SDO HMI 2014-10-09 18:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.23 | 0.00 | 8.48 | -17.52 | 100.02 | 30.73 | 230.46 | 0.6307 | -234.6 | -190.8 | |
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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 | 0.96 | 0.00 | 0.68 | -13.42 | 110.35 | 41.06 | 244.08 | 0.7127 | 672.0 | 535.9 | |
| 0.00 | 1.14 | 0.00 | 0.82 | -16.02 | 110.20 | 40.91 | 240.69 | 0.7242 | 593.0 | 570.8 | |
| 0.00 | 0.44 | 0.00 | 0.32 | -21.81 | 108.63 | 39.34 | 232.75 | 0.7417 | 531.0 | 562.4 | |
| 0.00 | 2.37 | 0.00 | 1.58 | -15.29 | 105.95 | 36.66 | 238.97 | 0.6745 | 92.0 | 105.6 | |
| 0.00 | 0.70 | 0.00 | 0.44 | -10.01 | 103.30 | 34.01 | 244.59 | 0.6121 | -534.0 | -523.6 | |
| 0.00 | 0.88 | 0.00 | 0.56 | -19.71 | 99.66 | 30.37 | 228.33 | 0.6395 | -611.0 | -482.8 | |
| 0.00 | 1.40 | 0.00 | 0.87 | -18.47 | 97.71 | 28.42 | 228.04 | 0.6092 | -251.0 | -388.4 | |
| 0.00 | 0.70 | 0.00 | 0.42 | -19.67 | 92.79 | 23.50 | 221.22 | 0.5720 | -800.0 | -585.5 | |
| 0.00 | 1.75 | 0.00 | 1.06 | -19.92 | 92.48 | 23.19 | 220.55 | 0.5718 | -771.0 | -607.0 | |
| 0.00 | 1.84 | 0.00 | 1.11 | -19.91 | 92.20 | 22.91 | 220.23 | 0.5690 | -788.0 | -620.6 | |
| 0.00 | 1.05 | 0.00 | 0.62 | -19.66 | 88.68 | 19.40 | 215.96 | 0.5347 | -714.0 | -614.8 | |
| 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. | |