| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.96 | 62.40 | 10.83 | 45.07 | 18.13 | 223.66 | 44.27 | 294.22 | 0.7298 | -297.5 | -247.8 | |
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back to the solar disc SDO HMI 2011-11-29 23:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.77 | 0.00 | 0.56 | 12.09 | 225.46 | 46.07 | 285.60 | 0.7335 | 653.0 | 558.3 | |
| 0.00 | 1.97 | 0.00 | 1.41 | 14.16 | 224.43 | 45.04 | 288.67 | 0.7265 | 517.0 | 439.7 | |
| 0.00 | 2.22 | 0.00 | 1.66 | 19.58 | 225.27 | 45.88 | 295.51 | 0.7518 | -473.0 | -385.8 | |
| 2.31 | 9.57 | 1.69 | 7.02 | 17.91 | 224.55 | 45.16 | 293.60 | 0.7387 | -714.0 | -462.6 | |
| 0.00 | 1.37 | 0.00 | 0.99 | 17.88 | 223.97 | 44.58 | 293.77 | 0.7323 | -703.0 | -590.8 | |
| 12.65 | 38.63 | 9.14 | 27.92 | 18.29 | 223.67 | 44.28 | 294.42 | 0.7304 | -806.1 | -347.3 | |
| 0.00 | 1.03 | 0.00 | 0.73 | 16.41 | 223.01 | 43.62 | 292.16 | 0.7169 | 413.0 | 348.6 | |
| 0.00 | 1.11 | 0.00 | 0.78 | 16.39 | 222.75 | 43.36 | 292.21 | 0.7138 | 240.0 | 278.2 | |
| 0.00 | 2.05 | 0.00 | 1.49 | 20.86 | 223.11 | 43.72 | 298.00 | 0.7338 | -670.0 | -551.1 | |
| 0.00 | 0.43 | 0.00 | 0.30 | 20.06 | 221.74 | 42.36 | 297.53 | 0.7160 | 492.0 | 432.8 | |
| 0.00 | 0.26 | 0.00 | 0.18 | 19.26 | 220.31 | 40.92 | 297.10 | 0.6970 | 545.0 | 446.7 | |
| 0.00 | 1.20 | 0.00 | 0.81 | 18.87 | 219.61 | 40.22 | 296.88 | 0.6875 | 539.0 | 500.9 | |
| 0.00 | 1.79 | 0.00 | 1.22 | 18.87 | 219.33 | 39.94 | 297.01 | 0.6842 | 526.0 | 437.1 | |
| 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. | |