| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.84 | 0.00 | 13.28 | 13.77 | 91.24 | -13.21 | 57.50 | 0.2630 | 263.5 | 357.0 | |
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back to the solar disc SDO HMI 2014-10-07 02:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.20 | 0.00 | 1.09 | 9.41 | 101.60 | -2.85 | 43.14 | 0.0721 | -1034.0 | -896.8 | |
| 0.00 | 0.97 | 0.00 | 0.48 | 12.25 | 99.09 | -5.36 | 41.82 | 0.1377 | -795.0 | -552.4 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 16.79 | 98.23 | -6.23 | 29.90 | 0.2092 | -620.0 | -493.2 | |
| 0.00 | 1.76 | 0.00 | 0.88 | 10.61 | 97.71 | -6.75 | 57.38 | 0.1377 | -1137.0 | -958.6 | |
| 0.00 | 2.11 | 0.00 | 1.09 | 17.49 | 92.73 | -11.72 | 44.92 | 0.2756 | 550.0 | 507.8 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 12.93 | 90.94 | -13.52 | 62.94 | 0.2570 | 643.0 | 511.2 | |
| 0.00 | 0.97 | 0.00 | 0.50 | 19.03 | 90.42 | -14.04 | 45.99 | 0.3202 | 794.0 | 687.8 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 16.34 | 89.34 | -15.12 | 54.88 | 0.3073 | 744.0 | 506.6 | |
| 0.00 | 7.64 | 0.00 | 3.94 | 13.47 | 89.44 | -15.01 | 63.36 | 0.2831 | 1287.0 | 1058.5 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 20.83 | 88.33 | -16.13 | 45.74 | 0.3640 | 745.0 | 690.9 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 12.41 | 87.43 | -17.02 | 69.10 | 0.3074 | 785.0 | 606.7 | |
| 0.00 | 1.76 | 0.00 | 0.91 | 8.11 | 87.22 | -17.23 | 83.31 | 0.2966 | -151.0 | -194.1 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 14.74 | 86.45 | -18.01 | 63.36 | 0.3359 | 797.0 | 653.6 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 15.62 | 84.73 | -19.73 | 62.92 | 0.3667 | 685.0 | 572.1 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 16.02 | 83.96 | -20.50 | 62.72 | 0.3803 | 660.0 | 574.3 | |
| 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. | |