.46 | 19.52 | 1.06 | 14.23 | 8.74 | 346.07 | -46.97 | 80.90 | 0.7341 | 506.6 | 417.8 | |
| 4.21 | -9.00 | 3.07 | -9.00 | 8.52 | 345.84 | -47.20 | 81.22 | 0.7366 | 757.4 | 999999 | |
| 3.27 | -9.00 | 2.39 | -9.00 | 8.12 | 345.73 | -47.32 | 81.76 | 0.7377 | 814.4 | 999999 | |
| 1.03 | 1.46 | 0.76 | 1.08 | 9.19 | 345.33 | -47.72 | 80.36 | 0.7432 | -600.8 | -615.4 | |
| 0.00 | 0.95 | 0.00 | 0.70 | 8.73 | 345.05 | -48.00 | 81.01 | 0.7460 | -697.0 | -546.6 | |
| 0.00 | 1.72 | 0.00 | 1.34 | 9.83 | 342.62 | -50.43 | 79.77 | 0.7741 | 630.0 | 449.2 | |
| 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. | |