| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 79.59 | 260.62 | 50.23 | 165.73 | -17.81 | 101.53 | 32.79 | 235.50 | 0.6265 | -48.4 | -69.0 | |
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back to the solar disc SDO HMI 2011-11-11 01:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.67 | -18.99 | 114.68 | 45.94 | 241.87 | 0.7728 | -608.0 | -506.2 | |
| 0.00 | 0.69 | 0.00 | 0.50 | -13.42 | 112.95 | 44.22 | 248.12 | 0.7334 | -500.0 | -409.5 | |
| 0.00 | 0.95 | 0.00 | 0.68 | -17.19 | 111.22 | 42.48 | 242.47 | 0.7298 | -649.0 | -581.1 | |
| 0.00 | 0.78 | 0.00 | 0.53 | -12.28 | 109.97 | 41.23 | 248.38 | 0.6951 | -520.0 | -443.4 | |
| 0.00 | 0.69 | 0.00 | 0.48 | -14.70 | 110.11 | 41.37 | 245.18 | 0.7068 | -605.0 | -532.1 | |
| 0.00 | 1.29 | 0.00 | 0.90 | -15.10 | 110.04 | 41.31 | 244.61 | 0.7078 | -645.0 | -462.1 | |
| 0.00 | 0.95 | 0.00 | 0.65 | -14.48 | 109.37 | 40.63 | 245.10 | 0.6975 | -660.0 | -574.2 | |
| 0.00 | 1.12 | 0.00 | 0.76 | -15.51 | 107.92 | 39.18 | 242.95 | 0.6858 | -602.0 | -536.5 | |
| 16.11 | 116.99 | 10.63 | 77.00 | -18.51 | 104.35 | 35.61 | 236.75 | 0.6626 | 974.8 | 335.2 | |
| 1.55 | -9.00 | 1.02 | -9.00 | -18.49 | 103.84 | 35.11 | 236.42 | 0.6569 | 759.8 | 999999 | |
| 12.92 | -9.00 | 8.43 | -9.00 | -18.23 | 103.63 | 34.89 | 236.63 | 0.6529 | 966.2 | 999999 | |
| 0.00 | 3.02 | 0.00 | 1.93 | -16.94 | 102.93 | 34.19 | 237.91 | 0.6368 | -577.0 | -466.2 | |
| 4.91 | 5.60 | 3.12 | 3.55 | -17.22 | 101.94 | 33.20 | 236.80 | 0.6274 | 803.6 | 599.4 | |
| 0.34 | 1.55 | 0.22 | 0.98 | -17.46 | 101.73 | 32.99 | 236.30 | 0.6266 | 695.2 | 587.6 | |
| 0.00 | 1.98 | 0.00 | 1.25 | -16.85 | 101.46 | 32.72 | 236.95 | 0.6195 | 187.0 | 162.4 | |
| 5.60 | 7.24 | 3.53 | 4.57 | -17.42 | 101.39 | 32.65 | 236.10 | 0.6225 | 850.1 | 672.7 | |
| 1.38 | 3.70 | 0.86 | 2.31 | -16.52 | 100.73 | 31.99 | 236.88 | 0.6088 | 712.9 | 650.1 | |
| 0.00 | 1.21 | 0.00 | 0.76 | -18.35 | 100.73 | 31.99 | 234.29 | 0.6216 | 468.0 | 395.4 | |
| 0.00 | 0.95 | 0.00 | 0.59 | -16.99 | 99.95 | 31.21 | 235.57 | 0.6030 | -391.0 | -262.5 | |
| 0.00 | 0.95 | 0.00 | 0.59 | -17.63 | 99.96 | 31.22 | 234.68 | 0.6077 | -542.0 | -473.4 | |
| 0.00 | 0.78 | 0.00 | 0.48 | -17.37 | 99.80 | 31.06 | 234.91 | 0.6040 | -438.0 | -387.0 | |
| 0.00 | 1.55 | 0.00 | 0.95 | -17.06 | 98.95 | 30.21 | 234.65 | 0.5920 | -391.0 | -238.3 | |
| 0.00 | 1.64 | 0.00 | 1.00 | -16.74 | 98.82 | 30.08 | 235.00 | 0.5881 | -514.0 | -438.3 | |
| 1.46 | 4.22 | 0.89 | 2.57 | -16.39 | 98.72 | 29.98 | 235.43 | 0.5844 | -731.6 | -575.9 | |
| 0.00 | 1.21 | 0.00 | 0.73 | -16.16 | 98.43 | 29.69 | 235.53 | 0.5794 | -659.0 | -559.1 | |
| 7.84 | 16.97 | 4.79 | 10.36 | -17.17 | 98.46 | 29.72 | 234.07 | 0.5873 | -634.3 | -299.2 | |
| 0.00 | 2.15 | 0.00 | 1.31 | -16.73 | 98.39 | 29.65 | 234.65 | 0.5830 | -916.0 | -758.8 | |
| 2.33 | -26.00 | 1.42 | -26.00 | -16.98 | 98.32 | 29.58 | 234.23 | 0.5842 | -804.9 | 999999 | |
| 0.00 | 2.33 | 0.00 | 1.41 | -16.25 | 98.16 | 29.42 | 235.16 | 0.5768 | -903.0 | -801.2 | |
| 0.00 | 0.78 | 0.00 | 0.47 | -17.96 | 98.21 | 29.47 | 232.72 | 0.5904 | -585.0 | -489.1 | |
| 2.07 | 2.58 | 1.25 | 1.56 | -16.55 | 97.93 | 29.19 | 234.50 | 0.5764 | -853.3 | -848.3 | |
| 0.34 | 49.62 | 0.21 | 30.11 | -17.50 | 97.99 | 29.25 | 233.17 | 0.5844 | -493.0 | -689.7 | |
| 2.67 | -32.00 | 1.62 | -32.00 | -17.12 | 97.81 | 29.07 | 233.57 | 0.5794 | -1022.3 | 999999 | |
| 7.06 | -32.00 | 4.29 | -32.00 | -17.53 | 97.74 | 29.00 | 232.91 | 0.5818 | -1098.3 | 999999 | |
| 13.01 | 26.27 | 7.95 | 16.08 | -18.39 | 97.68 | 28.94 | 231.64 | 0.5879 | -859.7 | -405.7 | |
| 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. | |