SDO HMI 2014-05-30 21:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.69 | 110.41 | 16.78 | 56.60 | -9.05 | 25.10 | 12.40 | 235.73 | 0.2575 | 926.4 | 521.6 | |
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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 | 0.54 | 0.00 | 0.28 | -6.96 | 26.99 | 14.29 | 246.39 | 0.2685 | 804.0 | 647.2 | |
| 1.90 | 21.04 | 0.98 | 10.83 | -9.13 | 26.40 | 13.70 | 238.25 | 0.2761 | 803.4 | 577.1 | |
| 7.67 | -2.00 | 3.95 | -2.00 | -8.83 | 26.29 | 13.59 | 239.02 | 0.2720 | 1055.9 | 999999 | |
| 1.90 | 69.43 | 0.97 | 35.61 | -9.35 | 25.58 | 12.88 | 236.00 | 0.2665 | 801.7 | 536.2 | |
| 18.87 | -4.00 | 9.68 | -4.00 | -8.98 | 25.38 | 12.68 | 236.78 | 0.2603 | 1260.6 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.69 | -7.21 | 24.61 | 11.90 | 241.47 | 0.2340 | 859.0 | 681.3 | |
| 0.00 | 2.17 | 0.00 | 1.11 | -9.63 | 23.61 | 10.91 | 230.63 | 0.2424 | 998.0 | 839.2 | |
| 0.54 | 3.97 | 0.28 | 2.02 | -9.79 | 23.18 | 10.47 | 229.00 | 0.2384 | 1081.2 | 694.1 | |
| 0.00 | 3.79 | 0.00 | 1.94 | -10.22 | 23.10 | 10.39 | 227.42 | 0.2422 | 858.0 | 656.0 | |
| 1.81 | 3.43 | 0.92 | 1.75 | -10.03 | 22.87 | 10.17 | 227.38 | 0.2373 | 1154.6 | 870.1 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -8.93 | 22.34 | 9.64 | 229.57 | 0.2182 | 862.0 | 656.1 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -8.44 | 20.12 | 7.42 | 223.98 | 0.1848 | -963.0 | -757.8 | |
| 0.00 | 2.17 | 0.00 | 1.09 | -8.56 | 20.00 | 7.30 | 223.05 | 0.1848 | -846.0 | -618.8 | |
| 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. | |