SDO HMI 2014-07-18 03:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.07 | 57.01 | 6.82 | 29.79 | 7.07 | 112.66 | 18.57 | 278.44 | 0.3209 | 68.5 | -47.2 | |
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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 | 2.45 | 0.00 | 1.29 | 6.83 | 113.75 | 19.66 | 277.39 | 0.3383 | -922.0 | -773.1 | |
| 1.00 | 22.15 | 0.53 | 11.64 | 7.44 | 113.71 | 19.62 | 279.21 | 0.3388 | -1039.9 | -635.3 | |
| 4.27 | -2.00 | 2.24 | -2.00 | 7.29 | 113.61 | 19.52 | 278.80 | 0.3368 | -973.0 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 6.78 | 113.26 | 19.17 | 277.39 | 0.3302 | -759.0 | -587.4 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 7.16 | 112.76 | 18.67 | 278.71 | 0.3227 | 397.0 | 298.5 | |
| 0.00 | 0.73 | 0.00 | 0.38 | 8.02 | 112.70 | 18.61 | 281.37 | 0.3237 | -592.0 | -489.2 | |
| 0.54 | 1.82 | 0.28 | 0.95 | 7.87 | 112.43 | 18.34 | 281.05 | 0.3190 | -909.0 | -757.9 | |
| 0.00 | 3.27 | 0.00 | 1.71 | 6.78 | 112.38 | 18.29 | 277.63 | 0.3159 | 510.0 | 208.0 | |
| 6.72 | 16.88 | 3.49 | 8.77 | 6.79 | 111.80 | 17.71 | 277.87 | 0.3063 | 1003.8 | 802.7 | |
| 0.00 | 1.82 | 0.00 | 0.94 | 6.55 | 111.76 | 17.67 | 277.09 | 0.3052 | 683.0 | 487.7 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 6.95 | 111.42 | 17.33 | 278.55 | 0.3004 | 653.0 | 543.9 | |
| 0.54 | 3.54 | 0.28 | 1.84 | 6.99 | 111.07 | 16.98 | 278.82 | 0.2947 | 725.5 | 607.6 | |
| 0.00 | 0.36 | 0.00 | 0.19 | 6.88 | 110.68 | 16.59 | 278.60 | 0.2880 | 644.0 | 481.2 | |
| 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. | |