| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.77 | 47.16 | 11.30 | 26.92 | 17.98 | 214.51 | -25.31 | 55.03 | 0.4984 | 289.3 | 224.3 | |
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back to the solar disc SDO HMI 2011-11-25 09:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.88 | 0.00 | 1.05 | 18.44 | 217.29 | -22.52 | 51.29 | 0.4676 | 883.0 | 701.8 | |
| 0.00 | 1.88 | 0.00 | 1.07 | 19.24 | 216.43 | -23.39 | 50.89 | 0.4850 | 689.0 | 486.4 | |
| 0.00 | 1.03 | 0.00 | 0.59 | 20.51 | 215.81 | -24.00 | 49.46 | 0.5034 | 568.0 | 475.2 | |
| 0.00 | 0.94 | 0.00 | 0.54 | 20.10 | 215.74 | -24.07 | 50.20 | 0.5006 | 639.0 | 500.8 | |
| 0.00 | 0.68 | 0.00 | 0.40 | 21.70 | 215.36 | -24.45 | 48.07 | 0.5191 | 602.0 | 524.0 | |
| 0.00 | 1.46 | 0.00 | 0.83 | 19.26 | 215.53 | -24.28 | 51.83 | 0.4958 | 761.0 | 666.5 | |
| 3.68 | 9.93 | 2.08 | 5.61 | 17.25 | 215.46 | -24.36 | 55.41 | 0.4804 | -922.7 | -632.4 | |
| 3.08 | -7.00 | 1.74 | -7.00 | 17.18 | 215.09 | -24.72 | 55.89 | 0.4846 | -792.8 | 999999 | |
| 1.46 | 10.62 | 0.83 | 6.03 | 17.67 | 214.99 | -24.83 | 55.12 | 0.4897 | -751.4 | -565.3 | |
| 2.65 | -9.00 | 1.51 | -9.00 | 17.98 | 214.80 | -25.01 | 54.77 | 0.4944 | -691.6 | 999999 | |
| 0.00 | 2.48 | 0.00 | 1.42 | 17.97 | 213.94 | -25.87 | 55.62 | 0.5050 | 842.0 | 727.0 | |
| 0.00 | 1.71 | 0.00 | 0.98 | 17.59 | 213.45 | -26.37 | 56.72 | 0.5084 | 949.0 | 845.0 | |
| 1.63 | 13.01 | 0.94 | 7.51 | 17.90 | 213.33 | -26.49 | 56.30 | 0.5122 | 904.0 | 819.0 | |
| 5.39 | -13.00 | 3.11 | -13.00 | 17.81 | 213.07 | -26.75 | 56.70 | 0.5148 | 884.6 | 999999 | |
| 1.88 | -13.00 | 1.09 | -13.00 | 17.71 | 212.87 | -26.94 | 57.04 | 0.5165 | 773.2 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.89 | 17.68 | 212.67 | -27.15 | 57.27 | 0.5189 | 462.0 | 396.7 | |
| 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. | |