SDO HMI 2011-10-29 13:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.77 | 23.75 | 3.46 | 16.20 | 17.15 | 275.83 | 42.24 | 290.37 | 0.6860 | 219.8 | 314.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.26 | 0.00 | 0.24 | 13.05 | 291.68 | 58.10 | 282.50 | 0.8492 | -316.0 | -314.7 | |
| 0.00 | 1.13 | 0.00 | 0.81 | 15.48 | 279.68 | 46.09 | 286.97 | 0.7282 | 217.0 | 312.8 | |
| 4.77 | 5.29 | 3.46 | 3.84 | 16.54 | 279.95 | 46.37 | 288.34 | 0.7333 | -656.5 | -497.0 | |
| 0.00 | 2.17 | 0.00 | 1.53 | 16.75 | 278.36 | 44.78 | 288.99 | 0.7157 | -511.0 | -446.2 | |
| 0.00 | 1.04 | 0.00 | 0.70 | 12.35 | 275.91 | 42.33 | 283.22 | 0.6780 | 560.0 | 501.8 | |
| 0.00 | 1.30 | 0.00 | 0.90 | 16.93 | 276.77 | 43.18 | 289.64 | 0.6975 | 655.0 | 483.7 | |
| 0.00 | 1.39 | 0.00 | 0.95 | 17.25 | 276.52 | 42.93 | 290.16 | 0.6953 | 453.0 | 372.1 | |
| 0.00 | 1.39 | 0.00 | 0.95 | 17.63 | 276.37 | 42.79 | 290.73 | 0.6946 | 688.0 | 556.8 | |
| 0.00 | 1.47 | 0.00 | 1.01 | 21.40 | 275.02 | 41.44 | 296.48 | 0.6907 | 489.0 | 343.9 | |
| 0.00 | 1.30 | 0.00 | 0.88 | 22.40 | 274.44 | 40.85 | 298.11 | 0.6880 | 543.0 | 464.3 | |
| 0.00 | 0.95 | 0.00 | 0.61 | 16.40 | 271.50 | 37.92 | 290.47 | 0.6315 | 673.0 | 554.1 | |
| 0.00 | 1.21 | 0.00 | 0.77 | 17.33 | 271.37 | 37.78 | 291.95 | 0.6328 | 767.0 | 589.5 | |
| 0.00 | 2.08 | 0.00 | 1.32 | 19.20 | 270.30 | 36.71 | 295.25 | 0.6265 | 691.0 | 530.0 | |
| 0.00 | 1.21 | 0.00 | 0.76 | 16.95 | 269.71 | 36.13 | 292.00 | 0.6106 | 532.0 | 419.1 | |
| 0.00 | 1.56 | 0.00 | 0.93 | 14.02 | 266.52 | 32.94 | 288.38 | 0.5581 | 669.0 | 498.3 | |
| 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. | |