SDO HMI 2014-10-04 15:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.32 | 370.03 | 38.03 | 194.51 | -1.39 | 154.71 | 17.80 | 246.48 | 0.3347 | 1009.8 | 395.2 | |
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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 |
| 61.52 | 308.67 | 32.39 | 162.60 | -1.41 | 155.07 | 18.16 | 246.94 | 0.3401 | 1401.3 | 394.3 | |
| 3.60 | 22.15 | 1.89 | 11.59 | -1.91 | 153.94 | 17.03 | 244.12 | 0.3268 | 941.4 | 662.1 | |
| 1.58 | -2.00 | 0.83 | -2.00 | -1.70 | 153.81 | 16.90 | 244.54 | 0.3233 | 1169.5 | 999999 | |
| 0.00 | 1.85 | 0.00 | 0.96 | -0.48 | 153.75 | 16.83 | 247.93 | 0.3139 | 951.0 | 719.2 | |
| 0.00 | 8.88 | 0.00 | 4.63 | -1.08 | 153.62 | 16.71 | 246.02 | 0.3160 | 848.0 | 820.4 | |
| 0.00 | 2.90 | 0.00 | 1.51 | -1.32 | 153.34 | 16.43 | 244.96 | 0.3135 | 249.0 | 261.4 | |
| 5.62 | 13.27 | 2.92 | 6.89 | -0.25 | 153.09 | 16.18 | 247.79 | 0.3023 | 1145.8 | 771.9 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -3.31 | 153.11 | 16.20 | 239.12 | 0.3260 | 811.0 | 671.5 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 0.69 | 152.00 | 15.09 | 249.36 | 0.2794 | 644.0 | 530.8 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -2.34 | 150.31 | 13.39 | 236.82 | 0.2778 | -765.0 | -600.5 | |
| 0.00 | 2.29 | 0.00 | 1.18 | -2.31 | 150.06 | 13.15 | 236.43 | 0.2740 | -977.0 | -827.6 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -1.54 | 149.81 | 12.90 | 238.31 | 0.2634 | -1034.0 | -821.2 | |
| 0.00 | 1.49 | 0.00 | 0.77 | -1.72 | 149.75 | 12.84 | 237.61 | 0.2642 | -971.0 | -860.8 | |
| 0.00 | 2.99 | 0.00 | 1.53 | -1.84 | 149.66 | 12.74 | 237.04 | 0.2640 | -829.0 | -682.7 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -1.70 | 147.70 | 10.78 | 232.91 | 0.2355 | -901.0 | -678.8 | |
| 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. | |