SDO HMI 2014-11-28 12:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.88 | 34.73 | 2.66 | 18.83 | 17.03 | 151.67 | 18.37 | 312.20 | 0.4090 | 158.9 | -124.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.40 | 0.00 | 1.32 | 18.10 | 153.69 | 20.39 | 311.36 | 0.4431 | 965.0 | 747.0 | |
| 3.42 | 7.61 | 1.88 | 4.19 | 18.01 | 153.35 | 20.05 | 311.66 | 0.4382 | 941.5 | 828.7 | |
| 0.43 | 2.14 | 0.23 | 1.17 | 18.08 | 152.60 | 19.30 | 312.82 | 0.4301 | 861.6 | 758.0 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 10.81 | 151.75 | 18.45 | 298.35 | 0.3548 | 860.0 | 665.3 | |
| 0.00 | 0.60 | 0.00 | 0.32 | 16.79 | 152.00 | 18.70 | 311.28 | 0.4101 | 560.0 | 391.0 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 16.33 | 151.72 | 18.42 | 310.79 | 0.4023 | 650.0 | 574.6 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 15.99 | 151.59 | 18.29 | 310.31 | 0.3974 | 812.0 | 672.9 | |
| 0.00 | 1.28 | 0.00 | 0.69 | 16.83 | 150.80 | 17.50 | 313.17 | 0.3963 | -703.0 | -545.6 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 17.47 | 150.83 | 17.53 | 314.34 | 0.4034 | -663.0 | -474.4 | |
| 0.00 | 10.35 | 0.00 | 5.56 | 16.37 | 150.69 | 17.39 | 312.44 | 0.3902 | -974.0 | -802.4 | |
| 0.00 | 1.97 | 0.00 | 1.07 | 18.37 | 150.66 | 17.36 | 316.25 | 0.4112 | -862.0 | -739.3 | |
| 0.00 | 0.68 | 0.00 | 0.37 | 17.44 | 150.44 | 17.13 | 314.92 | 0.3986 | -715.0 | -542.1 | |
| 1.03 | 2.91 | 0.55 | 1.56 | 17.45 | 149.85 | 16.55 | 315.88 | 0.3921 | -1072.2 | -820.4 | |
| 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. | |