SDO HMI 2014-10-06 02:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.67 | 290.39 | 30.72 | 183.64 | -1.51 | 155.20 | 37.55 | 259.27 | 0.6223 | 812.0 | 323.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.09 | 261.22 | 21.63 | 165.76 | -1.55 | 155.53 | 37.88 | 259.32 | 0.6269 | 1098.0 | 332.3 | |
| 4.83 | -1.00 | 3.04 | -1.00 | -1.56 | 154.85 | 37.20 | 259.06 | 0.6178 | 1078.6 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.67 | -3.82 | 154.63 | 36.98 | 255.42 | 0.6224 | 580.0 | 496.2 | |
| 6.50 | 9.93 | 4.05 | 6.19 | -1.75 | 154.14 | 36.49 | 258.49 | 0.6089 | 929.9 | 703.5 | |
| 0.00 | 0.97 | 0.00 | 0.60 | -1.70 | 153.84 | 36.19 | 258.46 | 0.6046 | 686.0 | 577.1 | |
| 0.00 | 1.05 | 0.00 | 0.65 | -0.11 | 153.60 | 35.95 | 260.97 | 0.5967 | 754.0 | 641.2 | |
| 3.25 | 5.62 | 2.00 | 3.46 | -0.41 | 153.53 | 35.88 | 260.46 | 0.5965 | 904.8 | 703.0 | |
| 0.00 | 0.44 | 0.00 | 0.26 | 0.36 | 151.91 | 34.26 | 261.22 | 0.5718 | 452.0 | 489.8 | |
| 0.00 | 2.46 | 0.00 | 1.48 | -0.12 | 151.84 | 34.19 | 260.37 | 0.5721 | 780.0 | 636.1 | |
| 0.00 | 1.32 | 0.00 | 0.80 | -1.10 | 151.66 | 34.01 | 258.62 | 0.5727 | -334.0 | -229.2 | |
| 0.00 | 1.23 | 0.00 | 0.74 | -0.91 | 151.52 | 33.87 | 258.89 | 0.5700 | -354.0 | -329.3 | |
| 0.00 | 2.64 | 0.00 | 1.58 | -0.68 | 151.15 | 33.50 | 259.15 | 0.5642 | -761.0 | -630.3 | |
| 0.00 | 1.32 | 0.00 | 0.78 | -0.36 | 150.54 | 32.89 | 259.46 | 0.5545 | -674.0 | -504.1 | |
| 0.00 | 1.14 | 0.00 | 0.67 | -1.71 | 148.40 | 30.75 | 256.08 | 0.5286 | -671.0 | -525.3 | |
| 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. | |