SDO HMI 2014-05-26 06:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.59 | 0.00 | 7.88 | -19.88 | 48.80 | -25.10 | 129.20 | 0.5124 | 483.6 | 299.5 | |
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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 | 1.62 | 0.00 | 0.89 | -18.02 | 54.99 | -18.91 | 133.04 | 0.4233 | 841.0 | 608.8 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -18.35 | 52.67 | -21.23 | 130.50 | 0.4538 | 874.0 | 652.3 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -18.06 | 52.54 | -21.36 | 129.82 | 0.4528 | 525.0 | 399.9 | |
| 0.00 | 2.16 | 0.00 | 1.22 | -19.46 | 51.83 | -22.07 | 131.37 | 0.4741 | 620.0 | 570.1 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -20.06 | 51.00 | -22.90 | 131.39 | 0.4892 | 627.0 | 522.2 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -19.51 | 51.02 | -22.88 | 130.51 | 0.4840 | 690.0 | 603.4 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -19.80 | 50.83 | -23.07 | 130.77 | 0.4888 | 709.0 | 523.0 | |
| 0.00 | 0.63 | 0.00 | 0.37 | -22.50 | 49.33 | -24.57 | 133.34 | 0.5302 | 582.0 | 471.3 | |
| 0.00 | 0.90 | 0.00 | 0.55 | -20.26 | 43.30 | -30.60 | 124.39 | 0.5808 | 745.0 | 705.4 | |
| 0.00 | 1.71 | 0.00 | 1.06 | -21.74 | 42.58 | -31.32 | 126.04 | 0.5993 | -336.0 | -379.9 | |
| 0.00 | 1.71 | 0.00 | 1.06 | -20.82 | 41.69 | -32.21 | 124.03 | 0.6034 | -557.0 | -476.0 | |
| 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. | |