SDO HMI 2014-08-03 04:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.73 | 213.75 | 51.61 | 290.53 | 9.09 | 172.89 | -69.00 | 82.54 | 0.9306 | 274.9 | 58.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.89 | 33.12 | 5.42 | 36.63 | 9.98 | 177.84 | -64.05 | 81.79 | 0.8966 | -751.9 | -496.7 | |
| 0.00 | 1.54 | 0.00 | 1.72 | 9.65 | 177.67 | -64.22 | 82.15 | 0.8979 | -99.0 | -132.4 | |
| 0.00 | 1.54 | 0.00 | 1.73 | 9.81 | 177.40 | -64.49 | 81.96 | 0.9000 | -311.0 | -222.9 | |
| 0.00 | 2.53 | 0.00 | 2.96 | 9.87 | 176.42 | -65.47 | 81.85 | 0.9072 | -519.0 | -321.8 | |
| 0.00 | 0.27 | 0.00 | 0.33 | 10.64 | 175.65 | -66.24 | 80.99 | 0.9125 | -103.0 | -96.0 | |
| 0.00 | 3.80 | 0.00 | 4.69 | 9.34 | 175.00 | -66.89 | 82.38 | 0.9173 | 291.0 | 173.2 | |
| 0.00 | 8.05 | 0.00 | 10.29 | 9.41 | 174.08 | -67.81 | 82.26 | 0.9235 | 757.0 | 506.2 | |
| 2.90 | 12.94 | 3.85 | 17.10 | 11.23 | 173.07 | -68.82 | 80.25 | 0.9295 | -42.2 | 318.2 | |
| 0.00 | 0.27 | 0.00 | 0.35 | 8.75 | 173.93 | -67.96 | 82.97 | 0.9247 | 361.0 | 398.3 | |
| 4.16 | 149.42 | 5.60 | 214.33 | 8.93 | 172.92 | -68.97 | 82.72 | 0.9311 | 634.4 | 120.0 | |
| 2.17 | -10.00 | 3.02 | -10.00 | 9.03 | 172.08 | -69.81 | 82.57 | 0.9363 | 657.6 | 999999 | |
| 6.24 | -10.00 | 8.69 | -10.00 | 8.64 | 172.15 | -69.74 | 82.99 | 0.9360 | 624.9 | 999999 | |
| 5.79 | -10.00 | 8.19 | -10.00 | 9.19 | 171.74 | -70.15 | 82.39 | 0.9383 | 550.0 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.40 | 10.57 | 171.05 | -70.84 | 80.87 | 0.9419 | 279.0 | 263.3 | |
| 11.58 | -10.00 | 16.84 | -10.00 | 8.40 | 171.24 | -70.65 | 83.20 | 0.9415 | 266.8 | 999999 | |
| 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. | |