SDO HMI 2014-10-09 03:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 11.57 | 0.00 | 7.12 | -15.85 | 105.81 | 28.29 | 230.51 | 0.5924 | -77.6 | 125.9 | |
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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 | 0.70 | 0.00 | 0.47 | -15.98 | 113.42 | 35.90 | 237.50 | 0.6707 | -563.0 | -478.9 | |
| 0.00 | 2.54 | 0.00 | 1.60 | -13.38 | 110.32 | 32.80 | 238.76 | 0.6187 | 647.0 | 502.4 | |
| 0.00 | 0.79 | 0.00 | 0.51 | -16.63 | 110.55 | 33.03 | 234.50 | 0.6439 | 735.0 | 640.0 | |
| 0.00 | 1.40 | 0.00 | 0.88 | -13.42 | 109.96 | 32.44 | 238.42 | 0.6148 | 746.0 | 634.8 | |
| 0.00 | 0.79 | 0.00 | 0.49 | -13.29 | 109.76 | 32.24 | 238.46 | 0.6114 | 750.0 | 649.6 | |
| 0.00 | 1.23 | 0.00 | 0.81 | -22.39 | 108.37 | 30.85 | 225.51 | 0.6669 | 703.0 | 528.6 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -9.91 | 102.70 | 25.18 | 237.33 | 0.5000 | -698.0 | -557.6 | |
| 0.00 | 0.61 | 0.00 | 0.36 | -15.96 | 100.83 | 23.31 | 225.78 | 0.5329 | -586.0 | -530.4 | |
| 0.00 | 0.53 | 0.00 | 0.31 | -19.03 | 100.07 | 22.55 | 220.81 | 0.5569 | -683.0 | -569.0 | |
| 0.00 | 0.70 | 0.00 | 0.40 | -19.45 | 93.92 | 16.41 | 211.76 | 0.5080 | -697.0 | -593.5 | |
| 0.00 | 0.44 | 0.00 | 0.25 | -19.45 | 92.80 | 15.28 | 209.99 | 0.4992 | -547.0 | -492.2 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -19.90 | 88.95 | 11.43 | 202.98 | 0.4792 | -738.0 | -562.9 | |
| 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. | |