| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 91.95 | 495.72 | 58.64 | 321.76 | 14.93 | 231.53 | -38.47 | 68.82 | 0.6453 | -513.7 | -134.0 | |
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back to the solar disc SDO HMI 2011-11-23 02:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.20 | 62.22 | 2.58 | 38.39 | 12.88 | 235.19 | -34.81 | 70.61 | 0.5922 | 632.3 | -374.4 | |
| 12.08 | 265.35 | 7.54 | 165.82 | 14.93 | 234.45 | -35.54 | 67.64 | 0.6097 | -1208.2 | -413.7 | |
| 12.77 | -1.00 | 7.88 | -1.00 | 12.96 | 234.73 | -35.27 | 70.67 | 0.5986 | -883.5 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.99 | 18.01 | 233.56 | -36.44 | 63.37 | 0.6342 | -699.0 | -604.3 | |
| 3.51 | -1.00 | 2.17 | -1.00 | 12.57 | 234.49 | -35.50 | 71.40 | 0.6003 | -694.4 | 999999 | |
| 33.51 | -2.00 | 20.97 | -2.00 | 14.68 | 234.09 | -35.91 | 68.20 | 0.6134 | -1121.4 | 999999 | |
| 2.40 | -2.00 | 1.51 | -2.00 | 15.10 | 234.00 | -35.99 | 67.58 | 0.6161 | -819.7 | 999999 | |
| 0.00 | 1.63 | 0.00 | 1.00 | 11.69 | 234.52 | -35.48 | 72.82 | 0.5972 | 851.0 | 667.4 | |
| 5.74 | -1.00 | 3.57 | -1.00 | 13.04 | 234.08 | -35.92 | 70.80 | 0.6075 | -725.1 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.59 | 12.25 | 233.61 | -36.39 | 72.25 | 0.6111 | -375.0 | -341.3 | |
| 0.00 | 1.20 | 0.00 | 0.75 | 12.70 | 233.42 | -36.58 | 71.61 | 0.6149 | -684.0 | -555.4 | |
| 0.00 | 1.71 | 0.00 | 1.09 | 14.56 | 232.73 | -37.27 | 68.96 | 0.6302 | -692.0 | -540.0 | |
| 0.00 | 2.40 | 0.00 | 1.53 | 14.29 | 232.67 | -37.33 | 69.41 | 0.6300 | -558.0 | -519.9 | |
| 0.00 | 0.34 | 0.00 | 0.22 | 13.86 | 232.37 | -37.63 | 70.19 | 0.6324 | -308.0 | -354.8 | |
| 0.00 | 2.23 | 0.00 | 1.41 | 12.11 | 232.60 | -37.39 | 72.83 | 0.6238 | 927.0 | 713.9 | |
| 0.00 | 1.11 | 0.00 | 0.72 | 15.76 | 231.66 | -38.34 | 67.60 | 0.6480 | -817.0 | -640.2 | |
| 0.00 | 0.94 | 0.00 | 0.62 | 16.23 | 230.60 | -39.40 | 67.34 | 0.6627 | -674.0 | -566.4 | |
| 2.66 | 3.86 | 1.75 | 2.54 | 15.46 | 230.50 | -39.50 | 68.50 | 0.6612 | -683.0 | -710.1 | |
| 0.00 | 0.94 | 0.00 | 0.63 | 16.24 | 229.43 | -40.57 | 67.79 | 0.6768 | -535.0 | -478.5 | |
| 0.00 | 3.00 | 0.00 | 2.04 | 17.33 | 228.77 | -41.23 | 66.50 | 0.6884 | -715.0 | -593.0 | |
| 0.00 | 0.94 | 0.00 | 0.64 | 15.15 | 228.63 | -41.36 | 69.63 | 0.6828 | 572.0 | 499.2 | |
| 0.00 | 1.29 | 0.00 | 0.91 | 17.28 | 226.51 | -43.49 | 67.40 | 0.7141 | -525.0 | -444.9 | |
| 0.00 | 10.46 | 0.00 | 7.34 | 16.82 | 226.65 | -43.35 | 67.98 | 0.7112 | 469.0 | 384.3 | |
| 0.00 | 1.54 | 0.00 | 1.10 | 18.01 | 226.03 | -43.97 | 66.58 | 0.7219 | -595.0 | -420.1 | |
| 2.06 | 3.60 | 1.46 | 2.55 | 17.27 | 226.17 | -43.83 | 67.53 | 0.7180 | -374.7 | -281.6 | |
| 3.17 | 115.79 | 2.22 | 81.66 | 15.38 | 226.62 | -43.38 | 69.97 | 0.7073 | 873.9 | 452.3 | |
| 0.94 | -26.00 | 0.66 | -26.00 | 15.62 | 226.55 | -43.45 | 69.65 | 0.7087 | 858.0 | 999999 | |
| 0.00 | 1.71 | 0.00 | 1.23 | 17.85 | 225.78 | -44.22 | 66.88 | 0.7242 | -463.0 | -380.2 | |
| 2.14 | -26.00 | 1.51 | -26.00 | 15.59 | 226.31 | -43.69 | 69.78 | 0.7115 | 1023.3 | 999999 | |
| 0.00 | 1.63 | 0.00 | 1.16 | 17.36 | 225.76 | -44.24 | 67.55 | 0.7229 | -275.0 | -183.2 | |
| 4.71 | -26.00 | 3.33 | -26.00 | 16.04 | 226.01 | -43.99 | 69.25 | 0.7161 | 1083.3 | 999999 | |
| 0.00 | 1.89 | 0.00 | 1.34 | 16.92 | 225.76 | -44.24 | 68.13 | 0.7216 | 337.0 | 423.8 | |
| 0.43 | -26.00 | 0.30 | -26.00 | 15.55 | 225.97 | -44.02 | 69.93 | 0.7152 | 730.4 | 999999 | |
| 0.60 | -26.00 | 0.43 | -26.00 | 15.64 | 225.82 | -44.18 | 69.86 | 0.7172 | 573.9 | 999999 | |
| 0.00 | 1.63 | 0.00 | 1.20 | 18.97 | 224.48 | -45.52 | 65.85 | 0.7419 | -682.0 | -499.9 | |
| 1.03 | 5.83 | 0.76 | 4.29 | 15.77 | 223.63 | -46.37 | 70.31 | 0.7421 | -500.1 | -358.0 | |
| 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. | |