SDO HMI 2014-04-05 23:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.17 | 431.31 | 40.01 | 226.64 | 12.53 | 13.64 | -4.88 | 14.48 | 0.3341 | -984.0 | -386.3 | |
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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 |
| 73.70 | 410.55 | 38.72 | 215.81 | 12.59 | 13.79 | -4.73 | 13.98 | 0.3343 | -1378.9 | -422.1 | |
| 1.85 | -1.00 | 0.97 | -1.00 | 13.16 | 13.35 | -5.17 | 14.78 | 0.3453 | -807.9 | 999999 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 3.79 | 12.89 | -5.63 | 29.30 | 0.2009 | 812.0 | 609.1 | |
| 0.62 | -1.00 | 0.32 | -1.00 | 12.86 | 12.52 | -6.00 | 17.29 | 0.3442 | -728.0 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.41 | 11.43 | 12.49 | -6.03 | 18.72 | 0.3221 | -731.0 | -537.3 | |
| 0.00 | 0.35 | 0.00 | 0.18 | 11.81 | 12.45 | -6.07 | 18.46 | 0.3282 | -442.0 | -469.0 | |
| 0.00 | 2.11 | 0.00 | 1.09 | 9.72 | 12.09 | -6.42 | 21.86 | 0.2975 | 771.0 | 571.2 | |
| 0.00 | 1.50 | 0.00 | 0.78 | 11.82 | 11.99 | -6.53 | 19.75 | 0.3308 | -697.0 | -561.4 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 10.09 | 12.00 | -6.52 | 21.69 | 0.3039 | 839.0 | 614.3 | |
| 0.00 | 2.90 | 0.00 | 1.53 | 12.33 | 11.79 | -6.73 | 19.77 | 0.3398 | -481.0 | -393.0 | |
| 0.00 | 2.99 | 0.00 | 1.57 | 12.05 | 11.55 | -6.97 | 20.72 | 0.3368 | -589.0 | -485.3 | |
| 0.00 | 1.76 | 0.00 | 0.92 | 11.45 | 11.38 | -7.14 | 21.85 | 0.3286 | 783.0 | 673.2 | |
| 0.00 | 2.64 | 0.00 | 1.38 | 11.55 | 11.04 | -7.48 | 22.67 | 0.3323 | 840.0 | 649.2 | |
| 0.00 | 1.76 | 0.00 | 0.93 | 11.81 | 10.60 | -7.92 | 23.54 | 0.3391 | 980.0 | 853.4 | |
| 0.00 | 1.50 | 0.00 | 0.78 | 9.36 | 9.34 | -9.18 | 30.41 | 0.3123 | 892.0 | 667.2 | |
| 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. | |