SDO HMI 2014-11-30 15:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.13 | 50.41 | 8.01 | 26.64 | -19.17 | 108.46 | 3.17 | 188.59 | 0.3505 | 372.5 | 215.1 | |
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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 |
| 4.36 | 26.32 | 2.31 | 13.94 | -19.31 | 109.76 | 4.47 | 191.97 | 0.3557 | 1059.0 | 557.5 | |
| 0.00 | 1.45 | 0.00 | 0.77 | -19.59 | 109.49 | 4.19 | 191.09 | 0.3594 | 738.0 | 601.3 | |
| 6.41 | -1.00 | 3.39 | -1.00 | -19.37 | 109.35 | 4.06 | 190.88 | 0.3554 | 1050.8 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -17.77 | 108.73 | 3.43 | 190.06 | 0.3276 | 830.0 | 593.2 | |
| 0.43 | 1.62 | 0.23 | 0.86 | -18.84 | 108.68 | 3.39 | 189.38 | 0.3448 | -770.6 | -592.1 | |
| 1.45 | 6.92 | 0.77 | 3.65 | -18.99 | 108.22 | 2.92 | 188.04 | 0.3462 | 1121.2 | 803.6 | |
| 1.03 | 4.02 | 0.54 | 2.11 | -18.14 | 107.77 | 2.47 | 187.14 | 0.3313 | -944.9 | -730.6 | |
| 0.00 | 2.05 | 0.00 | 1.08 | -19.27 | 106.66 | 1.36 | 183.71 | 0.3481 | -931.0 | -663.0 | |
| 0.00 | 1.79 | 0.00 | 0.94 | -18.83 | 106.56 | 1.26 | 183.53 | 0.3408 | -854.0 | -639.2 | |
| 1.45 | 4.10 | 0.77 | 2.16 | -19.21 | 105.15 | -0.14 | 179.61 | 0.3463 | -1009.0 | -822.2 | |
| 0.00 | 1.37 | 0.00 | 0.73 | -20.66 | 105.06 | -0.24 | 179.39 | 0.3702 | 799.0 | 535.6 | |
| 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. | |