| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.84 | 27.04 | 0.97 | 13.91 | 12.63 | 93.32 | -13.34 | 62.08 | 0.2518 | 42.2 | 52.0 | |
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back to the solar disc SDO HMI 2014-10-06 22:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.40 | 0.00 | 0.70 | 10.14 | 102.31 | -4.35 | 48.94 | 0.0994 | -526.0 | -415.4 | |
| 0.00 | 1.23 | 0.00 | 0.61 | 12.21 | 101.58 | -5.08 | 40.59 | 0.1337 | -814.0 | -640.0 | |
| 0.00 | 1.32 | 0.00 | 0.66 | 9.35 | 101.53 | -5.13 | 59.77 | 0.1025 | -1029.0 | -789.4 | |
| 0.00 | 1.40 | 0.00 | 0.70 | 9.56 | 101.47 | -5.19 | 58.33 | 0.1053 | -964.0 | -801.3 | |
| 0.00 | 1.32 | 0.00 | 0.66 | 10.55 | 98.29 | -8.37 | 63.00 | 0.1613 | -813.0 | -588.1 | |
| 0.00 | 1.93 | 0.00 | 0.97 | 10.69 | 97.70 | -8.96 | 63.73 | 0.1714 | -1235.0 | -880.2 | |
| 0.00 | 1.58 | 0.00 | 0.80 | 10.50 | 97.18 | -9.48 | 65.91 | 0.1781 | -804.0 | -678.2 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 10.32 | 97.16 | -9.50 | 66.90 | 0.1774 | -871.0 | -702.6 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 14.38 | 95.09 | -11.57 | 54.14 | 0.2407 | -928.0 | -673.1 | |
| 0.88 | 7.64 | 0.46 | 3.99 | 13.44 | 89.51 | -17.15 | 66.13 | 0.3150 | 1243.7 | 937.6 | |
| 0.26 | -10.00 | 0.14 | -10.00 | 13.56 | 89.47 | -17.19 | 65.82 | 0.3163 | 1108.0 | 999999 | |
| 0.00 | 1.58 | 0.00 | 0.83 | 16.22 | 89.19 | -17.47 | 58.74 | 0.3388 | 862.0 | 693.3 | |
| 0.44 | -10.00 | 0.23 | -10.00 | 13.38 | 89.39 | -17.27 | 66.45 | 0.3165 | 1116.6 | 999999 | |
| 0.26 | -10.00 | 0.14 | -10.00 | 13.56 | 89.37 | -17.29 | 65.93 | 0.3178 | 1043.3 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 13.91 | 87.10 | -19.56 | 67.23 | 0.3540 | 650.0 | 423.2 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 14.81 | 86.86 | -19.80 | 65.09 | 0.3627 | 762.0 | 563.8 | |
| 0.00 | 2.81 | 0.00 | 1.49 | 14.71 | 86.54 | -20.12 | 65.66 | 0.3668 | 826.0 | 732.2 | |
| 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. | |