SDO HMI 2014-11-13 00:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.40 | 40.53 | 6.82 | 22.36 | 8.89 | 3.24 | 25.66 | 283.97 | 0.4427 | -38.1 | -65.8 | |
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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 |
| 3.79 | 7.06 | 2.12 | 3.95 | 8.13 | 5.12 | 27.53 | 281.54 | 0.4690 | -903.4 | -683.1 | |
| 0.00 | 1.38 | 0.00 | 0.77 | 8.34 | 4.83 | 27.25 | 282.10 | 0.4652 | -855.0 | -696.6 | |
| 0.00 | 4.30 | 0.00 | 2.39 | 8.75 | 4.15 | 26.57 | 283.22 | 0.4560 | -910.0 | -603.9 | |
| 0.00 | 0.52 | 0.00 | 0.29 | 9.26 | 4.13 | 26.54 | 284.33 | 0.4571 | 351.0 | 352.2 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 8.07 | 4.04 | 26.45 | 281.77 | 0.4524 | -817.0 | -555.9 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 8.31 | 4.02 | 26.43 | 282.30 | 0.4528 | -832.0 | -649.7 | |
| 0.00 | 1.46 | 0.00 | 0.81 | 9.20 | 3.99 | 26.40 | 284.26 | 0.4548 | -463.0 | -336.9 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 9.60 | 3.75 | 26.17 | 285.22 | 0.4526 | 478.0 | 300.3 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 9.33 | 3.63 | 26.05 | 284.70 | 0.4498 | -748.0 | -669.8 | |
| 0.00 | 1.29 | 0.00 | 0.71 | 9.75 | 3.50 | 25.91 | 285.68 | 0.4492 | 605.0 | 348.2 | |
| 0.00 | 1.89 | 0.00 | 1.04 | 6.78 | 3.22 | 25.63 | 279.14 | 0.4370 | -868.0 | -682.2 | |
| 8.61 | 17.64 | 4.70 | 9.64 | 9.40 | 1.94 | 24.35 | 285.68 | 0.4244 | 967.6 | 725.2 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 9.67 | 1.76 | 24.18 | 286.41 | 0.4227 | 748.0 | 632.5 | |
| 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. | |