SDO HMI 2014-07-20 17:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.95 | 234.28 | 35.09 | 130.84 | -21.25 | 68.29 | 8.36 | 197.16 | 0.4621 | 137.4 | 140.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.42 | 165.62 | 7.51 | 92.62 | -21.26 | 69.55 | 9.62 | 199.55 | 0.4674 | 1037.3 | 336.4 | |
| 18.50 | -1.00 | 10.32 | -1.00 | -20.92 | 69.33 | 9.40 | 199.40 | 0.4613 | 1265.6 | 999999 | |
| 0.73 | -1.00 | 0.41 | -1.00 | -21.15 | 69.05 | 9.12 | 198.69 | 0.4633 | 711.5 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -20.30 | 68.67 | 8.74 | 198.59 | 0.4489 | 507.0 | 408.2 | |
| 2.81 | 4.35 | 1.55 | 2.40 | -19.96 | 68.16 | 8.23 | 197.82 | 0.4414 | 975.0 | 701.6 | |
| 0.00 | 0.91 | 0.00 | 0.50 | -19.85 | 67.66 | 7.73 | 196.89 | 0.4374 | 801.0 | 618.9 | |
| 0.00 | 0.73 | 0.00 | 0.40 | -20.86 | 67.61 | 7.69 | 196.11 | 0.4523 | 499.0 | 510.1 | |
| 0.00 | 2.63 | 0.00 | 1.45 | -20.37 | 66.41 | 6.48 | 193.97 | 0.4401 | -809.0 | -659.4 | |
| 0.00 | 2.36 | 0.00 | 1.32 | -22.31 | 66.13 | 6.20 | 192.37 | 0.4684 | -833.0 | -562.4 | |
| 0.00 | 0.91 | 0.00 | 0.50 | -21.45 | 65.93 | 6.00 | 192.41 | 0.4548 | -746.0 | -598.5 | |
| 2.00 | 10.07 | 1.11 | 5.62 | -22.06 | 65.52 | 5.60 | 191.31 | 0.4627 | -934.4 | -750.1 | |
| 0.00 | 5.62 | 0.00 | 3.15 | -22.37 | 65.54 | 5.61 | 191.19 | 0.4674 | -753.0 | -612.5 | |
| 13.79 | 18.50 | 7.66 | 10.28 | -21.55 | 65.31 | 5.38 | 191.11 | 0.4543 | -1161.2 | -746.0 | |
| 11.70 | 21.31 | 6.53 | 11.90 | -22.12 | 64.90 | 4.97 | 190.05 | 0.4619 | -946.5 | -694.7 | |
| 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. | |