SDO HMI 2014-04-01 02:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.96 | 0.00 | 9.58 | -16.10 | 125.26 | 42.42 | 252.48 | 0.6732 | 113.4 | 111.9 | |
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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 | 1.40 | 0.00 | 1.13 | -7.78 | 135.31 | 52.48 | 265.23 | 0.7908 | 548.0 | 456.6 | |
| 0.00 | 1.32 | 0.00 | 1.05 | -16.38 | 134.50 | 51.67 | 254.26 | 0.7842 | 440.0 | 345.5 | |
| 0.00 | 1.14 | 0.00 | 0.90 | -17.30 | 134.15 | 51.31 | 253.04 | 0.7814 | 462.0 | 397.4 | |
| 0.00 | 0.97 | 0.00 | 0.76 | -18.57 | 133.80 | 50.96 | 251.37 | 0.7793 | 514.0 | 447.6 | |
| 0.00 | 0.53 | 0.00 | 0.40 | -15.93 | 132.56 | 49.73 | 254.63 | 0.7632 | 535.0 | 501.3 | |
| 0.00 | 1.32 | 0.00 | 0.99 | -15.96 | 131.85 | 49.01 | 254.51 | 0.7554 | 548.0 | 479.0 | |
| 0.00 | 0.97 | 0.00 | 0.66 | -21.54 | 125.66 | 42.83 | 245.61 | 0.6966 | 501.0 | 378.5 | |
| 0.00 | 1.14 | 0.00 | 0.75 | -19.71 | 123.29 | 40.45 | 247.49 | 0.6635 | 604.0 | 476.2 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -18.78 | 114.62 | 31.78 | 245.45 | 0.5504 | -651.0 | -552.4 | |
| 0.00 | 0.70 | 0.00 | 0.42 | -20.50 | 114.85 | 32.02 | 242.62 | 0.5614 | -513.0 | -411.4 | |
| 0.00 | 2.54 | 0.00 | 1.40 | -10.60 | 108.22 | 25.38 | 259.08 | 0.4309 | -949.0 | -694.6 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -23.67 | 108.49 | 25.66 | 232.48 | 0.5020 | -678.0 | -599.5 | |
| 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. | |