| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.87 | 165.19 | 18.44 | 84.83 | 13.58 | 291.52 | 14.18 | 295.90 | 0.2661 | -639.9 | -425.6 | |
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back to the solar disc SDO HMI 2011-09-01 16:59:08 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.34 | 0.00 | 0.70 | 15.91 | 294.51 | 17.17 | 298.94 | 0.3258 | -736.0 | -579.9 | |
| 6.80 | 150.27 | 3.50 | 77.20 | 13.22 | 291.94 | 14.60 | 293.94 | 0.2697 | -1128.8 | -539.3 | |
| 1.70 | -2.00 | 0.87 | -2.00 | 12.97 | 291.92 | 14.58 | 293.11 | 0.2680 | -911.9 | 999999 | |
| 7.51 | -2.00 | 3.87 | -2.00 | 14.01 | 291.83 | 14.49 | 296.81 | 0.2732 | -1078.2 | 999999 | |
| 19.86 | -2.00 | 10.20 | -2.00 | 13.47 | 291.63 | 14.29 | 295.24 | 0.2666 | -1260.3 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.55 | 13.61 | 290.97 | 13.63 | 296.72 | 0.2575 | -884.0 | -740.8 | |
| 0.00 | 4.29 | 0.00 | 2.19 | 11.61 | 290.60 | 13.27 | 289.69 | 0.2398 | 730.0 | 642.9 | |
| 0.00 | 1.43 | 0.00 | 0.73 | 14.53 | 288.46 | 11.12 | 304.85 | 0.2286 | 789.0 | 659.6 | |
| 0.00 | 1.07 | 0.00 | 0.54 | 13.59 | 288.07 | 10.73 | 302.14 | 0.2147 | 880.0 | 673.8 | |
| 0.00 | 1.25 | 0.00 | 0.64 | 15.26 | 287.26 | 9.92 | 310.55 | 0.2197 | 802.0 | 656.1 | |
| 0.00 | 1.25 | 0.00 | 0.64 | 16.00 | 287.07 | 9.73 | 313.62 | 0.2255 | 975.0 | 808.2 | |
| 0.00 | 2.24 | 0.00 | 1.14 | 16.61 | 286.78 | 9.44 | 316.45 | 0.2292 | 896.0 | 670.4 | |
| 0.00 | 0.98 | 0.00 | 0.50 | 16.00 | 286.75 | 9.41 | 314.57 | 0.2217 | 761.0 | 597.2 | |
| 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. | |