| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.88 | 145.17 | 19.52 | 122.01 | 20.28 | 193.96 | 51.35 | 294.91 | 0.8095 | -424.2 | -247.7 | |
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back to the solar disc SDO HMI 2011-12-02 18:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.43 | 124.10 | 6.42 | 105.91 | 20.07 | 195.39 | 52.78 | 294.19 | 0.8221 | -501.0 | -291.2 | |
| 15.45 | -1.00 | 13.10 | -1.00 | 19.89 | 194.53 | 51.92 | 294.21 | 0.8138 | -919.8 | 999999 | |
| 0.00 | 1.62 | 0.00 | 1.22 | 15.69 | 189.72 | 47.10 | 290.38 | 0.7547 | -702.0 | -553.4 | |
| 0.00 | 0.85 | 0.00 | 0.68 | 20.99 | 191.40 | 48.78 | 296.51 | 0.7872 | -582.0 | -490.7 | |
| 0.00 | 0.94 | 0.00 | 0.75 | 21.18 | 191.15 | 48.53 | 296.83 | 0.7853 | -593.0 | -516.4 | |
| 0.00 | 1.45 | 0.00 | 1.16 | 21.43 | 191.26 | 48.64 | 297.10 | 0.7872 | -646.0 | -571.4 | |
| 0.00 | 3.84 | 0.00 | 3.05 | 21.91 | 190.85 | 48.23 | 297.83 | 0.7848 | -544.0 | -481.1 | |
| 0.00 | 1.02 | 0.00 | 0.82 | 22.20 | 190.93 | 48.32 | 298.15 | 0.7865 | -492.0 | -392.2 | |
| 0.00 | 0.94 | 0.00 | 0.75 | 22.10 | 190.74 | 48.13 | 298.10 | 0.7844 | -538.0 | -438.8 | |
| 0.00 | 0.85 | 0.00 | 0.64 | 21.97 | 187.66 | 45.04 | 299.13 | 0.7537 | 443.0 | 368.7 | |
| 0.00 | 1.79 | 0.00 | 1.33 | 22.23 | 187.00 | 44.38 | 299.74 | 0.7480 | 511.0 | 502.1 | |
| 0.00 | 1.11 | 0.00 | 0.82 | 23.61 | 186.00 | 43.38 | 301.92 | 0.7439 | 415.0 | 332.2 | |
| 0.00 | 1.28 | 0.00 | 0.94 | 23.39 | 185.77 | 43.16 | 301.75 | 0.7406 | 575.0 | 517.3 | |
| 0.00 | 1.28 | 0.00 | 0.93 | 23.72 | 185.11 | 42.50 | 302.47 | 0.7355 | 653.0 | 533.2 | |
| 0.00 | 1.79 | 0.00 | 1.33 | 25.04 | 185.49 | 42.88 | 303.94 | 0.7454 | 719.0 | 587.1 | |
| 0.00 | 1.71 | 0.00 | 1.26 | 27.15 | 184.43 | 41.81 | 307.05 | 0.7457 | 686.0 | 593.0 | |
| 0.00 | 0.60 | 0.00 | 0.42 | 26.64 | 181.84 | 39.23 | 307.87 | 0.7184 | 717.0 | 594.7 | |
| 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. | |