SDO HMI 2011-11-12 19:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.95 | 73.28 | 15.05 | 55.78 | -25.12 | 87.22 | 41.55 | 232.39 | 0.7594 | 182.9 | 72.2 | |
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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 | 0.26 | 0.00 | 0.21 | -25.74 | 91.41 | 45.73 | 234.02 | 0.7994 | -500.0 | -439.0 | |
| 10.84 | 50.84 | 8.39 | 39.47 | -24.95 | 88.55 | 42.88 | 233.42 | 0.7706 | 816.2 | 178.8 | |
| 0.00 | 2.49 | 0.00 | 1.94 | -25.55 | 88.51 | 42.83 | 232.70 | 0.7733 | -158.0 | -60.0 | |
| 1.46 | -2.00 | 1.13 | -2.00 | -25.21 | 88.31 | 42.63 | 232.98 | 0.7697 | 787.8 | 999999 | |
| 2.58 | 4.99 | 1.99 | 3.85 | -25.54 | 88.09 | 42.41 | 232.49 | 0.7696 | 722.5 | 494.4 | |
| 0.00 | 1.12 | 0.00 | 0.84 | -25.12 | 86.77 | 41.09 | 232.21 | 0.7554 | 709.0 | 513.5 | |
| 0.00 | 0.77 | 0.00 | 0.54 | -24.61 | 82.24 | 36.56 | 229.89 | 0.7105 | -564.0 | -452.6 | |
| 0.60 | 2.15 | 0.42 | 1.50 | -25.18 | 81.18 | 35.50 | 228.46 | 0.7044 | -695.1 | -580.6 | |
| 0.00 | 1.55 | 0.00 | 1.09 | -26.31 | 81.57 | 35.89 | 227.44 | 0.7159 | -382.0 | -390.1 | |
| 1.29 | 8.34 | 0.90 | 5.81 | -25.62 | 81.17 | 35.49 | 227.94 | 0.7073 | -728.7 | -722.8 | |
| 2.32 | -10.00 | 1.62 | -10.00 | -25.44 | 81.03 | 35.35 | 228.04 | 0.7048 | -855.8 | 999999 | |
| 0.86 | -10.00 | 0.60 | -10.00 | -25.24 | 80.92 | 35.24 | 228.20 | 0.7024 | -917.1 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.53 | -24.34 | 80.11 | 34.43 | 228.67 | 0.6883 | -669.0 | -582.7 | |
| 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. | |