SDO HMI 2014-04-06 05:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.51 | 0.00 | 10.19 | -16.93 | 330.52 | -44.70 | 107.67 | 0.7055 | 392.6 | 321.4 | |
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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 | 2.11 | 0.00 | 1.34 | -14.37 | 336.52 | -38.70 | 105.18 | 0.6298 | 69.0 | 90.2 | |
| 0.00 | 0.97 | 0.00 | 0.64 | -14.80 | 333.99 | -41.23 | 105.34 | 0.6630 | 493.0 | 406.1 | |
| 0.00 | 1.23 | 0.00 | 0.83 | -16.92 | 333.20 | -42.02 | 108.32 | 0.6769 | 349.0 | 297.7 | |
| 0.00 | 1.23 | 0.00 | 0.81 | -13.23 | 333.80 | -41.42 | 102.95 | 0.6631 | 682.0 | 521.9 | |
| 0.00 | 0.79 | 0.00 | 0.54 | -17.70 | 332.34 | -42.88 | 109.23 | 0.6889 | 609.0 | 501.6 | |
| 0.00 | 2.46 | 0.00 | 1.69 | -16.78 | 331.65 | -43.57 | 107.77 | 0.6952 | 708.0 | 529.5 | |
| 0.00 | 0.88 | 0.00 | 0.60 | -16.13 | 331.62 | -43.60 | 106.84 | 0.6944 | 312.0 | 267.3 | |
| 0.00 | 1.58 | 0.00 | 1.16 | -19.04 | 328.35 | -46.87 | 110.21 | 0.7375 | 378.0 | 379.4 | |
| 0.00 | 1.41 | 0.00 | 1.03 | -18.70 | 328.38 | -46.84 | 109.76 | 0.7365 | 445.0 | 371.2 | |
| 0.00 | 0.97 | 0.00 | 0.69 | -14.76 | 328.87 | -46.35 | 104.47 | 0.7250 | 560.0 | 493.1 | |
| 0.00 | 0.88 | 0.00 | 0.86 | -23.11 | 315.61 | -59.61 | 113.17 | 0.8650 | -286.0 | -305.4 | |
| 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. | |