SDO HMI 2014-11-15 07:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.89 | 101.17 | 31.07 | 135.50 | 13.83 | 15.66 | 68.27 | 283.77 | 0.9299 | -403.7 | -98.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.33 | 26.58 | 7.62 | 38.10 | 13.22 | 17.25 | 69.87 | 283.05 | 0.9398 | -395.9 | -95.1 | |
| 0.00 | 0.60 | 0.00 | 0.80 | 12.56 | 15.56 | 68.18 | 282.41 | 0.9294 | -498.0 | -440.0 | |
| 0.69 | 41.38 | 0.94 | 56.29 | 13.91 | 16.21 | 68.83 | 283.82 | 0.9337 | -33.9 | 17.9 | |
| 1.72 | -3.00 | 2.35 | -3.00 | 14.09 | 16.16 | 68.78 | 284.02 | 0.9335 | 43.5 | 999999 | |
| 4.39 | 14.88 | 5.81 | 19.67 | 13.42 | 15.48 | 68.10 | 283.33 | 0.9291 | -592.0 | -432.8 | |
| 4.65 | -3.00 | 6.26 | -3.00 | 14.17 | 15.87 | 68.48 | 284.12 | 0.9317 | -540.2 | 999999 | |
| 5.51 | -3.00 | 7.43 | -3.00 | 14.41 | 15.94 | 68.56 | 284.37 | 0.9322 | -534.3 | 999999 | |
| 0.00 | 4.56 | 0.00 | 5.89 | 14.06 | 14.81 | 67.43 | 284.06 | 0.9250 | -527.0 | -382.5 | |
| 0.00 | 1.81 | 0.00 | 2.26 | 15.20 | 14.01 | 66.63 | 285.34 | 0.9203 | -619.0 | -495.6 | |
| 0.00 | 0.43 | 0.00 | 0.48 | 13.80 | 11.08 | 63.69 | 283.99 | 0.8991 | -125.0 | -119.8 | |
| 0.00 | 1.12 | 0.00 | 1.26 | 14.81 | 11.12 | 63.73 | 285.11 | 0.8999 | -550.0 | -525.9 | |
| 0.00 | 1.20 | 0.00 | 1.33 | 14.21 | 10.67 | 63.28 | 284.49 | 0.8962 | 174.0 | 202.6 | |
| 0.00 | 0.95 | 0.00 | 1.05 | 14.39 | 10.76 | 63.37 | 284.68 | 0.8970 | 275.0 | 221.5 | |
| 0.60 | 7.14 | 0.66 | 7.80 | 13.90 | 10.17 | 62.78 | 284.17 | 0.8923 | 529.1 | 302.0 | |
| 0.00 | 0.52 | 0.00 | 0.57 | 15.63 | 10.39 | 63.01 | 286.09 | 0.8950 | -513.0 | -510.0 | |
| 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. | |