SDO HMI 2011-11-12 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 |
| 67.09 | 418.74 | 35.84 | 223.71 | 16.14 | 64.30 | 18.07 | 307.29 | 0.3767 | -1143.3 | -415.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.46 | 14.16 | 66.18 | 19.95 | 300.37 | 0.3851 | -702.0 | -541.7 | |
| 1.03 | 399.30 | 0.55 | 213.33 | 16.06 | 64.96 | 18.73 | 306.21 | 0.3842 | -819.8 | -426.4 | |
| 62.88 | -2.00 | 33.60 | -2.00 | 16.04 | 64.44 | 18.21 | 306.90 | 0.3772 | -1435.5 | 999999 | |
| 1.46 | -2.00 | 0.78 | -2.00 | 16.05 | 63.79 | 17.56 | 307.87 | 0.3689 | -1194.2 | 999999 | |
| 1.38 | -2.00 | 0.73 | -2.00 | 16.33 | 63.66 | 17.42 | 308.69 | 0.3698 | -837.0 | 999999 | |
| 0.00 | 2.41 | 0.00 | 1.29 | 17.55 | 63.51 | 17.28 | 311.53 | 0.3800 | -956.0 | -782.7 | |
| 0.00 | 0.95 | 0.00 | 0.50 | 15.64 | 62.95 | 16.72 | 308.23 | 0.3542 | -809.0 | -673.0 | |
| 0.00 | 0.95 | 0.00 | 0.50 | 15.13 | 62.43 | 16.19 | 307.87 | 0.3426 | 690.0 | 483.5 | |
| 0.00 | 1.81 | 0.00 | 1.00 | 23.44 | 63.03 | 16.80 | 322.75 | 0.4399 | -790.0 | -561.3 | |
| 0.00 | 1.98 | 0.00 | 1.05 | 17.72 | 62.33 | 16.09 | 313.82 | 0.3676 | -828.0 | -714.3 | |
| 0.00 | 1.63 | 0.00 | 0.89 | 22.03 | 62.42 | 16.19 | 321.54 | 0.4173 | -721.0 | -479.6 | |
| 0.00 | 1.63 | 0.00 | 0.87 | 17.82 | 61.79 | 15.55 | 314.96 | 0.3624 | -768.0 | -560.1 | |
| 0.34 | 2.58 | 0.18 | 1.33 | 11.11 | 61.12 | 14.89 | 299.05 | 0.2897 | 967.0 | 806.2 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 24.17 | 60.90 | 14.67 | 327.32 | 0.4296 | -757.0 | -663.5 | |
| 0.00 | 3.01 | 0.00 | 1.59 | 18.53 | 59.43 | 13.20 | 320.90 | 0.3447 | 670.0 | 586.7 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 23.59 | 59.33 | 13.10 | 329.33 | 0.4089 | -641.0 | -525.7 | |
| 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. | |