| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.37 | 50.17 | 8.87 | 25.65 | -20.20 | 68.24 | -3.43 | 167.32 | 0.2472 | 389.7 | 163.2 | |
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back to the solar disc SDO HMI 2011-02-11 06:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.30 | 13.10 | 4.23 | 6.67 | -19.96 | 70.91 | -0.76 | 176.91 | 0.2317 | 1181.5 | 863.4 | |
| 0.00 | 0.86 | 0.00 | 0.43 | -19.26 | 70.79 | -0.88 | 176.20 | 0.2199 | 794.0 | 578.1 | |
| 6.76 | 8.73 | 3.45 | 4.45 | -20.32 | 70.50 | -1.17 | 175.37 | 0.2383 | 1056.7 | 790.0 | |
| 0.00 | 1.97 | 0.00 | 1.01 | -20.72 | 70.27 | -1.39 | 174.65 | 0.2453 | 847.0 | 612.8 | |
| 0.00 | 2.14 | 0.00 | 1.09 | -20.32 | 70.21 | -1.45 | 174.26 | 0.2387 | 1014.0 | 841.6 | |
| 0.00 | 1.71 | 0.00 | 0.87 | -20.41 | 69.99 | -1.68 | 173.43 | 0.2407 | 861.0 | 692.3 | |
| 0.00 | 1.63 | 0.00 | 0.83 | -20.20 | 69.68 | -1.99 | 172.09 | 0.2377 | 1060.0 | 834.0 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -20.35 | 69.33 | -2.34 | 170.83 | 0.2411 | 776.0 | 619.9 | |
| 0.00 | 2.23 | 0.00 | 1.13 | -18.79 | 68.01 | -3.66 | 163.99 | 0.2202 | 862.0 | 677.9 | |
| 0.00 | 1.71 | 0.00 | 0.88 | -20.70 | 67.46 | -4.21 | 164.22 | 0.2538 | 975.0 | 667.9 | |
| 2.31 | 6.25 | 1.19 | 3.21 | -19.99 | 64.25 | -7.42 | 152.37 | 0.2629 | -1089.8 | -830.0 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -20.78 | 63.70 | -7.97 | 152.14 | 0.2786 | -985.0 | -789.2 | |
| 0.00 | 1.54 | 0.00 | 0.79 | -20.62 | 63.51 | -8.15 | 151.33 | 0.2778 | -943.0 | -695.6 | |
| 0.00 | 1.80 | 0.00 | 0.93 | -20.65 | 63.19 | -8.47 | 150.45 | 0.2808 | -914.0 | -725.3 | |
| 0.00 | 1.37 | 0.00 | 0.71 | -20.92 | 62.89 | -8.78 | 150.10 | 0.2872 | -842.0 | -708.9 | |
| 0.00 | 1.80 | 0.00 | 0.93 | -20.39 | 62.57 | -9.10 | 148.20 | 0.2825 | -1091.0 | -885.3 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -21.28 | 62.45 | -9.22 | 149.57 | 0.2959 | -848.0 | -662.1 | |
| 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. | |