SDO HMI 2014-10-11 23:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.12 | 0.00 | 12.30 | 13.40 | 59.61 | 19.47 | 293.37 | 0.3527 | 19.6 | -12.9 | |
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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 | 4.29 | 0.00 | 2.39 | 11.76 | 66.94 | 26.80 | 283.93 | 0.4567 | -736.0 | -555.4 | |
| 0.00 | 1.84 | 0.00 | 1.02 | 11.98 | 66.59 | 26.45 | 284.56 | 0.4520 | -760.0 | -644.1 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 15.24 | 63.43 | 23.29 | 293.64 | 0.4182 | -726.0 | -616.2 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 17.09 | 63.63 | 23.49 | 297.56 | 0.4315 | -553.0 | -481.3 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 18.53 | 60.63 | 20.49 | 303.70 | 0.4006 | -622.0 | -479.5 | |
| 0.00 | 1.75 | 0.00 | 0.93 | 12.75 | 59.80 | 19.66 | 290.34 | 0.3514 | 885.0 | 761.3 | |
| 0.00 | 2.28 | 0.00 | 1.21 | 16.80 | 59.43 | 19.28 | 301.14 | 0.3710 | -678.0 | -553.3 | |
| 0.00 | 3.50 | 0.00 | 1.81 | 13.20 | 55.23 | 15.09 | 296.60 | 0.2847 | 827.0 | 696.6 | |
| 0.00 | 1.40 | 0.00 | 0.72 | 13.56 | 55.25 | 15.11 | 297.72 | 0.2875 | 892.0 | 679.2 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 13.34 | 54.60 | 14.46 | 297.97 | 0.2763 | 764.0 | 568.2 | |
| 0.00 | 1.49 | 0.00 | 0.76 | 11.14 | 53.63 | 13.49 | 291.55 | 0.2471 | 974.0 | 806.8 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 13.37 | 53.24 | 13.10 | 300.33 | 0.2566 | 780.0 | 640.0 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 9.06 | 46.09 | 5.95 | 296.87 | 0.1153 | -792.0 | -578.4 | |
| 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. | |