| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.30 | 117.09 | 22.31 | 75.70 | 8.32 | 132.55 | -36.78 | 67.68 | 0.6422 | 545.6 | 305.2 | |
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back to the solar disc SDO HMI 2014-02-26 05:00:27 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.64 | 0.00 | 0.93 | 6.48 | 143.09 | -26.24 | 63.04 | 0.4949 | -736.0 | -603.7 | |
| 0.00 | 2.84 | 0.00 | 1.65 | 7.03 | 141.11 | -28.23 | 63.82 | 0.5252 | -663.0 | -658.2 | |
| 0.00 | 1.03 | 0.00 | 0.60 | 7.32 | 140.92 | -28.42 | 63.49 | 0.5296 | -634.0 | -508.8 | |
| 0.00 | 0.86 | 0.00 | 0.50 | 4.93 | 139.66 | -29.68 | 68.59 | 0.5320 | -677.0 | -559.9 | |
| 0.00 | 1.03 | 0.00 | 0.61 | 6.44 | 138.84 | -30.49 | 66.58 | 0.5516 | -534.0 | -422.2 | |
| 0.00 | 1.55 | 0.00 | 0.97 | 7.13 | 134.74 | -34.60 | 68.21 | 0.6090 | 685.0 | 556.3 | |
| 0.00 | 0.95 | 0.00 | 0.60 | 6.97 | 133.62 | -35.72 | 69.12 | 0.6226 | -529.0 | -481.5 | |
| 0.00 | 0.43 | 0.00 | 0.27 | 5.98 | 132.96 | -36.38 | 70.97 | 0.6263 | -585.0 | -452.0 | |
| 9.22 | 30.25 | 5.95 | 19.54 | 8.64 | 132.59 | -36.74 | 67.24 | 0.6437 | 1079.7 | 495.6 | |
| 0.00 | 1.46 | 0.00 | 0.94 | 7.14 | 132.56 | -36.78 | 69.45 | 0.6367 | 657.0 | 599.0 | |
| 0.00 | 1.38 | 0.00 | 0.90 | 8.62 | 132.14 | -37.19 | 67.54 | 0.6491 | 705.0 | 634.1 | |
| 0.00 | 1.29 | 0.00 | 0.83 | 7.24 | 132.14 | -37.20 | 69.54 | 0.6425 | 694.0 | 548.1 | |
| 0.00 | 1.72 | 0.00 | 1.11 | 7.43 | 132.04 | -37.29 | 69.31 | 0.6445 | 654.0 | 536.8 | |
| 25.08 | 66.87 | 16.36 | 43.74 | 8.40 | 131.75 | -37.59 | 68.07 | 0.6528 | 821.9 | 324.8 | |
| 0.00 | 2.50 | 0.00 | 1.65 | 9.58 | 131.30 | -38.04 | 66.66 | 0.6640 | 304.0 | 287.6 | |
| 0.00 | 1.29 | 0.00 | 0.86 | 9.17 | 131.01 | -38.33 | 67.40 | 0.6655 | 599.0 | 450.6 | |
| 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. | |