SDO HMI 2014-12-06 08:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.14 | 0.00 | 12.35 | 14.64 | 14.76 | -15.29 | 45.61 | 0.3571 | -357.2 | -358.4 | |
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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 | 0.85 | 0.00 | 0.44 | 13.95 | 23.54 | -6.52 | 24.89 | 0.2629 | -721.0 | -558.9 | |
| 0.00 | 3.16 | 0.00 | 1.60 | 8.36 | 20.13 | -9.93 | 50.30 | 0.2227 | -821.0 | -734.2 | |
| 0.00 | 0.77 | 0.00 | 0.40 | 13.32 | 19.19 | -10.86 | 38.97 | 0.2929 | -768.0 | -684.1 | |
| 0.00 | 3.33 | 0.00 | 1.71 | 10.00 | 17.91 | -12.14 | 50.63 | 0.2692 | -1110.0 | -953.9 | |
| 0.00 | 1.37 | 0.00 | 0.70 | 9.76 | 17.49 | -12.56 | 52.27 | 0.2723 | -781.0 | -691.8 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 13.35 | 16.99 | -13.07 | 44.07 | 0.3177 | -1019.0 | -850.9 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 11.66 | 16.89 | -13.17 | 48.36 | 0.2999 | -748.0 | -603.8 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 15.70 | 16.50 | -13.55 | 40.20 | 0.3511 | -796.0 | -642.2 | |
| 0.00 | 0.43 | 0.00 | 0.23 | 20.29 | 15.46 | -14.60 | 34.55 | 0.4186 | -395.0 | -399.0 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 20.04 | 15.38 | -14.67 | 35.05 | 0.4161 | -840.0 | -692.3 | |
| 0.00 | 2.65 | 0.00 | 1.43 | 16.65 | 13.14 | -16.91 | 44.56 | 0.3990 | -497.0 | -490.8 | |
| 0.00 | 1.88 | 0.00 | 1.05 | 19.70 | 9.59 | -20.47 | 44.62 | 0.4707 | 814.0 | 650.6 | |
| 0.00 | 1.37 | 0.00 | 0.76 | 18.17 | 9.38 | -20.67 | 47.40 | 0.4576 | 866.0 | 683.2 | |
| 0.00 | 1.19 | 0.00 | 0.71 | 21.85 | 4.46 | -25.59 | 47.38 | 0.5470 | 694.0 | 572.1 | |
| 0.00 | 1.19 | 0.00 | 0.70 | 19.92 | 4.74 | -25.31 | 49.99 | 0.5270 | 764.0 | 604.1 | |
| 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. | |