SDO HMI 2011-06-03 15:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.59 | 32.93 | 4.69 | 17.58 | 17.11 | 41.41 | 12.96 | 325.46 | 0.3733 | -98.2 | 78.3 | |
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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 |
| 8.59 | 11.30 | 4.69 | 6.17 | 17.98 | 45.53 | 17.09 | 318.42 | 0.4229 | -1002.0 | -714.8 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 18.23 | 44.79 | 16.34 | 320.07 | 0.4181 | -738.0 | -558.1 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 16.60 | 44.34 | 15.89 | 318.07 | 0.3944 | -520.0 | -416.5 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 16.28 | 44.18 | 15.74 | 317.78 | 0.3890 | -847.0 | -648.2 | |
| 0.00 | 1.90 | 0.00 | 1.01 | 17.20 | 41.70 | 13.25 | 324.08 | 0.3748 | -944.0 | -767.6 | |
| 0.00 | 1.99 | 0.00 | 1.05 | 16.50 | 40.96 | 12.52 | 324.43 | 0.3587 | -836.0 | -661.7 | |
| 0.00 | 1.81 | 0.00 | 0.95 | 16.72 | 38.13 | 9.68 | 331.30 | 0.3369 | 948.0 | 657.8 | |
| 0.00 | 1.17 | 0.00 | 0.62 | 16.72 | 37.71 | 9.26 | 332.35 | 0.3337 | 653.0 | 522.6 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 16.75 | 37.39 | 8.94 | 333.20 | 0.3317 | 791.0 | 671.6 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 16.59 | 37.29 | 8.84 | 333.24 | 0.3286 | 690.0 | 549.5 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 16.46 | 36.83 | 8.39 | 334.25 | 0.3234 | 910.0 | 718.1 | |
| 0.00 | 3.98 | 0.00 | 2.08 | 16.24 | 36.57 | 8.12 | 334.65 | 0.3182 | 879.0 | 655.6 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 16.27 | 36.22 | 7.77 | 335.65 | 0.3162 | 875.0 | 662.5 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 16.30 | 35.77 | 7.32 | 336.94 | 0.3137 | 1101.0 | 866.8 | |
| 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. | |