SDO HMI 2014-05-28 13:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.47 | 33.73 | 7.17 | 22.22 | -10.62 | 83.72 | 40.12 | 254.75 | 0.6576 | 292.5 | 123.9 | |
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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 |
| 10.47 | 17.42 | 7.17 | 11.93 | -9.75 | 86.70 | 43.10 | 257.00 | 0.6934 | 813.4 | 480.7 | |
| 0.00 | 0.90 | 0.00 | 0.60 | -10.42 | 84.22 | 40.63 | 255.42 | 0.6639 | 588.0 | 475.8 | |
| 0.00 | 1.08 | 0.00 | 0.72 | -11.69 | 84.23 | 40.63 | 253.55 | 0.6672 | 602.0 | 529.4 | |
| 0.00 | 0.90 | 0.00 | 0.59 | -11.76 | 83.55 | 39.95 | 253.24 | 0.6588 | 521.0 | 434.1 | |
| 0.00 | 0.90 | 0.00 | 0.59 | -10.74 | 83.30 | 39.70 | 254.69 | 0.6530 | 578.0 | 522.0 | |
| 0.00 | 1.17 | 0.00 | 0.77 | -11.58 | 83.24 | 39.64 | 253.41 | 0.6543 | 644.0 | 532.7 | |
| 0.00 | 0.99 | 0.00 | 0.65 | -12.23 | 83.07 | 39.47 | 252.38 | 0.6540 | 647.0 | 478.0 | |
| 0.00 | 0.99 | 0.00 | 0.64 | -12.21 | 82.02 | 38.42 | 252.05 | 0.6407 | 656.0 | 524.9 | |
| 0.00 | 1.17 | 0.00 | 0.74 | -10.43 | 80.92 | 37.32 | 254.45 | 0.6211 | -624.0 | -457.6 | |
| 0.00 | 0.81 | 0.00 | 0.51 | -10.12 | 80.84 | 37.24 | 254.91 | 0.6192 | -529.0 | -449.7 | |
| 0.00 | 1.44 | 0.00 | 0.90 | -10.22 | 79.92 | 36.32 | 254.45 | 0.6073 | -761.0 | -627.9 | |
| 0.00 | 2.17 | 0.00 | 1.32 | -11.20 | 77.89 | 34.29 | 252.09 | 0.5829 | -144.0 | -241.9 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -9.94 | 77.51 | 33.91 | 254.07 | 0.5736 | -563.0 | -504.8 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -15.90 | 75.18 | 31.58 | 242.87 | 0.5681 | -478.0 | -416.0 | |
| 0.00 | 2.17 | 0.00 | 1.28 | -13.68 | 74.24 | 30.64 | 246.01 | 0.5442 | -778.0 | -630.8 | |
| 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. | |