| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.83 | 86.48 | 17.81 | 53.35 | 19.04 | 170.85 | -32.70 | 58.86 | 0.5987 | -1.8 | 27.0 | |
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back to the solar disc SDO HMI 2011-11-28 03:58:56 UT
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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 | 1.42 | 19.18 | 174.63 | -28.92 | 55.85 | 0.5540 | -702.0 | -477.8 | |
| 4.96 | 9.41 | 3.00 | 5.68 | 18.41 | 172.54 | -31.01 | 58.68 | 0.5744 | -919.6 | -608.1 | |
| 3.25 | 26.86 | 1.98 | 16.40 | 18.93 | 171.89 | -31.66 | 58.34 | 0.5856 | -859.6 | -406.4 | |
| 6.25 | -3.00 | 3.81 | -3.00 | 18.68 | 171.65 | -31.90 | 58.89 | 0.5870 | -765.2 | 999999 | |
| 0.00 | 1.71 | 0.00 | 1.05 | 19.71 | 171.31 | -32.24 | 57.57 | 0.5973 | -740.0 | -613.3 | |
| 0.00 | 1.97 | 0.00 | 1.21 | 19.64 | 171.14 | -32.41 | 57.78 | 0.5989 | -233.0 | -111.7 | |
| 1.71 | 2.48 | 1.07 | 1.55 | 20.61 | 170.42 | -33.13 | 56.85 | 0.6133 | 647.5 | 523.7 | |
| 1.28 | 16.51 | 0.79 | 10.19 | 19.26 | 170.67 | -32.89 | 58.68 | 0.6023 | 619.7 | 356.9 | |
| 0.00 | 0.86 | 0.00 | 0.53 | 17.56 | 170.63 | -32.93 | 61.32 | 0.5930 | -676.0 | -548.9 | |
| 0.00 | 2.91 | 0.00 | 1.81 | 19.26 | 170.18 | -33.37 | 59.01 | 0.6080 | 870.0 | 698.9 | |
| 6.33 | 9.32 | 3.97 | 5.85 | 19.56 | 169.58 | -33.97 | 58.94 | 0.6169 | 767.2 | 673.9 | |
| 0.00 | 1.11 | 0.00 | 0.70 | 18.19 | 169.26 | -34.30 | 61.19 | 0.6132 | 366.0 | 401.9 | |
| 5.05 | 9.32 | 3.19 | 5.90 | 18.65 | 168.50 | -35.05 | 60.96 | 0.6247 | 904.5 | 613.7 | |
| 0.00 | 0.68 | 0.00 | 0.44 | 20.39 | 167.99 | -35.56 | 58.73 | 0.6401 | 741.0 | 588.9 | |
| 0.00 | 0.94 | 0.00 | 0.62 | 21.57 | 166.51 | -37.04 | 57.95 | 0.6633 | 589.0 | 509.5 | |
| 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. | |