| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.83 | 269.58 | 27.64 | 187.32 | -18.47 | 352.24 | 41.78 | 244.42 | 0.7029 | 849.5 | 314.1 | |
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back to the solar disc SDO HMI 2011-12-17 08:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.04 | 0.00 | 1.48 | -19.06 | 354.74 | 44.29 | 244.65 | 0.7327 | -752.0 | -644.2 | |
| 0.00 | 2.21 | 0.00 | 1.58 | -18.44 | 354.11 | 43.65 | 245.21 | 0.7236 | -613.0 | -555.9 | |
| 0.00 | 1.19 | 0.00 | 0.85 | -18.97 | 354.06 | 43.61 | 244.50 | 0.7250 | 137.0 | 172.0 | |
| 0.00 | 1.02 | 0.00 | 0.72 | -18.89 | 353.48 | 43.02 | 244.38 | 0.7183 | 524.0 | 345.2 | |
| 2.30 | 250.27 | 1.62 | 173.86 | -19.21 | 352.81 | 42.35 | 243.68 | 0.7122 | 526.7 | 326.1 | |
| 36.17 | -5.00 | 25.08 | -5.00 | -18.34 | 352.21 | 41.75 | 244.59 | 0.7021 | 1152.4 | 999999 | |
| 0.00 | 1.19 | 0.00 | 0.84 | -19.83 | 352.59 | 42.13 | 242.75 | 0.7122 | -560.0 | -395.9 | |
| 0.00 | 0.94 | 0.00 | 0.64 | -19.91 | 351.15 | 40.69 | 241.99 | 0.6967 | 418.0 | 376.6 | |
| 0.00 | 0.68 | 0.00 | 0.47 | -19.79 | 350.98 | 40.53 | 242.08 | 0.6943 | 478.0 | 491.6 | |
| 0.00 | 3.49 | 0.00 | 2.40 | -20.19 | 351.03 | 40.57 | 241.55 | 0.6966 | 658.0 | 592.7 | |
| 0.00 | 1.53 | 0.00 | 1.05 | -19.73 | 350.76 | 40.30 | 242.06 | 0.6916 | 708.0 | 588.3 | |
| 1.36 | 2.38 | 0.94 | 1.64 | -20.48 | 350.95 | 40.49 | 241.14 | 0.6970 | 434.6 | 283.4 | |
| 0.00 | 1.02 | 0.00 | 0.69 | -18.03 | 350.23 | 39.77 | 244.16 | 0.6782 | 838.0 | 662.8 | |
| 0.00 | 1.62 | 0.00 | 1.10 | -19.73 | 350.39 | 39.93 | 241.87 | 0.6875 | 824.0 | 705.4 | |
| 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. | |