SDO HMI 2014-11-07 19:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.38 | 29.41 | 0.77 | 16.26 | 5.50 | 72.50 | 26.23 | 275.14 | 0.4429 | -174.0 | -291.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 6.81 | 0.00 | 3.87 | 5.59 | 75.72 | 29.45 | 274.82 | 0.4930 | -1001.0 | -715.3 | |
| 0.00 | 0.78 | 0.00 | 0.44 | 5.42 | 75.57 | 29.30 | 274.48 | 0.4907 | -553.0 | -441.9 | |
| 0.60 | 1.98 | 0.34 | 1.12 | 5.32 | 74.85 | 28.58 | 274.34 | 0.4796 | -944.3 | -805.8 | |
| 0.00 | 2.16 | 0.00 | 1.21 | 4.05 | 74.69 | 28.42 | 271.67 | 0.4769 | -733.0 | -593.2 | |
| 0.00 | 0.60 | 0.00 | 0.34 | 4.47 | 74.64 | 28.37 | 272.55 | 0.4761 | -575.0 | -500.4 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 4.00 | 73.54 | 27.27 | 271.54 | 0.4591 | -843.0 | -693.5 | |
| 0.00 | 5.00 | 0.00 | 2.77 | 5.23 | 73.05 | 26.78 | 274.28 | 0.4519 | -861.0 | -816.9 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 5.15 | 72.65 | 26.38 | 274.14 | 0.4456 | -750.0 | -679.6 | |
| 0.00 | 0.69 | 0.00 | 0.38 | 6.40 | 72.61 | 26.35 | 276.95 | 0.4462 | -613.0 | -502.9 | |
| 0.78 | 2.76 | 0.43 | 1.52 | 5.98 | 71.79 | 25.52 | 276.13 | 0.4328 | 881.6 | 699.0 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 6.05 | 67.88 | 21.61 | 277.09 | 0.3707 | 770.0 | 582.2 | |
| 0.00 | 3.19 | 0.00 | 1.68 | 6.42 | 66.43 | 20.16 | 278.52 | 0.3478 | 930.0 | 687.9 | |
| 0.00 | 1.21 | 0.00 | 0.64 | 5.74 | 66.27 | 20.00 | 276.60 | 0.3442 | 824.0 | 673.3 | |
| 0.00 | 1.21 | 0.00 | 0.64 | 6.45 | 66.27 | 20.00 | 278.67 | 0.3453 | 840.0 | 707.1 | |
| 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. | |