SDO HMI 2014-10-03 23:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.84 | 31.04 | 2.51 | 16.33 | -11.90 | 139.59 | -6.10 | 161.83 | 0.3355 | 265.8 | 327.7 | |
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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 | 0.97 | 0.00 | 0.51 | -12.80 | 143.85 | -1.84 | 174.62 | 0.3350 | 763.0 | 616.7 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -11.55 | 141.84 | -3.85 | 168.07 | 0.3194 | 811.0 | 687.7 | |
| 3.78 | 13.01 | 1.96 | 6.76 | -9.96 | 140.37 | -5.32 | 162.19 | 0.3000 | 1223.6 | 797.5 | |
| 0.00 | 1.49 | 0.00 | 0.77 | -9.46 | 140.22 | -5.47 | 161.20 | 0.2929 | 1299.0 | 1030.6 | |
| 1.06 | -3.00 | 0.55 | -3.00 | -9.86 | 140.16 | -5.53 | 161.43 | 0.2997 | 1099.9 | 999999 | |
| 0.00 | 2.81 | 0.00 | 1.52 | -16.18 | 139.85 | -5.84 | 165.80 | 0.4004 | 751.0 | 631.4 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -12.45 | 139.82 | -5.87 | 162.97 | 0.3422 | 798.0 | 667.8 | |
| 0.00 | 2.11 | 0.00 | 1.11 | -11.60 | 139.72 | -5.97 | 161.90 | 0.3293 | 895.0 | 740.2 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -14.37 | 139.12 | -6.57 | 162.76 | 0.3756 | -829.0 | -604.2 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -10.88 | 139.06 | -6.63 | 159.27 | 0.3217 | 580.0 | 551.4 | |
| 0.00 | 2.02 | 0.00 | 1.09 | -15.54 | 138.39 | -7.30 | 161.97 | 0.3971 | -568.0 | -592.8 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -15.35 | 138.37 | -7.32 | 161.76 | 0.3943 | -856.0 | -657.7 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -14.58 | 137.83 | -7.86 | 159.84 | 0.3854 | -870.0 | -683.4 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -12.01 | 135.53 | -10.16 | 151.46 | 0.3627 | -767.0 | -611.6 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -10.63 | 133.87 | -11.82 | 145.58 | 0.3576 | -887.0 | -699.6 | |
| 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. | |