SDO HMI 2014-08-22 03:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.29 | 149.66 | 14.60 | 92.85 | 16.51 | 27.76 | 36.50 | 288.43 | 0.6028 | -475.4 | -303.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.73 | 15.64 | 28.93 | 37.67 | 286.59 | 0.6162 | -127.0 | -143.7 | |
| 23.29 | 121.04 | 14.60 | 75.88 | 16.33 | 28.68 | 37.42 | 287.78 | 0.6146 | -1045.2 | -389.5 | |
| 0.00 | 5.22 | 0.00 | 3.20 | 17.78 | 26.72 | 35.46 | 290.75 | 0.5929 | -714.0 | -592.4 | |
| 0.00 | 0.99 | 0.00 | 0.60 | 14.43 | 25.88 | 34.62 | 285.35 | 0.5727 | -568.0 | -383.3 | |
| 0.00 | 1.26 | 0.00 | 0.77 | 17.71 | 26.39 | 35.13 | 290.75 | 0.5884 | -708.0 | -591.2 | |
| 0.00 | 3.42 | 0.00 | 2.07 | 17.09 | 25.91 | 34.64 | 289.89 | 0.5800 | -807.0 | -669.6 | |
| 0.00 | 1.89 | 0.00 | 1.15 | 17.43 | 25.86 | 34.60 | 290.48 | 0.5806 | -785.0 | -642.3 | |
| 0.00 | 1.08 | 0.00 | 0.63 | 17.70 | 21.68 | 30.42 | 292.77 | 0.5252 | 563.0 | 430.9 | |
| 0.00 | 3.69 | 0.00 | 2.13 | 17.25 | 21.34 | 30.08 | 292.11 | 0.5187 | 496.0 | 570.7 | |
| 0.00 | 1.26 | 0.00 | 0.73 | 18.28 | 21.39 | 30.13 | 293.98 | 0.5237 | 694.0 | 581.9 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 18.28 | 20.73 | 29.46 | 294.36 | 0.5147 | 673.0 | 612.3 | |
| 0.00 | 3.42 | 0.00 | 1.96 | 17.00 | 20.39 | 29.12 | 292.12 | 0.5044 | 875.0 | 680.0 | |
| 0.00 | 1.08 | 0.00 | 0.62 | 17.31 | 20.40 | 29.14 | 292.70 | 0.5060 | 531.0 | 468.2 | |
| 0.00 | 1.17 | 0.00 | 0.68 | 18.91 | 20.63 | 29.36 | 295.58 | 0.5163 | 745.0 | 660.5 | |
| 0.00 | 2.07 | 0.00 | 1.18 | 17.23 | 19.66 | 28.40 | 292.95 | 0.4953 | 797.0 | 520.3 | |
| 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. | |