SDO HMI 2014-10-10 07:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.52 | 0.00 | 10.37 | 13.35 | 57.81 | -4.33 | 211.31 | 0.1805 | 45.8 | 33.6 | |
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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 | 1.14 | 0.00 | 0.58 | 17.27 | 68.47 | 6.34 | 331.30 | 0.2205 | -657.0 | -571.9 | |
| 0.00 | 2.54 | 0.00 | 1.27 | 12.63 | 65.62 | 3.48 | 332.12 | 0.1274 | -750.0 | -679.6 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 21.30 | 64.15 | 2.02 | 352.82 | 0.2638 | -825.0 | -655.2 | |
| 0.00 | 1.40 | 0.00 | 0.70 | 10.66 | 63.49 | 1.35 | 343.36 | 0.0814 | -902.0 | -684.1 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 14.82 | 63.02 | 0.89 | 354.30 | 0.1512 | -880.0 | -730.0 | |
| 0.00 | 2.28 | 0.00 | 1.14 | 14.52 | 62.77 | 0.64 | 355.75 | 0.1456 | -889.0 | -734.8 | |
| 0.00 | 1.58 | 0.00 | 0.79 | 11.89 | 58.23 | -3.90 | 33.89 | 0.1200 | 909.0 | 702.9 | |
| 0.00 | 1.32 | 0.00 | 0.66 | 13.49 | 55.21 | -6.93 | 42.61 | 0.1740 | 872.0 | 685.9 | |
| 0.00 | 1.58 | 0.00 | 0.80 | 11.56 | 53.01 | -9.13 | 58.67 | 0.1828 | 869.0 | 668.3 | |
| 0.00 | 1.23 | 0.00 | 0.63 | 14.51 | 51.11 | -11.03 | 51.67 | 0.2371 | 817.0 | 653.4 | |
| 0.00 | 2.72 | 0.00 | 1.38 | 10.79 | 50.49 | -11.65 | 67.50 | 0.2156 | 826.0 | 671.0 | |
| 0.00 | 1.49 | 0.00 | 0.76 | 12.11 | 50.40 | -11.73 | 62.13 | 0.2259 | 495.0 | 384.2 | |
| 0.00 | 1.40 | 0.00 | 0.72 | 14.45 | 49.44 | -12.70 | 55.58 | 0.2592 | 710.0 | 471.7 | |
| 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. | |