| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.40 | 0.00 | 12.27 | 14.19 | 58.66 | 33.91 | 286.71 | 0.5652 | 40.3 | 77.5 | |
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back to the solar disc SDO HMI 2014-10-13 03:00:31 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.66 | 0.00 | 1.10 | 13.21 | 66.58 | 41.83 | 283.10 | 0.6689 | -559.0 | -436.2 | |
| 0.00 | 1.49 | 0.00 | 0.98 | 13.05 | 66.29 | 41.55 | 282.89 | 0.6651 | -421.0 | -401.8 | |
| 0.00 | 0.88 | 0.00 | 0.56 | 10.28 | 63.83 | 39.09 | 278.91 | 0.6302 | -625.0 | -405.9 | |
| 0.00 | 0.79 | 0.00 | 0.50 | 14.65 | 63.24 | 38.49 | 285.94 | 0.6285 | -663.0 | -590.3 | |
| 0.00 | 1.31 | 0.00 | 0.80 | 13.29 | 60.16 | 35.41 | 284.45 | 0.5845 | 689.0 | 562.8 | |
| 0.00 | 0.61 | 0.00 | 0.38 | 19.27 | 60.46 | 35.71 | 294.21 | 0.6064 | -641.0 | -529.0 | |
| 0.00 | 2.28 | 0.00 | 1.38 | 16.31 | 59.06 | 34.31 | 289.92 | 0.5776 | -786.0 | -617.8 | |
| 0.00 | 1.23 | 0.00 | 0.74 | 16.82 | 58.67 | 33.92 | 290.94 | 0.5741 | -481.0 | -432.9 | |
| 0.00 | 2.28 | 0.00 | 1.32 | 13.48 | 55.77 | 31.02 | 286.07 | 0.5236 | 531.0 | 415.2 | |
| 0.00 | 0.96 | 0.00 | 0.56 | 13.25 | 55.70 | 30.95 | 285.64 | 0.5219 | 675.0 | 526.0 | |
| 0.00 | 1.58 | 0.00 | 0.91 | 13.50 | 55.38 | 30.63 | 286.25 | 0.5180 | 824.0 | 676.3 | |
| 0.00 | 3.06 | 0.00 | 1.76 | 13.74 | 54.87 | 30.13 | 286.89 | 0.5116 | 745.0 | 641.1 | |
| 0.00 | 0.96 | 0.00 | 0.55 | 13.32 | 54.32 | 29.57 | 286.27 | 0.5023 | 538.0 | 389.5 | |
| 0.00 | 1.31 | 0.00 | 0.73 | 16.17 | 49.96 | 25.22 | 294.41 | 0.4512 | 738.0 | 647.1 | |
| 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. | |