| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.68 | 171.94 | 20.00 | 96.40 | 17.88 | 223.63 | 22.81 | 307.96 | 0.4701 | -624.4 | -361.6 | |
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back to the solar disc SDO HMI 2011-11-28 08:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.48 | 15.00 | 225.82 | 24.99 | 300.40 | 0.4751 | 766.0 | 573.2 | |
| 0.00 | 0.34 | 0.00 | 0.19 | 16.77 | 225.88 | 25.06 | 303.60 | 0.4889 | 740.0 | 603.5 | |
| 0.00 | 0.77 | 0.00 | 0.44 | 16.40 | 225.73 | 24.91 | 303.08 | 0.4842 | 588.0 | 520.9 | |
| 11.21 | 157.22 | 6.30 | 88.23 | 17.71 | 224.28 | 23.46 | 306.92 | 0.4763 | -1041.4 | -406.2 | |
| 0.86 | -4.00 | 0.48 | -4.00 | 17.65 | 223.93 | 23.11 | 307.19 | 0.4715 | -983.8 | 999999 | |
| 22.33 | -4.00 | 12.51 | -4.00 | 17.99 | 223.51 | 22.69 | 308.28 | 0.4693 | -1143.6 | 999999 | |
| 1.28 | 1.80 | 0.71 | 0.99 | 15.75 | 222.86 | 22.04 | 304.89 | 0.4421 | 635.9 | 298.3 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 16.06 | 222.66 | 21.84 | 305.71 | 0.4421 | 309.0 | 304.5 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 15.33 | 222.38 | 21.56 | 304.61 | 0.4324 | 990.0 | 795.7 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 17.29 | 222.31 | 21.49 | 308.44 | 0.4484 | -745.0 | -468.3 | |
| 0.00 | 4.02 | 0.00 | 2.25 | 19.87 | 221.61 | 20.79 | 313.84 | 0.4647 | -852.0 | -735.2 | |
| 0.00 | 1.20 | 0.00 | 0.66 | 18.42 | 219.80 | 18.97 | 313.84 | 0.4295 | 578.0 | 487.3 | |
| 0.00 | 1.71 | 0.00 | 0.95 | 20.99 | 219.08 | 18.25 | 319.18 | 0.4493 | 765.0 | 605.7 | |
| 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. | |