SDO HMI 2014-06-08 14:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.39 | 0.00 | 10.20 | 4.13 | 260.45 | 2.98 | 230.71 | 0.1370 | 259.4 | 313.9 | |
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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 | 1.36 | 0.00 | 0.70 | 4.45 | 274.00 | 16.53 | 284.62 | 0.2944 | -692.0 | -611.9 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 4.46 | 272.07 | 14.59 | 286.42 | 0.2630 | -999.0 | -837.3 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 4.22 | 271.75 | 14.27 | 285.84 | 0.2567 | -861.0 | -753.9 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 3.71 | 267.34 | 9.87 | 289.58 | 0.1823 | -872.0 | -666.8 | |
| 0.00 | 2.90 | 0.00 | 1.44 | 4.63 | 261.33 | 3.85 | 318.94 | 0.1024 | 761.0 | 656.4 | |
| 0.00 | 4.62 | 0.00 | 2.30 | 5.88 | 259.81 | 2.33 | 337.71 | 0.1071 | 191.0 | 565.2 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 6.50 | 259.60 | 2.12 | 341.41 | 0.1158 | 886.0 | 676.2 | |
| 0.00 | 1.36 | 0.00 | 0.67 | 0.43 | 257.29 | -0.18 | 40.63 | 0.0049 | 870.0 | 549.8 | |
| 0.00 | 0.81 | 0.00 | 0.40 | -1.69 | 256.65 | -0.82 | 156.73 | 0.0366 | 791.0 | 667.0 | |
| 0.00 | 1.18 | 0.00 | 0.58 | -0.23 | 255.16 | -2.31 | 101.10 | 0.0413 | 794.0 | 635.2 | |
| 0.00 | 1.18 | 0.00 | 0.58 | -0.20 | 254.77 | -2.71 | 98.88 | 0.0480 | 860.0 | 746.1 | |
| 0.00 | 1.81 | 0.00 | 0.91 | 9.61 | 252.55 | -4.93 | 27.46 | 0.1846 | 874.0 | 659.7 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 1.33 | 243.09 | -14.39 | 85.53 | 0.2503 | 769.0 | 570.9 | |
| 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. | |