SDO HMI 2014-05-26 09:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.75 | 0.00 | 10.08 | -18.63 | 48.75 | -23.50 | 128.74 | 0.4823 | 428.9 | 337.3 | |
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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 | 0.90 | 0.00 | 0.49 | -16.02 | 53.96 | -18.29 | 130.12 | 0.3962 | 770.0 | 591.4 | |
| 0.00 | 2.89 | 0.00 | 1.56 | -15.70 | 53.23 | -19.03 | 128.42 | 0.4023 | 780.0 | 634.5 | |
| 0.00 | 1.35 | 0.00 | 0.73 | -14.97 | 53.06 | -19.19 | 126.71 | 0.3978 | 737.0 | 591.6 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -18.28 | 52.64 | -19.61 | 132.54 | 0.4344 | 824.0 | 588.0 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -18.53 | 52.41 | -19.85 | 132.66 | 0.4396 | 788.0 | 600.5 | |
| 0.00 | 2.62 | 0.00 | 1.46 | -19.45 | 51.19 | -21.07 | 132.64 | 0.4626 | 841.0 | 709.4 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -20.12 | 51.03 | -21.23 | 133.55 | 0.4710 | 826.0 | 660.1 | |
| 0.00 | 0.72 | 0.00 | 0.39 | -14.93 | 51.16 | -21.10 | 124.18 | 0.4222 | 747.0 | 513.5 | |
| 0.00 | 1.71 | 0.00 | 1.02 | -20.26 | 43.23 | -29.03 | 125.68 | 0.5625 | 794.0 | 640.2 | |
| 0.00 | 1.44 | 0.00 | 0.88 | -22.09 | 42.11 | -30.15 | 127.50 | 0.5887 | -707.0 | -532.1 | |
| 0.00 | 1.26 | 0.00 | 0.77 | -20.41 | 41.86 | -30.40 | 124.79 | 0.5797 | -714.0 | -645.2 | |
| 0.00 | 1.53 | 0.00 | 0.93 | -20.95 | 41.73 | -30.52 | 125.52 | 0.5849 | -539.0 | -398.3 | |
| 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. | |