SDO HMI 2014-04-05 20:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.90 | 19.45 | 1.46 | 9.85 | -8.24 | 8.15 | -12.03 | 100.24 | 0.2129 | 96.1 | 70.2 | |
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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 | 1.06 | 0.00 | 0.53 | -3.54 | 11.88 | -8.30 | 72.01 | 0.1521 | 851.0 | 594.8 | |
| 0.00 | 1.41 | 0.00 | 0.71 | -8.06 | 11.44 | -8.74 | 102.10 | 0.1545 | 979.0 | 922.3 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -7.06 | 10.97 | -9.20 | 95.38 | 0.1602 | 787.0 | 618.1 | |
| 0.00 | 1.23 | 0.00 | 0.62 | -7.44 | 10.38 | -9.79 | 97.35 | 0.1709 | 742.0 | 580.2 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -8.96 | 10.16 | -10.02 | 105.74 | 0.1794 | -692.0 | -479.3 | |
| 2.90 | 5.10 | 1.46 | 2.57 | -9.86 | 9.79 | -10.39 | 109.84 | 0.1897 | 1133.6 | 848.8 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -9.82 | 9.33 | -10.85 | 108.92 | 0.1970 | 577.0 | 527.2 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -12.22 | 5.49 | -14.69 | 113.34 | 0.2711 | 750.0 | 602.6 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -7.23 | 5.59 | -14.58 | 94.60 | 0.2517 | -857.0 | -692.6 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -7.18 | 5.00 | -15.18 | 94.30 | 0.2616 | -930.0 | -818.4 | |
| 0.00 | 1.14 | 0.00 | 0.59 | -6.85 | 4.98 | -15.20 | 93.03 | 0.2618 | -822.0 | -697.0 | |
| 0.00 | 2.20 | 0.00 | 1.13 | -6.64 | 3.89 | -16.29 | 92.18 | 0.2800 | -993.0 | -786.3 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -8.85 | 3.48 | -16.69 | 99.86 | 0.2894 | -753.0 | -576.9 | |
| 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. | |