SDO HMI 2014-11-10 13:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.32 | 0.00 | 9.62 | -23.45 | 9.23 | -0.80 | 178.45 | 0.4534 | 748.6 | 647.3 | |
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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 | 1.98 | 0.00 | 1.07 | -20.63 | 10.18 | 0.15 | 180.36 | 0.4086 | 817.0 | 648.7 | |
| 0.00 | 0.95 | 0.00 | 0.52 | -22.30 | 10.11 | 0.09 | 180.19 | 0.4352 | 783.0 | 556.3 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -22.56 | 10.08 | 0.06 | 180.12 | 0.4393 | 688.0 | 606.4 | |
| 0.00 | 1.64 | 0.00 | 0.89 | -21.51 | 10.05 | 0.03 | 180.06 | 0.4227 | 839.0 | 758.4 | |
| 0.00 | 0.60 | 0.00 | 0.33 | -21.90 | 9.47 | -0.55 | 178.81 | 0.4290 | 848.0 | 660.4 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -24.93 | 9.19 | -0.83 | 178.42 | 0.4764 | 662.0 | 575.6 | |
| 0.00 | 1.29 | 0.00 | 0.72 | -24.13 | 9.17 | -0.85 | 178.31 | 0.4640 | 724.0 | 583.6 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -24.36 | 9.13 | -0.89 | 178.26 | 0.4676 | 777.0 | 694.2 | |
| 0.00 | 2.15 | 0.00 | 1.21 | -24.56 | 8.97 | -1.05 | 177.96 | 0.4708 | 852.0 | 774.1 | |
| 0.00 | 1.64 | 0.00 | 0.92 | -24.87 | 8.97 | -1.06 | 177.98 | 0.4755 | 679.0 | 587.3 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -24.19 | 8.94 | -1.08 | 177.87 | 0.4651 | 860.0 | 703.5 | |
| 0.00 | 0.60 | 0.00 | 0.34 | -24.06 | 8.65 | -1.37 | 177.28 | 0.4632 | 866.0 | 758.1 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -24.56 | 8.19 | -1.84 | 176.44 | 0.4714 | 321.0 | 402.3 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -23.86 | 7.81 | -2.22 | 175.58 | 0.4609 | 765.0 | 645.6 | |
| 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. | |