SDO HMI 2014-05-27 00:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.20 | 71.42 | 37.27 | 130.48 | -14.36 | 137.81 | 73.84 | 255.42 | 0.9621 | 272.4 | 89.0 | |
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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 | 1.71 | 0.00 | 3.57 | -14.08 | 140.09 | 76.13 | 255.81 | 0.9723 | -387.0 | -315.0 | |
| 3.79 | 48.34 | 7.55 | 94.16 | -14.41 | 139.39 | 75.42 | 255.45 | 0.9695 | 63.1 | 166.2 | |
| 12.90 | -2.00 | 24.43 | -2.00 | -14.49 | 138.60 | 74.63 | 255.33 | 0.9662 | 586.9 | 999999 | |
| 0.00 | 2.53 | 0.00 | 3.96 | -13.74 | 135.36 | 71.39 | 255.94 | 0.9504 | -235.0 | -104.4 | |
| 0.00 | 0.27 | 0.00 | 0.43 | -13.90 | 135.47 | 71.50 | 255.79 | 0.9510 | -233.0 | -124.7 | |
| 1.98 | 3.97 | 3.00 | 6.00 | -13.48 | 134.59 | 70.62 | 256.18 | 0.9461 | -213.5 | -108.8 | |
| 0.00 | 1.08 | 0.00 | 1.70 | -14.78 | 135.25 | 71.28 | 254.85 | 0.9501 | 309.0 | 266.2 | |
| 0.90 | 9.38 | 1.39 | 14.63 | -14.53 | 134.96 | 70.99 | 255.09 | 0.9485 | -180.1 | 92.5 | |
| 0.00 | 0.99 | 0.00 | 1.46 | -13.45 | 134.10 | 70.13 | 256.17 | 0.9434 | -260.0 | -264.7 | |
| 0.00 | 0.63 | 0.00 | 0.92 | -13.52 | 133.77 | 69.81 | 256.08 | 0.9416 | -414.0 | -416.7 | |
| 0.00 | 0.81 | 0.00 | 1.19 | -13.74 | 133.92 | 69.95 | 255.86 | 0.9425 | -275.0 | -279.8 | |
| 0.63 | 1.71 | 0.90 | 2.46 | -13.59 | 133.46 | 69.49 | 255.98 | 0.9398 | -409.6 | -451.5 | |
| 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. | |