SDO HMI 2011-04-29 09:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.12 | 26.73 | 1.65 | 14.04 | -18.25 | 120.95 | -13.70 | 137.25 | 0.3322 | 21.1 | -118.8 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.34 | 0.00 | 0.69 | -17.26 | 125.93 | -8.72 | 147.14 | 0.2680 | 1010.0 | 789.4 | |
| 0.00 | 1.43 | 0.00 | 0.74 | -17.99 | 122.18 | -12.47 | 139.13 | 0.3152 | 721.0 | 535.6 | |
| 0.00 | 1.16 | 0.00 | 0.61 | -18.36 | 122.12 | -12.53 | 139.80 | 0.3204 | 768.0 | 560.3 | |
| 0.00 | 1.60 | 0.00 | 0.84 | -17.46 | 122.15 | -12.50 | 137.89 | 0.3092 | 1072.0 | 871.0 | |
| 0.00 | 2.67 | 0.00 | 1.39 | -17.74 | 122.10 | -12.55 | 138.40 | 0.3131 | 896.0 | 714.5 | |
| 0.00 | 1.69 | 0.00 | 0.88 | -17.41 | 121.37 | -13.27 | 136.13 | 0.3175 | 753.0 | 530.1 | |
| 0.00 | 1.16 | 0.00 | 0.61 | -17.68 | 120.57 | -14.07 | 135.11 | 0.3297 | -611.0 | -466.7 | |
| 0.00 | 4.99 | 0.00 | 2.62 | -17.52 | 120.32 | -14.32 | 134.27 | 0.3309 | -940.0 | -618.6 | |
| 3.12 | 7.75 | 1.65 | 4.11 | -19.48 | 119.99 | -14.66 | 137.81 | 0.3567 | -947.1 | -820.8 | |
| 0.00 | 1.16 | 0.00 | 0.61 | -18.25 | 119.54 | -15.11 | 134.43 | 0.3481 | -869.0 | -572.5 | |
| 0.00 | 1.78 | 0.00 | 0.94 | -18.44 | 119.49 | -15.16 | 134.74 | 0.3507 | -992.0 | -716.7 | |
| 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. | |