| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.30 | 151.79 | 53.89 | 251.64 | 19.68 | 87.70 | 72.25 | 289.78 | 0.9530 | -41.7 | -134.5 | |
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back to the solar disc SDO HMI 2011-11-15 02:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.32 | 59.51 | 4.59 | 116.04 | 19.37 | 91.09 | 75.63 | 289.27 | 0.9692 | 340.8 | -155.8 | |
| 5.76 | -1.00 | 11.10 | -1.00 | 19.24 | 90.65 | 75.19 | 289.14 | 0.9674 | -572.3 | 999999 | |
| 0.60 | -1.00 | 1.19 | -1.00 | 19.66 | 90.98 | 75.52 | 289.57 | 0.9688 | 193.7 | 999999 | |
| 2.84 | 7.40 | 4.71 | 12.29 | 18.17 | 88.10 | 72.65 | 288.14 | 0.9557 | 270.3 | 40.0 | |
| 0.00 | 0.43 | 0.00 | 0.72 | 19.06 | 88.34 | 72.89 | 289.06 | 0.9570 | -271.0 | -299.8 | |
| 0.60 | 3.44 | 0.98 | 5.60 | 19.22 | 87.66 | 72.21 | 289.26 | 0.9538 | -427.9 | -389.3 | |
| 2.75 | 70.77 | 4.14 | 101.79 | 18.10 | 86.13 | 70.67 | 288.17 | 0.9455 | 298.7 | -119.7 | |
| 0.00 | 0.95 | 0.00 | 1.50 | 19.27 | 87.21 | 71.75 | 289.34 | 0.9515 | -371.0 | -348.6 | |
| 3.18 | 4.73 | 4.59 | 6.83 | 18.39 | 85.18 | 69.73 | 288.54 | 0.9404 | 314.4 | 88.2 | |
| 0.00 | 0.69 | 0.00 | 1.10 | 20.98 | 87.18 | 71.72 | 291.14 | 0.9520 | -383.0 | -390.6 | |
| 1.03 | 2.49 | 1.54 | 3.72 | 21.20 | 85.75 | 70.29 | 291.48 | 0.9447 | 225.3 | 112.7 | |
| 0.00 | 1.38 | 0.00 | 2.05 | 21.39 | 85.67 | 70.22 | 291.69 | 0.9444 | 197.0 | 120.8 | |
| 4.99 | -7.00 | 6.92 | -7.00 | 20.42 | 84.20 | 68.75 | 290.77 | 0.9357 | 433.5 | 999999 | |
| 2.92 | -7.00 | 4.02 | -7.00 | 20.68 | 83.93 | 68.48 | 291.08 | 0.9343 | 327.8 | 999999 | |
| 5.33 | -7.00 | 7.36 | -7.00 | 20.87 | 84.03 | 68.57 | 291.27 | 0.9349 | -545.5 | 999999 | |
| 1.98 | -7.00 | 2.75 | -7.00 | 21.24 | 84.22 | 68.77 | 291.64 | 0.9363 | -439.9 | 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. | |