SDO HMI 2014-10-09 19:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.36 | 0.00 | 9.48 | -16.94 | 102.12 | 33.39 | 233.32 | 0.6538 | -92.6 | -64.7 | |
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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 | 1.05 | 0.00 | 0.75 | -13.29 | 110.59 | 41.86 | 244.67 | 0.7208 | 617.0 | 477.5 | |
| 0.00 | 1.14 | 0.00 | 0.81 | -13.42 | 110.33 | 41.59 | 244.36 | 0.7186 | 610.0 | 540.5 | |
| 0.00 | 1.49 | 0.00 | 1.08 | -16.03 | 110.23 | 41.50 | 241.01 | 0.7304 | 679.0 | 566.2 | |
| 0.00 | 0.53 | 0.00 | 0.38 | -16.55 | 110.28 | 41.55 | 240.39 | 0.7336 | 379.0 | 421.8 | |
| 0.00 | 0.96 | 0.00 | 0.68 | -13.99 | 109.38 | 40.65 | 243.12 | 0.7110 | 545.0 | 467.9 | |
| 0.00 | 1.31 | 0.00 | 1.00 | -23.56 | 108.77 | 40.04 | 231.23 | 0.7587 | 84.0 | 162.3 | |
| 0.00 | 0.79 | 0.00 | 0.50 | -9.98 | 103.34 | 34.60 | 245.01 | 0.6193 | -622.0 | -512.4 | |
| 0.00 | 1.31 | 0.00 | 0.81 | -12.48 | 100.70 | 31.96 | 239.46 | 0.6024 | -616.0 | -407.9 | |
| 0.00 | 1.31 | 0.00 | 0.80 | -19.12 | 93.79 | 25.05 | 223.70 | 0.5814 | -504.0 | -527.8 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -19.98 | 92.53 | 23.80 | 221.19 | 0.5780 | -834.0 | -703.8 | |
| 0.00 | 1.75 | 0.00 | 1.06 | -20.00 | 92.22 | 23.49 | 220.80 | 0.5753 | -763.0 | -654.2 | |
| 0.00 | 1.58 | 0.00 | 0.92 | -19.22 | 88.92 | 20.19 | 217.55 | 0.5367 | -686.0 | -507.9 | |
| 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. | |