SDO HMI 2014-10-06 00:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.50 | 32.58 | 3.71 | 18.31 | 13.70 | 91.64 | -27.11 | 72.96 | 0.4644 | 50.5 | 17.4 | |
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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 | 1.14 | 0.00 | 0.59 | 9.69 | 102.17 | -16.58 | 77.85 | 0.2891 | -662.0 | -549.4 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 10.96 | 100.40 | -18.35 | 74.86 | 0.3216 | -861.0 | -682.3 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 12.91 | 99.23 | -19.52 | 70.06 | 0.3480 | -913.0 | -703.9 | |
| 0.00 | 2.11 | 0.00 | 1.13 | 10.46 | 96.83 | -21.92 | 78.09 | 0.3768 | -628.0 | -573.7 | |
| 0.00 | 1.58 | 0.00 | 0.85 | 10.28 | 96.71 | -22.04 | 78.63 | 0.3783 | -758.0 | -628.2 | |
| 0.00 | 0.70 | 0.00 | 0.38 | 13.41 | 95.84 | -22.91 | 71.15 | 0.4018 | -560.0 | -481.8 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 10.94 | 95.30 | -23.45 | 77.46 | 0.4019 | -674.0 | -576.2 | |
| 0.00 | 4.48 | 0.00 | 2.45 | 14.54 | 94.68 | -24.07 | 69.24 | 0.4240 | -472.0 | -278.4 | |
| 0.00 | 1.05 | 0.00 | 0.61 | 18.82 | 88.89 | -29.86 | 64.20 | 0.5254 | 659.0 | 490.8 | |
| 6.50 | 13.35 | 3.71 | 7.63 | 13.34 | 89.28 | -29.47 | 74.41 | 0.4989 | 1071.6 | 626.3 | |
| 0.00 | 1.23 | 0.00 | 0.71 | 13.39 | 88.03 | -30.72 | 74.73 | 0.5172 | 724.0 | 514.5 | |
| 0.00 | 1.67 | 0.00 | 0.99 | 15.39 | 85.74 | -33.01 | 71.83 | 0.5549 | 208.0 | 286.1 | |
| 0.00 | 1.05 | 0.00 | 0.66 | 22.40 | 83.10 | -35.65 | 61.39 | 0.6160 | 563.0 | 395.6 | |
| 0.00 | 0.79 | 0.00 | 0.49 | 20.80 | 83.55 | -35.20 | 63.67 | 0.6034 | 242.0 | 289.4 | |
| 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. | |