SDO HMI 2011-10-29 11:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.64 | 82.01 | 21.98 | 97.93 | 12.77 | 300.52 | 65.84 | 281.94 | 0.9102 | 273.9 | 87.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.65 | 4.51 | 2.59 | 7.11 | 12.88 | 306.96 | 72.28 | 282.05 | 0.9508 | -498.6 | -316.2 | |
| 0.00 | 0.87 | 0.00 | 1.37 | 13.19 | 306.98 | 72.30 | 282.37 | 0.9509 | -315.0 | -273.9 | |
| 0.00 | 2.17 | 0.00 | 3.23 | 12.82 | 305.82 | 71.14 | 281.96 | 0.9447 | -430.0 | -285.9 | |
| 0.00 | 5.63 | 0.00 | 7.57 | 11.47 | 303.57 | 68.89 | 280.50 | 0.9314 | -642.0 | -405.6 | |
| 0.00 | 1.82 | 0.00 | 2.46 | 11.70 | 303.69 | 69.01 | 280.75 | 0.9322 | -277.0 | -202.4 | |
| 0.00 | 0.52 | 0.00 | 0.68 | 12.71 | 302.74 | 68.06 | 281.84 | 0.9261 | 101.0 | 48.5 | |
| 3.12 | 3.64 | 3.89 | 4.54 | 11.93 | 301.76 | 67.07 | 281.00 | 0.9197 | 337.2 | 247.3 | |
| 0.00 | 4.77 | 0.00 | 5.90 | 13.33 | 301.47 | 66.79 | 282.52 | 0.9178 | 252.0 | 79.2 | |
| 0.00 | 0.87 | 0.00 | 1.07 | 13.58 | 301.38 | 66.70 | 282.80 | 0.9172 | 363.0 | 284.9 | |
| 7.54 | 55.13 | 8.49 | 61.72 | 13.15 | 298.91 | 64.23 | 282.37 | 0.8996 | 516.2 | 248.7 | |
| 1.65 | -10.00 | 1.83 | -10.00 | 12.89 | 298.65 | 63.97 | 282.09 | 0.8976 | 730.4 | 999999 | |
| 4.68 | -10.00 | 5.18 | -10.00 | 12.63 | 298.46 | 63.78 | 281.80 | 0.8962 | 644.2 | 999999 | |
| 0.00 | 1.30 | 0.00 | 1.46 | 13.73 | 298.85 | 64.17 | 283.02 | 0.8993 | 416.0 | 359.8 | |
| 0.00 | 0.78 | 0.00 | 0.82 | 11.17 | 296.83 | 62.15 | 280.18 | 0.8833 | -58.0 | -63.0 | |
| 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. | |