SDO HMI 2014-08-04 18:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.44 | 23.60 | 1.42 | 13.54 | -18.94 | 238.46 | 17.50 | 214.03 | 0.5093 | -123.0 | 24.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.18 | 0.00 | 0.69 | -16.08 | 245.08 | 24.11 | 226.90 | 0.5397 | 651.0 | 516.8 | |
| 0.00 | 3.89 | 0.00 | 2.26 | -17.73 | 242.15 | 21.18 | 221.00 | 0.5267 | 827.0 | 721.0 | |
| 2.44 | 4.07 | 1.42 | 2.36 | -19.12 | 240.27 | 19.30 | 216.68 | 0.5249 | 984.4 | 795.7 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -19.76 | 240.34 | 19.38 | 216.03 | 0.5330 | 670.0 | 520.2 | |
| 0.00 | 1.99 | 0.00 | 1.16 | -19.80 | 239.56 | 18.60 | 214.89 | 0.5268 | 855.0 | 745.8 | |
| 0.00 | 2.17 | 0.00 | 1.24 | -19.27 | 237.74 | 16.78 | 212.80 | 0.5051 | -521.0 | -343.9 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -20.63 | 237.18 | 16.22 | 210.44 | 0.5178 | -342.0 | -400.0 | |
| 0.00 | 1.45 | 0.00 | 0.83 | -20.05 | 237.08 | 16.12 | 210.91 | 0.5098 | -760.0 | -589.9 | |
| 0.00 | 0.63 | 0.00 | 0.35 | -17.31 | 236.12 | 15.16 | 212.46 | 0.4672 | -776.0 | -633.6 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -19.72 | 236.04 | 15.08 | 209.61 | 0.4976 | -778.0 | -610.5 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -20.18 | 234.58 | 13.62 | 206.73 | 0.4933 | -597.0 | -493.9 | |
| 0.00 | 1.81 | 0.00 | 1.01 | -18.62 | 234.12 | 13.16 | 207.50 | 0.4690 | -833.0 | -634.8 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -19.15 | 233.93 | 12.97 | 206.63 | 0.4749 | -798.0 | -605.2 | |
| 0.00 | 1.45 | 0.00 | 0.81 | -19.25 | 232.65 | 11.69 | 204.23 | 0.4679 | -770.0 | -545.4 | |
| 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. | |