SDO HMI 2011-10-25 18:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.77 | 164.75 | 30.23 | 138.25 | -21.63 | 331.34 | 47.77 | 238.45 | 0.8097 | -412.5 | -315.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.56 | 0.00 | 1.43 | -17.81 | 336.91 | 53.33 | 245.10 | 0.8441 | 618.0 | 502.2 | |
| 4.34 | 10.59 | 4.05 | 9.91 | -19.01 | 337.14 | 53.56 | 243.83 | 0.8496 | 684.2 | 504.6 | |
| 0.00 | 0.43 | 0.00 | 0.40 | -19.33 | 337.02 | 53.44 | 243.44 | 0.8495 | 488.0 | 506.8 | |
| 0.00 | 0.87 | 0.00 | 0.81 | -19.44 | 336.86 | 53.29 | 243.25 | 0.8486 | 401.0 | 394.6 | |
| 1.13 | 1.56 | 1.04 | 1.43 | -19.06 | 336.47 | 52.89 | 243.53 | 0.8442 | 592.4 | 503.0 | |
| 0.00 | 0.95 | 0.00 | 0.89 | -19.60 | 336.72 | 53.15 | 243.03 | 0.8479 | 523.0 | 417.8 | |
| 0.00 | 2.17 | 0.00 | 1.97 | -19.16 | 336.04 | 52.47 | 243.26 | 0.8409 | 604.0 | 588.0 | |
| 0.00 | 0.78 | 0.00 | 0.69 | -20.29 | 334.61 | 51.03 | 241.43 | 0.8325 | -300.0 | -238.8 | |
| 0.00 | 0.69 | 0.00 | 0.59 | -21.72 | 331.60 | 48.02 | 238.51 | 0.8121 | -441.0 | -382.4 | |
| 5.82 | 19.53 | 4.84 | 16.24 | -21.35 | 331.00 | 47.43 | 238.65 | 0.8054 | -691.0 | -299.7 | |
| 2.08 | 123.71 | 1.74 | 102.32 | -21.78 | 330.95 | 47.37 | 238.14 | 0.8067 | -487.4 | -432.9 | |
| 0.00 | 1.91 | 0.00 | 1.57 | -21.06 | 330.55 | 46.97 | 238.77 | 0.8001 | -526.0 | -431.5 | |
| 13.72 | -11.00 | 11.41 | -11.00 | -22.28 | 330.55 | 46.98 | 237.38 | 0.8055 | -731.2 | 999999 | |
| 8.68 | -11.00 | 7.15 | -11.00 | -21.96 | 330.22 | 46.65 | 237.58 | 0.8012 | -1117.6 | 999999 | |
| 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. | |