SDO HMI 2014-05-29 17:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.61 | 178.76 | 14.34 | 89.64 | -9.04 | 25.12 | -3.04 | 160.20 | 0.1524 | 909.6 | 437.2 | |
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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 | 1.26 | 0.00 | 0.63 | -6.34 | 27.04 | -1.12 | 168.24 | 0.0959 | 869.0 | 609.7 | |
| 0.27 | 158.66 | 0.14 | 79.47 | -8.84 | 25.89 | -2.27 | 164.05 | 0.1430 | 1095.0 | 433.2 | |
| 0.00 | 1.99 | 0.00 | 1.00 | -9.86 | 25.79 | -2.37 | 165.22 | 0.1604 | -9.0 | 16.0 | |
| 28.07 | -2.00 | 14.06 | -2.00 | -9.00 | 25.52 | -2.64 | 161.95 | 0.1474 | 1326.4 | 999999 | |
| 0.27 | -2.00 | 0.14 | -2.00 | -9.30 | 25.36 | -2.80 | 161.62 | 0.1533 | 853.7 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.77 | -10.16 | 23.53 | -4.63 | 153.55 | 0.1791 | 841.0 | 629.7 | |
| 0.00 | 0.90 | 0.00 | 0.45 | -8.78 | 23.33 | -4.82 | 148.53 | 0.1599 | 903.0 | 696.8 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -10.16 | 23.16 | -5.00 | 151.74 | 0.1820 | 805.0 | 630.5 | |
| 0.00 | 3.07 | 0.00 | 1.54 | -9.51 | 23.07 | -5.08 | 149.53 | 0.1731 | 1133.0 | 954.5 | |
| 0.00 | 4.24 | 0.00 | 2.14 | -9.91 | 23.04 | -5.12 | 150.50 | 0.1793 | 1034.0 | 861.0 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -8.74 | 20.46 | -7.70 | 135.59 | 0.1901 | -861.0 | -715.1 | |
| 0.00 | 1.08 | 0.00 | 0.56 | -14.24 | 20.14 | -8.02 | 149.51 | 0.2676 | 887.0 | 619.1 | |
| 0.00 | 0.81 | 0.00 | 0.41 | -9.38 | 20.04 | -8.12 | 136.40 | 0.2029 | -816.0 | -657.9 | |
| 0.00 | 1.53 | 0.00 | 0.78 | -2.04 | 15.36 | -12.79 | 94.90 | 0.2231 | 1043.0 | 870.6 | |
| 0.00 | 1.44 | 0.00 | 0.75 | -11.91 | 13.12 | -15.04 | 126.84 | 0.3186 | -922.0 | -716.4 | |
| 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. | |