| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.81 | 108.88 | 20.81 | 59.91 | -17.69 | 100.66 | 14.87 | 214.11 | 0.4370 | 44.2 | 37.5 | |
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back to the solar disc SDO HMI 2011-11-09 18:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.99 | 73.22 | 5.53 | 40.55 | -17.75 | 101.89 | 16.11 | 216.26 | 0.4486 | 990.7 | 416.1 | |
| 12.32 | -1.00 | 6.83 | -1.00 | -18.09 | 101.60 | 15.82 | 215.30 | 0.4502 | 1046.6 | 999999 | |
| 4.39 | -1.00 | 2.43 | -1.00 | -17.74 | 101.57 | 15.78 | 215.73 | 0.4456 | 1171.4 | 999999 | |
| 0.00 | 1.64 | 0.00 | 0.89 | -17.30 | 99.89 | 14.10 | 213.35 | 0.4250 | -847.0 | -596.6 | |
| 0.00 | 1.29 | 0.00 | 0.70 | -17.10 | 99.20 | 13.42 | 212.33 | 0.4164 | -854.0 | -669.4 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -17.00 | 99.00 | 13.22 | 212.08 | 0.4134 | -822.0 | -686.5 | |
| 0.00 | 1.72 | 0.00 | 0.94 | -17.16 | 98.86 | 13.07 | 211.59 | 0.4143 | -798.0 | -639.3 | |
| 0.43 | 1.81 | 0.23 | 0.98 | -17.19 | 98.60 | 12.82 | 211.06 | 0.4126 | -991.4 | -799.7 | |
| 3.79 | 11.89 | 2.06 | 6.47 | -17.47 | 98.56 | 12.77 | 210.60 | 0.4160 | -905.5 | -699.6 | |
| 0.00 | 1.98 | 0.00 | 1.08 | -17.95 | 98.59 | 12.81 | 210.06 | 0.4228 | -727.0 | -578.7 | |
| 0.00 | 1.72 | 0.00 | 0.94 | -18.14 | 98.51 | 12.73 | 209.67 | 0.4247 | -683.0 | -517.0 | |
| 1.38 | 1.55 | 0.75 | 0.84 | -17.06 | 98.37 | 12.58 | 210.77 | 0.4089 | -856.0 | -893.0 | |
| 0.00 | 2.50 | 0.00 | 1.36 | -17.73 | 98.39 | 12.60 | 209.94 | 0.4181 | -733.0 | -649.8 | |
| 1.72 | -9.00 | 0.94 | -9.00 | -17.41 | 98.27 | 12.48 | 210.12 | 0.4128 | -945.3 | 999999 | |
| 0.00 | 1.64 | 0.00 | 0.89 | -17.12 | 98.09 | 12.30 | 210.13 | 0.4074 | -962.0 | -872.8 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -16.70 | 98.03 | 12.24 | 210.55 | 0.4013 | -915.0 | -721.7 | |
| 3.79 | 5.94 | 2.04 | 3.20 | -16.42 | 97.85 | 12.07 | 210.57 | 0.3960 | -1056.8 | -874.5 | |
| 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. | |