| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.92 | 0.00 | 10.84 | 19.67 | 324.15 | 32.34 | 297.63 | 0.5701 | 44.4 | 54.7 | |
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back to the solar disc SDO HMI 2011-10-25 03:59:00 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.78 | 0.00 | 0.52 | 22.39 | 331.04 | 39.23 | 298.38 | 0.6670 | -658.0 | -591.4 | |
| 0.00 | 0.26 | 0.00 | 0.17 | 22.93 | 330.43 | 38.62 | 299.43 | 0.6624 | -654.0 | -555.7 | |
| 0.00 | 1.56 | 0.00 | 1.03 | 23.10 | 330.11 | 38.31 | 299.83 | 0.6596 | -704.0 | -500.6 | |
| 0.00 | 0.96 | 0.00 | 0.63 | 23.93 | 329.41 | 37.60 | 301.36 | 0.6554 | -642.0 | -538.8 | |
| 0.00 | 0.96 | 0.00 | 0.63 | 24.55 | 329.16 | 37.36 | 302.37 | 0.6558 | -726.0 | -622.0 | |
| 0.00 | 0.87 | 0.00 | 0.55 | 21.86 | 327.86 | 36.05 | 299.14 | 0.6276 | -617.0 | -493.1 | |
| 0.00 | 0.96 | 0.00 | 0.58 | 18.19 | 324.88 | 33.07 | 294.87 | 0.5737 | 575.0 | 468.2 | |
| 0.00 | 1.74 | 0.00 | 1.06 | 20.43 | 325.17 | 33.37 | 298.38 | 0.5880 | 595.0 | 466.5 | |
| 0.00 | 1.39 | 0.00 | 0.83 | 17.51 | 324.22 | 32.41 | 294.08 | 0.5621 | 696.0 | 652.2 | |
| 0.00 | 1.22 | 0.00 | 0.70 | 12.40 | 321.51 | 29.71 | 286.01 | 0.5056 | 791.0 | 683.6 | |
| 0.00 | 0.70 | 0.00 | 0.40 | 12.79 | 321.56 | 29.76 | 286.74 | 0.5075 | 845.0 | 658.2 | |
| 0.00 | 0.78 | 0.00 | 0.47 | 22.86 | 321.99 | 30.18 | 304.33 | 0.5632 | 613.0 | 463.1 | |
| 0.00 | 1.83 | 0.00 | 1.05 | 17.64 | 320.46 | 28.65 | 296.50 | 0.5127 | 743.0 | 602.8 | |
| 0.00 | 1.56 | 0.00 | 0.90 | 21.39 | 318.73 | 26.92 | 304.50 | 0.5136 | 656.0 | 539.7 | |
| 0.00 | 2.35 | 0.00 | 1.32 | 16.86 | 317.90 | 26.10 | 296.81 | 0.4737 | -847.0 | -665.7 | |
| 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. | |