SDO HMI 2014-07-06 17:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.43 | 45.49 | 16.17 | 39.58 | -12.88 | 298.41 | 53.22 | 251.74 | 0.8241 | 92.1 | 29.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.54 | 20.79 | 6.77 | 18.70 | -13.29 | 299.66 | 54.46 | 251.60 | 0.8367 | 712.3 | 486.3 | |
| 2.72 | -1.00 | 2.46 | -1.00 | -13.64 | 299.78 | 54.58 | 251.22 | 0.8386 | 586.3 | 999999 | |
| 0.91 | -1.00 | 0.81 | -1.00 | -13.29 | 299.17 | 53.98 | 251.46 | 0.8323 | 702.2 | 999999 | |
| 0.00 | 1.18 | 0.00 | 1.05 | -13.45 | 299.17 | 53.98 | 251.27 | 0.8327 | 622.0 | 644.2 | |
| 0.00 | 1.27 | 0.00 | 1.12 | -13.12 | 298.90 | 53.71 | 251.59 | 0.8295 | 816.0 | 717.4 | |
| 0.00 | 1.09 | 0.00 | 0.93 | -12.62 | 297.76 | 52.56 | 251.86 | 0.8175 | -280.0 | -333.7 | |
| 0.00 | 1.09 | 0.00 | 0.94 | -13.07 | 297.84 | 52.64 | 251.35 | 0.8193 | -219.0 | -172.8 | |
| 3.72 | 7.99 | 3.14 | 6.73 | -11.81 | 297.37 | 52.18 | 252.72 | 0.8119 | -578.6 | -456.8 | |
| 0.00 | 1.00 | 0.00 | 0.86 | -13.31 | 297.65 | 52.46 | 251.01 | 0.8182 | -388.0 | -292.9 | |
| 2.27 | 4.27 | 1.93 | 3.63 | -13.14 | 297.34 | 52.15 | 251.13 | 0.8148 | -627.8 | -452.0 | |
| 1.27 | 3.54 | 1.06 | 2.94 | -11.90 | 296.59 | 51.39 | 252.40 | 0.8044 | -635.8 | -513.7 | |
| 0.00 | 0.27 | 0.00 | 0.22 | -11.29 | 296.43 | 51.24 | 253.09 | 0.8014 | -420.0 | -331.0 | |
| 0.00 | 2.36 | 0.00 | 1.94 | -12.31 | 296.05 | 50.85 | 251.74 | 0.8001 | -375.0 | -268.6 | |
| 0.00 | 0.64 | 0.00 | 0.52 | -13.25 | 295.81 | 50.62 | 250.53 | 0.8002 | -662.0 | -565.3 | |
| 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. | |