SDO HMI 2014-08-05 02:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.36 | 21.34 | 0.21 | 12.70 | -18.92 | 239.20 | 22.66 | 221.14 | 0.5551 | 228.0 | 200.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.45 | 0.00 | 0.28 | -16.93 | 244.06 | 27.52 | 229.38 | 0.5846 | 519.0 | 514.8 | |
| 0.00 | 1.45 | 0.00 | 0.88 | -17.66 | 242.71 | 26.17 | 227.00 | 0.5768 | 777.0 | 625.9 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -18.09 | 242.18 | 25.63 | 225.84 | 0.5754 | 469.0 | 361.8 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -19.44 | 241.04 | 24.50 | 222.84 | 0.5772 | 559.0 | 480.2 | |
| 0.00 | 1.54 | 0.00 | 0.93 | -19.20 | 240.97 | 24.43 | 223.06 | 0.5741 | 264.0 | 293.8 | |
| 0.00 | 2.53 | 0.00 | 1.51 | -18.12 | 240.66 | 24.12 | 224.09 | 0.5603 | 564.0 | 458.1 | |
| 0.00 | 3.35 | 0.00 | 2.01 | -19.21 | 240.30 | 23.76 | 222.28 | 0.5676 | 792.0 | 710.9 | |
| 0.00 | 1.18 | 0.00 | 0.71 | -19.74 | 240.31 | 23.77 | 221.62 | 0.5733 | 604.0 | 457.0 | |
| 0.00 | 1.27 | 0.00 | 0.76 | -19.86 | 239.94 | 23.40 | 221.04 | 0.5710 | 782.0 | 724.1 | |
| 0.00 | 0.99 | 0.00 | 0.59 | -18.31 | 238.87 | 22.33 | 221.69 | 0.5445 | 785.0 | 613.4 | |
| 0.36 | 2.62 | 0.21 | 1.55 | -20.04 | 237.10 | 20.56 | 217.26 | 0.5471 | -804.8 | -641.9 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -18.49 | 236.90 | 20.36 | 218.87 | 0.5278 | -661.0 | -521.6 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -19.44 | 234.46 | 17.92 | 214.27 | 0.5172 | -600.0 | -530.5 | |
| 0.00 | 2.17 | 0.00 | 1.24 | -18.61 | 233.86 | 17.32 | 214.34 | 0.5021 | -640.0 | -575.6 | |
| 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. | |