SDO HMI 2011-10-29 14:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.58 | 48.08 | 10.09 | 24.74 | 14.81 | 244.90 | 11.87 | 312.47 | 0.2706 | -317.7 | -161.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.69 | 23.74 | 7.08 | 12.28 | 14.40 | 246.87 | 13.84 | 306.52 | 0.2895 | -1082.4 | -501.1 | |
| 0.00 | 1.73 | 0.00 | 0.90 | 15.52 | 246.66 | 13.62 | 310.04 | 0.2978 | -771.0 | -586.5 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 14.86 | 245.00 | 11.97 | 311.73 | 0.2698 | -846.0 | -609.1 | |
| 0.00 | 2.25 | 0.00 | 1.16 | 15.02 | 244.29 | 11.26 | 313.90 | 0.2628 | -820.0 | -713.9 | |
| 0.00 | 0.78 | 0.00 | 0.40 | 12.94 | 244.12 | 11.09 | 307.82 | 0.2384 | 855.0 | 697.8 | |
| 0.00 | 0.78 | 0.00 | 0.40 | 15.23 | 244.21 | 11.17 | 314.70 | 0.2642 | -708.0 | -565.9 | |
| 5.89 | 9.18 | 3.01 | 4.70 | 14.39 | 243.88 | 10.85 | 313.08 | 0.2507 | -1016.4 | -684.2 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 15.59 | 242.69 | 9.65 | 319.74 | 0.2511 | 680.0 | 537.8 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 16.96 | 242.16 | 9.12 | 324.69 | 0.2636 | 766.0 | 573.2 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 14.89 | 240.41 | 7.38 | 325.15 | 0.2182 | 902.0 | 710.8 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 17.14 | 239.81 | 6.77 | 332.53 | 0.2454 | 816.0 | 682.1 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 16.35 | 239.62 | 6.59 | 331.55 | 0.2322 | 1047.0 | 879.9 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 16.62 | 239.44 | 6.41 | 332.77 | 0.2349 | 954.0 | 772.8 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 16.29 | 239.28 | 6.24 | 332.69 | 0.2286 | 829.0 | 607.1 | |
| 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. | |