SDO HMI 2014-07-06 23:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.79 | 0.00 | 10.05 | -13.32 | 256.23 | 14.37 | 219.66 | 0.3784 | 636.7 | 572.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 0.59 | -12.50 | 259.91 | 18.04 | 227.97 | 0.4088 | 711.0 | 534.7 | |
| 0.00 | 2.09 | 0.00 | 1.14 | -13.20 | 259.76 | 17.90 | 226.47 | 0.4144 | 729.0 | 585.7 | |
| 0.00 | 0.54 | 0.00 | 0.30 | -13.73 | 259.41 | 17.54 | 224.95 | 0.4162 | 681.0 | 604.7 | |
| 0.00 | 0.82 | 0.00 | 0.44 | -14.16 | 258.69 | 16.82 | 223.02 | 0.4130 | 570.0 | 551.1 | |
| 0.00 | 1.09 | 0.00 | 0.59 | -14.00 | 258.54 | 16.68 | 223.05 | 0.4096 | 903.0 | 756.3 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -13.71 | 258.39 | 16.52 | 223.30 | 0.4046 | 689.0 | 487.1 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -13.30 | 256.57 | 14.71 | 220.74 | 0.3802 | 779.0 | 677.7 | |
| 0.00 | 1.36 | 0.00 | 0.72 | -11.90 | 256.33 | 14.47 | 222.86 | 0.3609 | 590.0 | 570.1 | |
| 0.00 | 4.27 | 0.00 | 2.29 | -14.75 | 255.69 | 13.83 | 216.59 | 0.3893 | 949.0 | 817.0 | |
| 0.00 | 1.63 | 0.00 | 0.86 | -11.99 | 254.32 | 12.45 | 218.46 | 0.3405 | 964.0 | 741.8 | |
| 0.00 | 1.18 | 0.00 | 0.62 | -11.51 | 254.01 | 12.14 | 218.68 | 0.3313 | 761.0 | 556.0 | |
| 0.00 | 1.18 | 0.00 | 0.61 | -11.16 | 251.21 | 9.35 | 212.29 | 0.2996 | 716.0 | 565.5 | |
| 0.00 | 1.27 | 0.00 | 0.67 | -14.55 | 250.41 | 8.55 | 204.96 | 0.3423 | -765.0 | -625.3 | |
| 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. | |