SDO HMI 2014-08-24 21:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 27.12 | 0.00 | 15.03 | -10.07 | 334.86 | 19.94 | 228.98 | 0.4472 | 389.8 | 298.2 | |
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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 | 0.72 | 0.00 | 0.42 | -11.07 | 342.35 | 27.43 | 236.68 | 0.5431 | 541.0 | 477.1 | |
| 0.00 | 0.45 | 0.00 | 0.26 | -11.00 | 342.17 | 27.24 | 236.62 | 0.5403 | 671.0 | 588.2 | |
| 0.00 | 2.51 | 0.00 | 1.48 | -11.11 | 342.01 | 27.08 | 236.28 | 0.5392 | 557.0 | 398.2 | |
| 0.00 | 2.69 | 0.00 | 1.50 | -8.91 | 336.99 | 22.06 | 234.39 | 0.4583 | 664.0 | 554.4 | |
| 0.00 | 1.88 | 0.00 | 1.05 | -9.03 | 336.73 | 21.80 | 233.86 | 0.4561 | 618.0 | 571.0 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -16.53 | 336.91 | 21.98 | 222.53 | 0.5329 | 307.0 | 405.9 | |
| 0.00 | 3.50 | 0.00 | 1.93 | -8.64 | 335.88 | 20.96 | 233.46 | 0.4419 | 656.0 | 742.7 | |
| 0.00 | 1.88 | 0.00 | 1.04 | -9.04 | 335.74 | 20.82 | 232.54 | 0.4440 | 748.0 | 623.2 | |
| 0.00 | 3.86 | 0.00 | 2.16 | -12.17 | 335.27 | 20.34 | 226.60 | 0.4695 | -727.0 | -519.2 | |
| 0.00 | 1.35 | 0.00 | 0.72 | -5.98 | 333.71 | 18.79 | 235.68 | 0.3894 | 812.0 | 626.3 | |
| 0.00 | 1.44 | 0.00 | 0.77 | -6.36 | 333.15 | 18.22 | 234.04 | 0.3856 | 826.0 | 619.9 | |
| 0.00 | 1.62 | 0.00 | 0.85 | -4.39 | 330.04 | 15.12 | 233.32 | 0.3256 | 733.0 | 592.0 | |
| 0.00 | 1.17 | 0.00 | 0.63 | -10.64 | 329.72 | 14.79 | 219.96 | 0.3923 | 863.0 | 692.8 | |
| 0.00 | 1.53 | 0.00 | 0.85 | -16.84 | 328.16 | 13.23 | 208.62 | 0.4593 | -657.0 | -545.4 | |
| 0.00 | 1.62 | 0.00 | 0.85 | -11.41 | 322.60 | 7.67 | 202.55 | 0.3427 | -765.0 | -548.0 | |
| 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. | |