SDO HMI 2014-12-05 18:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.89 | 290.76 | 28.54 | 181.22 | -3.66 | 0.62 | -37.12 | 96.48 | 0.6084 | 855.3 | 299.8 | |
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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 | 0.94 | 0.00 | 0.56 | -6.17 | 3.76 | -33.99 | 101.40 | 0.5692 | 621.0 | 471.0 | |
| 0.00 | 0.85 | 0.00 | 0.51 | -4.45 | 3.65 | -34.09 | 98.36 | 0.5671 | 688.0 | 573.1 | |
| 0.00 | 1.28 | 0.00 | 0.77 | -6.29 | 3.50 | -34.25 | 101.53 | 0.5731 | 652.0 | 530.2 | |
| 0.00 | 1.28 | 0.00 | 0.78 | -1.79 | 2.42 | -35.32 | 93.54 | 0.5812 | -501.0 | -441.3 | |
| 45.89 | 275.76 | 28.54 | 171.58 | -3.62 | 0.74 | -37.00 | 96.43 | 0.6068 | 1242.2 | 323.0 | |
| 0.00 | 1.36 | 0.00 | 0.87 | -6.95 | 359.37 | -38.38 | 101.50 | 0.6312 | -514.0 | -457.5 | |
| 0.00 | 2.39 | 0.00 | 1.50 | -2.21 | 359.68 | -38.07 | 93.98 | 0.6199 | 604.0 | 463.5 | |
| 0.00 | 1.54 | 0.00 | 0.98 | -4.40 | 358.74 | -39.01 | 97.36 | 0.6351 | 607.0 | 477.4 | |
| 0.00 | 0.85 | 0.00 | 0.55 | -4.46 | 357.93 | -39.82 | 97.32 | 0.6460 | -648.0 | -545.0 | |
| 0.00 | 1.19 | 0.00 | 0.77 | -4.26 | 357.82 | -39.92 | 96.99 | 0.6471 | -738.0 | -608.9 | |
| 0.00 | 2.13 | 0.00 | 1.51 | -5.01 | 352.43 | -45.32 | 97.34 | 0.7165 | -483.0 | -446.6 | |
| 0.00 | 0.68 | 0.00 | 0.48 | -3.95 | 352.52 | -45.23 | 95.86 | 0.7144 | -511.0 | -431.2 | |
| 0.00 | 0.51 | 0.00 | 0.36 | -4.84 | 352.32 | -45.43 | 97.08 | 0.7177 | -557.0 | -454.3 | |
| 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. | |