SDO HMI 2014-03-25 08:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.16 | 0.00 | 11.01 | -15.20 | 128.83 | -43.04 | 104.66 | 0.6821 | 522.9 | 417.4 | |
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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 | 0.79 | 0.00 | 0.51 | -14.79 | 132.04 | -39.83 | 104.89 | 0.6432 | 806.0 | 751.2 | |
| 0.00 | 1.92 | 0.00 | 1.25 | -15.11 | 131.52 | -40.35 | 105.30 | 0.6504 | 600.0 | 535.3 | |
| 0.00 | 1.22 | 0.00 | 0.80 | -15.44 | 131.40 | -40.47 | 105.77 | 0.6524 | 704.0 | 624.1 | |
| 0.00 | 1.22 | 0.00 | 0.80 | -15.22 | 131.25 | -40.62 | 105.40 | 0.6540 | 648.0 | 499.0 | |
| 0.00 | 1.05 | 0.00 | 0.67 | -9.49 | 132.01 | -39.87 | 96.61 | 0.6388 | 574.0 | 420.2 | |
| 0.00 | 1.14 | 0.00 | 0.74 | -11.96 | 131.53 | -40.35 | 100.44 | 0.6463 | 535.0 | 427.0 | |
| 0.00 | 0.70 | 0.00 | 0.46 | -15.48 | 130.74 | -41.14 | 105.71 | 0.6609 | 450.0 | 363.8 | |
| 0.00 | 1.14 | 0.00 | 0.74 | -12.68 | 131.07 | -40.81 | 101.50 | 0.6530 | 647.0 | 467.2 | |
| 0.00 | 0.96 | 0.00 | 0.63 | -8.31 | 131.13 | -40.75 | 94.78 | 0.6504 | 602.0 | 529.3 | |
| 0.00 | 0.87 | 0.00 | 0.58 | -13.35 | 129.53 | -42.35 | 102.33 | 0.6732 | 671.0 | 427.8 | |
| 0.00 | 1.92 | 0.00 | 1.29 | -13.19 | 129.48 | -42.40 | 102.09 | 0.6737 | 601.0 | 465.0 | |
| 0.00 | 0.70 | 0.00 | 0.48 | -13.08 | 128.15 | -43.72 | 101.80 | 0.6901 | 529.0 | 434.4 | |
| 0.00 | 1.22 | 0.00 | 0.91 | -21.17 | 124.41 | -47.47 | 112.41 | 0.7456 | 514.0 | 397.7 | |
| 0.00 | 0.35 | 0.00 | 0.27 | -24.15 | 122.55 | -49.32 | 115.84 | 0.7712 | 452.0 | 429.0 | |
| 0.00 | 0.96 | 0.00 | 0.88 | -25.69 | 114.89 | -56.99 | 116.19 | 0.8443 | -489.0 | -374.5 | |
| 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. | |