SDO HMI 2014-08-07 22:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.54 | 19.04 | 0.31 | 11.08 | -19.50 | 160.84 | -18.24 | 145.75 | 0.5242 | 444.5 | 376.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.54 | 2.71 | 0.31 | 1.53 | -19.59 | 166.58 | -12.50 | 154.80 | 0.4807 | -902.0 | -714.4 | |
| 0.00 | 1.17 | 0.00 | 0.67 | -20.49 | 165.81 | -13.27 | 154.31 | 0.4981 | 793.0 | 662.0 | |
| 0.00 | 0.63 | 0.00 | 0.35 | -17.12 | 165.16 | -13.91 | 149.71 | 0.4575 | 366.0 | 396.1 | |
| 0.00 | 0.27 | 0.00 | 0.15 | -17.04 | 164.28 | -14.79 | 148.07 | 0.4635 | 759.0 | 736.3 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -20.13 | 163.06 | -16.02 | 149.52 | 0.5127 | 589.0 | 509.6 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -17.24 | 162.25 | -16.83 | 144.93 | 0.4832 | 641.0 | 476.5 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -20.09 | 160.25 | -18.83 | 145.31 | 0.5347 | 778.0 | 568.0 | |
| 0.00 | 1.54 | 0.00 | 0.91 | -21.19 | 159.93 | -19.15 | 146.09 | 0.5503 | 719.0 | 534.6 | |
| 0.00 | 1.54 | 0.00 | 0.88 | -17.35 | 159.82 | -19.25 | 141.41 | 0.5066 | 878.0 | 671.1 | |
| 0.00 | 3.43 | 0.00 | 2.02 | -20.22 | 159.41 | -19.67 | 144.30 | 0.5434 | 799.0 | 674.8 | |
| 0.00 | 1.08 | 0.00 | 0.65 | -20.89 | 157.82 | -21.26 | 142.98 | 0.5647 | 661.0 | 578.1 | |
| 0.00 | 1.35 | 0.00 | 0.81 | -20.01 | 157.88 | -21.20 | 142.03 | 0.5543 | 495.0 | 461.2 | |
| 0.00 | 1.45 | 0.00 | 0.83 | -16.27 | 157.98 | -21.09 | 137.41 | 0.5125 | 694.0 | 602.8 | |
| 0.00 | 1.08 | 0.00 | 0.67 | -21.60 | 154.26 | -24.82 | 139.54 | 0.6036 | -630.0 | -423.5 | |
| 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. | |