| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.28 | 87.57 | 26.40 | 71.28 | 16.26 | 298.23 | 51.29 | 289.29 | 0.7956 | -256.0 | -248.9 | |
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back to the solar disc SDO HMI 2011-11-24 20:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.44 | 41.69 | 13.83 | 35.07 | 16.06 | 299.75 | 52.81 | 288.69 | 0.8104 | -756.5 | -394.5 | |
| 0.00 | 1.20 | 0.00 | 0.99 | 15.52 | 299.25 | 52.30 | 288.13 | 0.8045 | -536.0 | -413.4 | |
| 0.00 | 0.68 | 0.00 | 0.56 | 15.28 | 298.81 | 51.87 | 287.93 | 0.7998 | -428.0 | -415.1 | |
| 1.63 | 2.48 | 1.33 | 2.03 | 15.41 | 298.71 | 51.76 | 288.11 | 0.7990 | -429.6 | -408.4 | |
| 6.93 | 12.50 | 5.57 | 10.02 | 15.95 | 297.71 | 50.77 | 288.99 | 0.7900 | 480.4 | -61.7 | |
| 0.00 | 2.14 | 0.00 | 1.69 | 16.24 | 296.84 | 49.90 | 289.56 | 0.7817 | -344.0 | -324.0 | |
| 0.00 | 3.08 | 0.00 | 2.42 | 16.28 | 296.52 | 49.58 | 289.69 | 0.7785 | -632.0 | -481.9 | |
| 0.00 | 1.03 | 0.00 | 0.81 | 16.56 | 296.52 | 49.58 | 290.04 | 0.7791 | -73.0 | -142.9 | |
| 2.23 | 5.05 | 1.74 | 3.95 | 16.10 | 296.32 | 49.38 | 289.51 | 0.7760 | -679.5 | -589.4 | |
| 0.00 | 2.05 | 0.00 | 1.59 | 16.27 | 295.76 | 48.82 | 289.86 | 0.7705 | -753.0 | -624.5 | |
| 0.00 | 1.20 | 0.00 | 0.92 | 16.46 | 295.49 | 48.55 | 290.17 | 0.7681 | -499.0 | -499.1 | |
| 5.05 | 11.04 | 3.93 | 8.59 | 17.59 | 295.75 | 48.81 | 291.55 | 0.7735 | 693.1 | 425.2 | |
| 0.00 | 2.57 | 0.00 | 1.98 | 17.04 | 295.51 | 48.56 | 290.91 | 0.7697 | 595.0 | 377.7 | |
| 0.00 | 0.86 | 0.00 | 0.66 | 17.23 | 295.57 | 48.63 | 291.13 | 0.7708 | 423.0 | 400.0 | |
| 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. | |