| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 89.83 | 293.21 | 74.87 | 245.91 | -17.84 | 102.97 | 50.15 | 244.96 | 0.8069 | 96.1 | 47.5 | |
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back to the solar disc SDO HMI 2011-11-12 06:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.29 | 0.00 | 1.34 | -17.62 | 111.58 | 58.77 | 247.97 | 0.8811 | -408.0 | -324.9 | |
| 0.00 | 0.86 | 0.00 | 0.81 | -14.06 | 109.00 | 56.18 | 251.31 | 0.8529 | -349.0 | -310.6 | |
| 0.00 | 1.64 | 0.00 | 1.45 | -16.25 | 105.94 | 53.12 | 247.92 | 0.8309 | 595.0 | 540.4 | |
| 20.06 | 91.71 | 18.18 | 83.27 | -17.78 | 106.47 | 53.65 | 246.31 | 0.8397 | 787.9 | 216.6 | |
| 1.03 | -4.00 | 0.95 | -4.00 | -18.30 | 106.70 | 53.88 | 245.80 | 0.8430 | 180.8 | 999999 | |
| 0.00 | 1.12 | 0.00 | 1.02 | -18.41 | 106.33 | 53.51 | 245.55 | 0.8401 | 208.0 | 183.3 | |
| 7.58 | 14.55 | 6.82 | 13.08 | -18.49 | 105.94 | 53.12 | 245.33 | 0.8370 | 635.4 | 508.8 | |
| 0.00 | 0.60 | 0.00 | 0.55 | -18.90 | 106.02 | 53.21 | 244.89 | 0.8389 | 211.0 | 163.4 | |
| 0.00 | 2.15 | 0.00 | 1.88 | -17.78 | 105.01 | 52.19 | 245.84 | 0.8268 | 373.0 | 335.3 | |
| 1.38 | 2.41 | 1.20 | 2.10 | -17.92 | 104.71 | 51.90 | 245.57 | 0.8245 | 445.4 | 424.2 | |
| 0.34 | 5.77 | 0.30 | 4.98 | -17.66 | 104.56 | 51.74 | 245.82 | 0.8223 | 644.2 | 542.4 | |
| 0.00 | 0.86 | 0.00 | 0.75 | -18.24 | 104.80 | 51.98 | 245.23 | 0.8262 | -238.0 | -163.8 | |
| 0.00 | 1.46 | 0.00 | 1.31 | -19.74 | 105.42 | 52.60 | 243.73 | 0.8360 | 323.0 | 250.4 | |
| 0.00 | 1.03 | 0.00 | 0.88 | -17.48 | 104.08 | 51.26 | 245.87 | 0.8175 | 445.0 | 449.2 | |
| 0.86 | 11.45 | 0.74 | 9.81 | -18.16 | 104.31 | 51.49 | 245.16 | 0.8215 | 369.6 | 536.2 | |
| 0.00 | 1.21 | 0.00 | 1.03 | -17.32 | 103.97 | 51.15 | 246.02 | 0.8159 | 326.0 | 320.6 | |
| 2.67 | 18.26 | 2.27 | 15.43 | -17.66 | 103.80 | 50.98 | 245.57 | 0.8154 | 696.3 | 607.8 | |
| 2.24 | 5.08 | 1.87 | 4.26 | -16.90 | 103.17 | 50.35 | 246.23 | 0.8072 | -451.9 | 16.1 | |
| 9.82 | -17.00 | 8.27 | -17.00 | -17.64 | 103.35 | 50.53 | 245.43 | 0.8112 | 876.8 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.51 | -17.86 | 103.34 | 50.52 | 245.16 | 0.8117 | 598.0 | 523.0 | |
| 0.00 | 0.69 | 0.00 | 0.57 | -17.08 | 102.89 | 50.08 | 245.92 | 0.8052 | -129.0 | -127.9 | |
| 0.00 | 2.07 | 0.00 | 1.80 | -19.99 | 103.89 | 51.07 | 242.89 | 0.8235 | -255.0 | -299.6 | |
| 0.00 | 0.60 | 0.00 | 0.56 | -23.68 | 105.53 | 52.71 | 239.34 | 0.8491 | 358.0 | 268.9 | |
| 0.00 | 0.78 | 0.00 | 0.65 | -18.44 | 102.88 | 50.06 | 244.31 | 0.8094 | 292.0 | 297.9 | |
| 4.39 | 6.63 | 3.79 | 5.71 | -20.23 | 103.49 | 50.68 | 242.47 | 0.8208 | 553.3 | 619.2 | |
| 0.00 | 1.55 | 0.00 | 1.38 | -21.84 | 104.22 | 51.40 | 240.89 | 0.8324 | 509.0 | 387.8 | |
| 0.00 | 2.07 | 0.00 | 1.69 | -17.45 | 101.87 | 49.05 | 245.11 | 0.7966 | 683.0 | 584.7 | |
| 0.00 | 0.86 | 0.00 | 0.71 | -17.93 | 102.05 | 49.23 | 244.61 | 0.7999 | 681.0 | 548.6 | |
| 2.67 | 3.36 | 2.23 | 2.81 | -19.47 | 102.32 | 49.51 | 242.90 | 0.8077 | -447.6 | -333.8 | |
| 2.50 | 3.27 | 2.02 | 2.65 | -18.46 | 101.11 | 48.29 | 243.61 | 0.7928 | -290.7 | -158.7 | |
| 8.61 | 10.85 | 6.92 | 8.72 | -19.39 | 100.47 | 47.66 | 242.24 | 0.7901 | -568.8 | -296.0 | |
| 0.00 | 1.46 | 0.00 | 1.15 | -18.21 | 99.90 | 47.08 | 243.41 | 0.7802 | -394.0 | -244.5 | |
| 0.00 | 0.43 | 0.00 | 0.33 | -16.52 | 99.28 | 46.46 | 245.23 | 0.7678 | -201.0 | -253.6 | |
| 0.00 | 0.34 | 0.00 | 0.26 | -16.46 | 98.82 | 46.00 | 245.10 | 0.7629 | -521.0 | -511.5 | |
| 0.00 | 2.50 | 0.00 | 1.91 | -17.02 | 98.63 | 45.82 | 244.33 | 0.7631 | -333.0 | -139.8 | |
| 0.78 | 72.77 | 0.59 | 54.73 | -16.67 | 98.39 | 45.57 | 244.67 | 0.7592 | 195.3 | -442.9 | |
| 1.64 | 1.89 | 1.23 | 1.43 | -16.28 | 98.14 | 45.32 | 245.05 | 0.7552 | -560.5 | -567.3 | |
| 8.53 | -36.00 | 6.45 | -36.00 | -17.00 | 98.18 | 45.36 | 244.16 | 0.7584 | -688.1 | 999999 | |
| 0.00 | 2.50 | 0.00 | 1.93 | -18.48 | 98.62 | 45.80 | 242.54 | 0.7687 | -656.0 | -486.1 | |
| 0.00 | 0.86 | 0.00 | 0.66 | -17.92 | 98.21 | 45.39 | 243.04 | 0.7623 | -491.0 | -347.1 | |
| 0.00 | 1.81 | 0.00 | 1.39 | -18.56 | 98.25 | 45.43 | 242.27 | 0.7652 | -581.0 | -476.5 | |
| 0.00 | 1.64 | 0.00 | 1.24 | -17.56 | 97.83 | 45.01 | 243.32 | 0.7569 | 151.0 | 96.4 | |
| 0.00 | 2.50 | 0.00 | 1.90 | -18.42 | 98.02 | 45.20 | 242.34 | 0.7624 | -617.0 | -626.3 | |
| 0.00 | 1.03 | 0.00 | 0.77 | -16.37 | 97.33 | 44.51 | 244.58 | 0.7471 | -332.0 | -255.0 | |
| 9.99 | -36.00 | 7.48 | -36.00 | -17.13 | 97.52 | 44.70 | 243.71 | 0.7521 | -916.4 | 999999 | |
| 1.21 | -36.00 | 0.90 | -36.00 | -17.42 | 97.47 | 44.65 | 243.33 | 0.7528 | -558.9 | 999999 | |
| 3.53 | 5.60 | 2.66 | 4.22 | -18.24 | 97.52 | 44.70 | 242.33 | 0.7566 | -766.6 | -649.7 | |
| 0.00 | 3.10 | 0.00 | 2.28 | -16.97 | 96.60 | 43.78 | 243.49 | 0.7418 | -796.0 | -681.5 | |
| 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. | |