SDO HMI 2011-10-15 18:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.85 | 190.20 | 17.24 | 118.59 | -26.74 | 36.69 | -18.78 | 151.85 | 0.6088 | 712.0 | 327.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.85 | 176.33 | 17.24 | 109.13 | -26.59 | 37.41 | -18.06 | 152.48 | 0.6021 | 1183.1 | 359.7 | |
| 0.00 | 0.96 | 0.00 | 0.62 | -28.11 | 33.98 | -21.49 | 149.68 | 0.6423 | 742.0 | 557.1 | |
| 0.00 | 1.05 | 0.00 | 0.67 | -27.90 | 33.99 | -21.48 | 149.50 | 0.6399 | 573.0 | 389.7 | |
| 0.00 | 0.61 | 0.00 | 0.39 | -26.30 | 34.02 | -21.45 | 148.06 | 0.6219 | 658.0 | 526.0 | |
| 0.00 | 2.18 | 0.00 | 1.40 | -27.55 | 33.62 | -21.84 | 148.77 | 0.6386 | 828.0 | 653.8 | |
| 0.00 | 0.26 | 0.00 | 0.17 | -27.97 | 33.21 | -22.26 | 148.68 | 0.6460 | 594.0 | 487.7 | |
| 0.00 | 0.96 | 0.00 | 0.62 | -27.72 | 33.19 | -22.28 | 148.43 | 0.6434 | 532.0 | 542.4 | |
| 0.00 | 1.05 | 0.00 | 0.70 | -29.56 | 30.82 | -24.65 | 147.58 | 0.6791 | 672.0 | 556.2 | |
| 0.00 | 1.83 | 0.00 | 1.26 | -28.15 | 27.04 | -28.43 | 142.57 | 0.6929 | -709.0 | -560.1 | |
| 0.00 | 1.22 | 0.00 | 0.84 | -27.95 | 26.71 | -28.76 | 142.07 | 0.6936 | -537.0 | -458.0 | |
| 0.00 | 0.87 | 0.00 | 0.61 | -28.48 | 24.99 | -30.48 | 141.05 | 0.7116 | -568.0 | -414.7 | |
| 0.00 | 0.35 | 0.00 | 0.26 | -30.38 | 22.21 | -33.26 | 140.64 | 0.7483 | -465.0 | -454.5 | |
| 0.00 | 1.66 | 0.00 | 1.24 | -30.26 | 21.93 | -33.54 | 140.29 | 0.7493 | -794.0 | -570.6 | |
| 0.00 | 0.87 | 0.00 | 0.68 | -29.67 | 17.96 | -37.51 | 136.77 | 0.7746 | -393.0 | -373.0 | |
| 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. | |