| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.42 | 392.86 | 29.14 | 218.36 | 16.22 | 64.15 | 23.97 | 300.68 | 0.4560 | -1047.4 | -407.9 | |
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back to the solar disc SDO HMI 2011-11-13 05:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.03 | 0.00 | 0.58 | 14.17 | 66.81 | 26.63 | 294.45 | 0.4794 | 347.0 | 361.2 | |
| 51.47 | 375.64 | 28.62 | 208.81 | 16.05 | 64.30 | 24.12 | 300.21 | 0.4563 | -1391.6 | -418.8 | |
| 0.95 | -2.00 | 0.52 | -2.00 | 15.72 | 63.95 | 23.77 | 299.88 | 0.4494 | -1294.9 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 14.08 | 62.69 | 22.51 | 297.64 | 0.4210 | -747.0 | -492.4 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 14.23 | 62.54 | 22.36 | 298.12 | 0.4199 | -852.0 | -731.8 | |
| 0.00 | 1.64 | 0.00 | 0.90 | 17.61 | 62.64 | 22.46 | 304.95 | 0.4462 | -657.0 | -568.2 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 17.49 | 62.42 | 22.24 | 304.96 | 0.4424 | -823.0 | -637.2 | |
| 0.00 | 1.38 | 0.00 | 0.78 | 22.12 | 62.25 | 22.07 | 313.44 | 0.4814 | -830.0 | -667.4 | |
| 0.00 | 0.86 | 0.00 | 0.49 | 24.28 | 61.97 | 21.79 | 317.16 | 0.4996 | -516.0 | -438.3 | |
| 0.00 | 1.03 | 0.00 | 0.59 | 24.13 | 61.55 | 21.37 | 317.45 | 0.4938 | -818.0 | -563.8 | |
| 0.00 | 1.46 | 0.00 | 0.83 | 24.84 | 61.16 | 20.98 | 319.00 | 0.4972 | -618.0 | -410.8 | |
| 0.00 | 1.64 | 0.00 | 0.89 | 18.00 | 59.75 | 19.57 | 309.24 | 0.4131 | 603.0 | 475.2 | |
| 0.00 | 1.64 | 0.00 | 0.89 | 18.59 | 59.72 | 19.54 | 310.43 | 0.4182 | 857.0 | 706.1 | |
| 0.00 | 1.38 | 0.00 | 0.74 | 18.99 | 57.82 | 17.63 | 313.96 | 0.3997 | 847.0 | 604.0 | |
| 0.00 | 1.29 | 0.00 | 0.72 | 25.47 | 57.78 | 17.60 | 324.51 | 0.4723 | -646.0 | -503.1 | |
| 0.00 | 0.77 | 0.00 | 0.44 | 28.42 | 56.19 | 16.01 | 330.56 | 0.4954 | -831.0 | -684.1 | |
| 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. | |