| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.38 | 111.84 | 15.02 | 68.78 | 18.09 | 223.69 | 32.77 | 299.77 | 0.5949 | -586.0 | -380.5 | |
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back to the solar disc SDO HMI 2011-11-29 02:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.26 | 28.90 | 0.16 | 17.92 | 18.06 | 224.65 | 33.73 | 299.08 | 0.6064 | -508.0 | -415.3 | |
| 5.13 | -1.00 | 3.18 | -1.00 | 17.81 | 224.45 | 33.53 | 298.83 | 0.6026 | -944.3 | 999999 | |
| 1.03 | -1.00 | 0.64 | -1.00 | 18.06 | 224.43 | 33.51 | 299.23 | 0.6037 | -744.1 | 999999 | |
| 0.00 | 1.80 | 0.00 | 1.12 | 18.96 | 224.59 | 33.67 | 300.48 | 0.6107 | -578.0 | -394.6 | |
| 0.00 | 2.65 | 0.00 | 1.64 | 17.78 | 224.14 | 33.22 | 298.98 | 0.5987 | -908.0 | -728.7 | |
| 0.00 | 1.62 | 0.00 | 1.00 | 17.51 | 223.97 | 33.06 | 298.66 | 0.5951 | -803.0 | -703.6 | |
| 0.00 | 2.48 | 0.00 | 1.52 | 17.64 | 223.56 | 32.64 | 299.13 | 0.5906 | -911.0 | -825.8 | |
| 17.96 | 66.70 | 11.04 | 40.98 | 18.22 | 223.61 | 32.69 | 300.01 | 0.5946 | -975.7 | -405.6 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 15.12 | 222.98 | 32.06 | 295.47 | 0.5697 | 751.0 | 619.0 | |
| 0.00 | 0.86 | 0.00 | 0.52 | 16.16 | 223.09 | 32.17 | 297.09 | 0.5766 | -343.0 | -286.6 | |
| 0.00 | 1.71 | 0.00 | 1.03 | 15.59 | 222.51 | 31.59 | 296.52 | 0.5662 | 597.0 | 447.5 | |
| 0.00 | 1.45 | 0.00 | 0.88 | 19.15 | 221.41 | 30.49 | 302.99 | 0.5737 | -748.0 | -602.3 | |
| 0.00 | 0.77 | 0.00 | 0.45 | 18.20 | 219.19 | 28.27 | 303.27 | 0.5402 | 735.0 | 590.9 | |
| 0.00 | 1.62 | 0.00 | 0.95 | 20.49 | 217.45 | 26.53 | 308.50 | 0.5367 | 743.0 | 590.9 | |
| 0.00 | 0.34 | 0.00 | 0.20 | 21.28 | 217.35 | 26.43 | 309.81 | 0.5421 | 471.0 | 550.8 | |
| 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. | |