SDO HMI 2014-05-22 22:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.60 | 118.30 | 25.60 | 97.28 | -10.82 | 65.51 | -52.49 | 102.24 | 0.7987 | 612.5 | 241.3 | |
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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 |
| 11.34 | 98.23 | 9.08 | 78.73 | -10.70 | 66.65 | -51.34 | 102.24 | 0.7874 | 894.4 | 287.0 | |
| 9.72 | -1.00 | 7.78 | -1.00 | -10.43 | 66.62 | -51.38 | 101.88 | 0.7874 | 1006.3 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.81 | -12.54 | 65.87 | -52.13 | 104.43 | 0.7979 | 479.0 | 519.1 | |
| 1.62 | -1.00 | 1.31 | -1.00 | -10.88 | 66.26 | -51.74 | 102.41 | 0.7917 | 353.6 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.84 | -14.26 | 64.75 | -53.24 | 106.36 | 0.8115 | 259.0 | 316.2 | |
| 0.00 | 1.08 | 0.00 | 0.91 | -8.92 | 64.16 | -53.84 | 99.73 | 0.8115 | -421.0 | -350.5 | |
| 0.00 | 0.90 | 0.00 | 0.82 | -11.25 | 61.43 | -56.57 | 102.28 | 0.8398 | 337.0 | 275.6 | |
| 4.68 | 9.18 | 4.29 | 8.43 | -11.05 | 61.03 | -56.97 | 102.00 | 0.8433 | 608.8 | 277.9 | |
| 0.27 | -8.00 | 0.25 | -8.00 | -11.23 | 60.75 | -57.25 | 102.19 | 0.8460 | 243.7 | 999999 | |
| 1.62 | 6.93 | 1.57 | 6.74 | -12.80 | 59.08 | -58.92 | 103.84 | 0.8621 | -448.8 | -456.4 | |
| 1.35 | -10.00 | 1.32 | -10.00 | -12.55 | 58.93 | -59.07 | 103.53 | 0.8632 | -406.3 | 999999 | |
| 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. | |