| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.53 | 318.46 | 23.68 | 182.11 | 17.72 | 61.98 | -20.90 | 42.89 | 0.5008 | -705.2 | -361.3 | |
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back to the solar disc SDO HMI 2011-05-03 07:59:07 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.43 | 0.00 | 0.84 | 22.65 | 62.99 | -19.89 | 35.25 | 0.5461 | -719.0 | -564.9 | |
| 0.00 | 1.25 | 0.00 | 0.74 | 22.52 | 62.80 | -20.08 | 35.65 | 0.5462 | -698.0 | -492.6 | |
| 0.00 | 0.54 | 0.00 | 0.32 | 22.76 | 62.45 | -20.43 | 35.83 | 0.5520 | -436.0 | -409.5 | |
| 40.90 | 299.17 | 23.30 | 170.40 | 17.54 | 62.31 | -20.57 | 42.75 | 0.4955 | -1262.9 | -408.3 | |
| 0.00 | 2.05 | 0.00 | 1.24 | 22.96 | 60.37 | -22.51 | 38.20 | 0.5722 | -582.0 | -501.1 | |
| 0.00 | 1.16 | 0.00 | 0.69 | 18.25 | 56.84 | -26.04 | 48.30 | 0.5605 | 762.0 | 639.5 | |
| 0.00 | 2.95 | 0.00 | 1.77 | 18.68 | 56.59 | -26.29 | 47.96 | 0.5670 | 756.0 | 627.7 | |
| 0.00 | 0.89 | 0.00 | 0.54 | 19.35 | 56.23 | -26.65 | 47.42 | 0.5769 | 578.0 | 457.2 | |
| 0.00 | 1.88 | 0.00 | 1.12 | 17.29 | 56.39 | -26.49 | 50.14 | 0.5569 | 622.0 | 551.5 | |
| 0.00 | 1.07 | 0.00 | 0.65 | 19.39 | 56.00 | -26.87 | 47.60 | 0.5796 | 539.0 | 415.9 | |
| 0.00 | 1.07 | 0.00 | 0.65 | 19.03 | 56.03 | -26.85 | 48.06 | 0.5761 | 452.0 | 453.4 | |
| 0.00 | 1.52 | 0.00 | 0.96 | 22.69 | 54.72 | -28.16 | 44.63 | 0.6221 | 475.0 | 399.4 | |
| 0.00 | 1.52 | 0.00 | 0.98 | 23.11 | 53.38 | -29.50 | 45.37 | 0.6386 | 677.0 | 523.2 | |
| 0.63 | 1.96 | 0.38 | 1.21 | 18.19 | 53.58 | -29.30 | 51.58 | 0.5957 | 822.3 | 659.5 | |
| 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. | |