| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.47 | 278.62 | 63.38 | 527.18 | 19.00 | 106.42 | 75.03 | 288.88 | 0.9659 | -266.6 | -171.0 | |
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back to the solar disc SDO HMI 2011-11-13 21:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.26 | 125.89 | 17.94 | 273.54 | 19.06 | 108.44 | 77.05 | 288.87 | 0.9745 | 353.5 | 91.4 | |
| 14.79 | -1.00 | 30.99 | -1.00 | 19.05 | 108.01 | 76.62 | 288.87 | 0.9729 | -480.8 | 999999 | |
| 0.00 | 13.84 | 0.00 | 26.28 | 19.03 | 106.42 | 75.03 | 288.90 | 0.9665 | -435.0 | -408.9 | |
| 2.58 | 109.30 | 4.54 | 180.84 | 18.60 | 105.16 | 73.77 | 288.49 | 0.9608 | -463.6 | -467.6 | |
| 5.07 | -4.00 | 8.63 | -4.00 | 18.50 | 104.50 | 73.11 | 288.43 | 0.9577 | -666.2 | 999999 | |
| 0.77 | -4.00 | 1.28 | -4.00 | 18.43 | 104.09 | 72.70 | 288.37 | 0.9557 | -820.7 | 999999 | |
| 0.00 | 7.40 | 0.00 | 13.03 | 21.34 | 105.08 | 73.69 | 291.36 | 0.9611 | -485.0 | -392.1 | |
| 0.00 | 1.81 | 0.00 | 2.87 | 19.88 | 103.18 | 71.79 | 289.94 | 0.9516 | -607.0 | -563.6 | |
| 0.00 | 7.22 | 0.00 | 11.24 | 20.35 | 102.69 | 71.30 | 290.46 | 0.9493 | -427.0 | -316.6 | |
| 0.00 | 3.35 | 0.00 | 5.20 | 20.80 | 102.59 | 71.20 | 290.94 | 0.9489 | -312.0 | -288.8 | |
| 0.00 | 7.14 | 0.00 | 10.55 | 20.02 | 101.65 | 70.26 | 290.18 | 0.9437 | -38.0 | -73.0 | |
| 0.00 | 1.12 | 0.00 | 1.54 | 19.57 | 100.03 | 68.64 | 289.82 | 0.9343 | 259.0 | 239.2 | |
| 0.00 | 1.55 | 0.00 | 2.09 | 19.65 | 99.58 | 68.19 | 289.94 | 0.9317 | 481.0 | 436.2 | |
| 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. | |