SDO HMI 2011-10-29 16:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.40 | 55.09 | 11.47 | 72.61 | 12.76 | 300.27 | 68.33 | 281.91 | 0.9270 | 106.7 | 167.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.73 | 3.38 | 3.22 | 6.29 | 12.87 | 307.14 | 75.21 | 282.08 | 0.9651 | -332.7 | -233.8 | |
| 0.00 | 0.95 | 0.00 | 1.47 | 11.42 | 303.78 | 71.85 | 280.50 | 0.9487 | -116.0 | -148.6 | |
| 0.00 | 1.73 | 0.00 | 2.68 | 11.60 | 303.79 | 71.86 | 280.69 | 0.9487 | -432.0 | -378.5 | |
| 0.00 | 1.21 | 0.00 | 1.72 | 11.68 | 301.95 | 70.02 | 280.74 | 0.9383 | -96.0 | -99.2 | |
| 0.00 | 0.69 | 0.00 | 0.97 | 11.48 | 301.75 | 69.82 | 280.53 | 0.9371 | -418.0 | -399.0 | |
| 0.00 | 1.82 | 0.00 | 2.55 | 11.94 | 301.74 | 69.81 | 281.02 | 0.9370 | 278.0 | 218.2 | |
| 0.00 | 4.94 | 0.00 | 6.86 | 13.44 | 301.60 | 69.67 | 282.63 | 0.9361 | -440.0 | 14.8 | |
| 0.00 | 0.69 | 0.00 | 0.86 | 10.97 | 298.82 | 66.89 | 279.95 | 0.9185 | 265.0 | 232.6 | |
| 1.04 | 38.81 | 1.32 | 48.13 | 12.79 | 299.34 | 67.41 | 281.93 | 0.9219 | 165.8 | 291.3 | |
| 0.52 | -9.00 | 0.65 | -9.00 | 13.05 | 299.09 | 67.16 | 282.22 | 0.9203 | 221.7 | 999999 | |
| 1.30 | -9.00 | 1.62 | -9.00 | 13.37 | 298.95 | 67.01 | 282.56 | 0.9193 | 481.9 | 999999 | |
| 1.04 | -9.00 | 1.27 | -9.00 | 12.52 | 298.49 | 66.55 | 281.64 | 0.9162 | 432.6 | 999999 | |
| 1.21 | -9.00 | 1.49 | -9.00 | 12.84 | 298.58 | 66.65 | 282.00 | 0.9168 | 615.4 | 999999 | |
| 1.56 | -9.00 | 1.90 | -9.00 | 12.67 | 298.41 | 66.48 | 281.81 | 0.9157 | 664.1 | 999999 | |
| 0.00 | 0.87 | 0.00 | 1.08 | 13.83 | 298.89 | 66.96 | 283.07 | 0.9190 | 235.0 | 265.7 | |
| 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. | |