SDO HMI 2014-09-24 14:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.95 | 37.58 | 2.49 | 18.98 | 14.37 | 261.49 | -7.93 | 45.63 | 0.1878 | -45.2 | 68.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.77 | 0.00 | 0.89 | 13.29 | 263.54 | -5.89 | 42.04 | 0.1497 | -817.0 | -514.5 | |
| 0.00 | 2.03 | 0.00 | 1.02 | 14.81 | 263.44 | -5.99 | 36.37 | 0.1708 | -965.0 | -742.0 | |
| 0.88 | 5.75 | 0.44 | 2.89 | 14.71 | 262.94 | -6.48 | 38.90 | 0.1747 | -1012.7 | -816.1 | |
| 0.00 | 2.48 | 0.00 | 1.25 | 14.74 | 262.53 | -6.89 | 40.50 | 0.1795 | -755.0 | -415.1 | |
| 0.00 | 1.33 | 0.00 | 0.67 | 15.27 | 261.67 | -7.76 | 41.85 | 0.1960 | -878.0 | -635.4 | |
| 4.07 | 9.81 | 2.05 | 4.94 | 13.36 | 261.58 | -7.85 | 49.79 | 0.1748 | 1086.4 | 876.0 | |
| 0.00 | 3.09 | 0.00 | 1.56 | 13.60 | 261.26 | -8.17 | 49.85 | 0.1815 | -256.0 | -56.1 | |
| 0.00 | 0.71 | 0.00 | 0.36 | 13.86 | 260.93 | -8.49 | 49.78 | 0.1886 | -703.0 | -586.1 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 13.74 | 260.88 | -8.55 | 50.47 | 0.1881 | -694.0 | -432.9 | |
| 0.00 | 1.95 | 0.00 | 0.98 | 14.86 | 260.39 | -9.03 | 47.59 | 0.2064 | 636.0 | 573.5 | |
| 0.00 | 1.77 | 0.00 | 0.90 | 15.21 | 259.78 | -9.65 | 48.14 | 0.2181 | 548.0 | 589.5 | |
| 0.00 | 3.71 | 0.00 | 1.89 | 15.57 | 259.70 | -9.73 | 47.11 | 0.2231 | 734.0 | 732.0 | |
| 0.00 | 1.68 | 0.00 | 0.86 | 15.68 | 259.12 | -10.30 | 48.32 | 0.2316 | 905.0 | 679.9 | |
| 0.00 | 0.62 | 0.00 | 0.32 | 16.10 | 258.59 | -10.83 | 48.34 | 0.2428 | 776.0 | 569.9 | |
| 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. | |