SDO HMI 2014-08-03 03:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.20 | 0.00 | 9.60 | 12.43 | 260.35 | 17.91 | 292.44 | 0.3342 | 433.5 | 271.0 | |
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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 | 1.72 | 0.00 | 0.98 | 12.94 | 271.73 | 29.29 | 285.79 | 0.4975 | -685.0 | -562.9 | |
| 0.00 | 0.36 | 0.00 | 0.20 | 17.05 | 268.54 | 26.10 | 295.75 | 0.4689 | -582.0 | -578.2 | |
| 0.00 | 2.53 | 0.00 | 1.41 | 15.90 | 267.74 | 25.30 | 293.97 | 0.4516 | -868.0 | -689.2 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 7.03 | 260.08 | 17.64 | 274.58 | 0.3031 | 758.0 | 593.8 | |
| 0.00 | 1.90 | 0.00 | 0.99 | 9.57 | 259.78 | 17.34 | 283.05 | 0.3031 | 632.0 | 478.1 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 9.89 | 259.22 | 16.78 | 284.48 | 0.2950 | 647.0 | 534.8 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 9.65 | 259.18 | 16.73 | 283.70 | 0.2935 | 853.0 | 691.4 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 9.35 | 259.16 | 16.72 | 282.69 | 0.2922 | 638.0 | 643.7 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 10.99 | 258.38 | 15.94 | 288.86 | 0.2861 | 761.0 | 663.9 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 17.75 | 257.90 | 15.45 | 309.38 | 0.3298 | 685.0 | 547.5 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 17.65 | 257.06 | 14.62 | 310.61 | 0.3182 | 828.0 | 692.8 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 4.59 | 256.35 | 13.91 | 265.12 | 0.2416 | 859.0 | 634.2 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 20.54 | 249.68 | 7.24 | 335.02 | 0.2805 | 758.0 | 617.5 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 14.80 | 248.87 | 6.43 | 325.05 | 0.1898 | 785.0 | 591.9 | |
| 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. | |