SDO HMI 2014-10-10 05:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.79 | 0.00 | 8.78 | -20.76 | 97.00 | 33.77 | 228.99 | 0.6857 | -180.1 | -173.2 | |
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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 | 1.14 | 0.00 | 0.90 | -13.34 | 110.95 | 47.72 | 247.36 | 0.7823 | 442.0 | 407.6 | |
| 0.00 | 0.70 | 0.00 | 0.57 | -21.63 | 108.84 | 45.61 | 236.67 | 0.7973 | 349.0 | 285.5 | |
| 0.00 | 1.14 | 0.00 | 0.93 | -21.91 | 108.58 | 45.35 | 236.22 | 0.7964 | 309.0 | 215.1 | |
| 0.00 | 0.61 | 0.00 | 0.48 | -19.63 | 107.59 | 44.36 | 238.28 | 0.7764 | 576.0 | 477.9 | |
| 0.00 | 0.26 | 0.00 | 0.19 | -19.66 | 101.03 | 37.80 | 234.28 | 0.7133 | -566.0 | -555.0 | |
| 0.00 | 1.93 | 0.00 | 1.25 | -18.93 | 94.96 | 31.73 | 230.53 | 0.6468 | -735.0 | -485.8 | |
| 0.00 | 1.23 | 0.00 | 0.78 | -19.37 | 92.98 | 29.76 | 228.21 | 0.6302 | -651.0 | -463.2 | |
| 0.00 | 1.05 | 0.00 | 0.67 | -19.77 | 92.33 | 29.10 | 227.11 | 0.6271 | -608.0 | -428.7 | |
| 0.00 | 1.84 | 0.00 | 1.13 | -19.32 | 88.95 | 25.72 | 224.21 | 0.5895 | -797.0 | -644.6 | |
| 0.00 | 1.49 | 0.00 | 0.97 | -26.53 | 88.23 | 25.00 | 215.41 | 0.6549 | -229.0 | -308.9 | |
| 0.00 | 1.40 | 0.00 | 0.91 | -27.27 | 86.59 | 23.36 | 212.95 | 0.6504 | -71.0 | -104.8 | |
| 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. | |