SDO HMI 2014-10-11 04:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.03 | 0.00 | 8.59 | -14.15 | 57.88 | 7.29 | 200.20 | 0.3847 | -16.3 | 211.1 | |
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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 | 0.57 | -14.21 | 64.15 | 13.57 | 213.37 | 0.4151 | 807.0 | 662.7 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -13.23 | 63.08 | 12.50 | 212.60 | 0.3928 | 877.0 | 645.2 | |
| 0.00 | 0.96 | 0.00 | 0.51 | -12.97 | 61.47 | 10.89 | 209.46 | 0.3758 | 855.0 | 670.8 | |
| 0.00 | 1.66 | 0.00 | 0.89 | -13.57 | 61.37 | 10.79 | 208.45 | 0.3835 | 875.0 | 685.7 | |
| 0.00 | 4.73 | 0.00 | 2.52 | -12.74 | 61.15 | 10.56 | 209.03 | 0.3700 | 952.0 | 840.0 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -12.29 | 58.99 | 8.40 | 204.36 | 0.3476 | -1003.0 | -767.5 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -13.01 | 58.92 | 8.33 | 203.33 | 0.3580 | -781.0 | -658.8 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -13.23 | 58.67 | 8.09 | 202.49 | 0.3597 | -781.0 | -561.6 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -15.33 | 48.39 | -2.20 | 174.23 | 0.3697 | -647.0 | -554.0 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -19.57 | 44.86 | -5.73 | 167.76 | 0.4456 | -714.0 | -558.8 | |
| 0.00 | 1.49 | 0.00 | 0.82 | -19.44 | 44.57 | -6.01 | 167.11 | 0.4445 | -619.0 | -440.1 | |
| 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. | |