| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.75 | 357.89 | 38.78 | 233.63 | 16.03 | 110.32 | -38.34 | 66.56 | 0.6520 | -844.5 | -273.2 | |
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back to the solar disc SDO HMI 2014-11-27 08:00:26 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.72 | 344.28 | 38.11 | 223.81 | 16.02 | 110.62 | -38.04 | 66.47 | 0.6484 | -1239.4 | -310.1 | |
| 1.03 | -1.00 | 0.67 | -1.00 | 16.50 | 109.84 | -38.83 | 66.11 | 0.6598 | -466.8 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.59 | 16.96 | 107.21 | -41.46 | 66.56 | 0.6926 | 566.0 | 484.8 | |
| 0.00 | 1.54 | 0.00 | 1.06 | 17.42 | 107.04 | -41.62 | 65.99 | 0.6962 | 486.0 | 470.7 | |
| 0.00 | 2.05 | 0.00 | 1.45 | 16.38 | 105.10 | -43.57 | 68.14 | 0.7149 | 642.0 | 452.0 | |
| 0.00 | 1.80 | 0.00 | 1.28 | 16.40 | 104.45 | -44.22 | 68.33 | 0.7223 | 554.0 | 465.1 | |
| 0.00 | 1.11 | 0.00 | 0.80 | 15.93 | 104.23 | -44.43 | 69.02 | 0.7233 | -152.0 | -201.0 | |
| 0.00 | 0.68 | 0.00 | 0.50 | 16.34 | 102.84 | -45.82 | 68.91 | 0.7400 | 716.0 | 683.9 | |
| 0.00 | 1.54 | 0.00 | 1.14 | 16.21 | 102.17 | -46.50 | 69.29 | 0.7470 | 630.0 | 527.6 | |
| 0.00 | 0.26 | 0.00 | 0.19 | 16.45 | 102.05 | -46.62 | 69.00 | 0.7489 | 466.0 | 512.7 | |
| 0.00 | 1.03 | 0.00 | 0.77 | 15.71 | 101.73 | -46.93 | 70.06 | 0.7504 | 654.0 | 619.2 | |
| 0.00 | 1.97 | 0.00 | 1.46 | 15.07 | 101.83 | -46.83 | 70.87 | 0.7478 | 513.0 | 374.2 | |
| 0.00 | 0.77 | 0.00 | 0.58 | 15.56 | 101.51 | -47.16 | 70.33 | 0.7525 | 429.0 | 345.7 | |
| 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. | |