SDO HMI 2014-11-02 09:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.66 | 27.81 | 3.65 | 15.83 | -17.73 | 98.06 | -19.64 | 139.88 | 0.4925 | -203.2 | -217.4 | |
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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 | 1.13 | 0.00 | 0.62 | -18.98 | 105.55 | -12.15 | 153.13 | 0.4422 | 598.0 | 460.8 | |
| 1.38 | 3.72 | 0.76 | 2.03 | -16.23 | 103.16 | -14.53 | 145.27 | 0.4247 | 1029.1 | 831.0 | |
| 5.28 | 8.14 | 2.89 | 4.45 | -16.23 | 102.87 | -14.82 | 144.75 | 0.4274 | 956.3 | 755.7 | |
| 0.00 | 1.21 | 0.00 | 0.70 | -19.30 | 97.64 | -20.05 | 140.69 | 0.5130 | -725.0 | -645.9 | |
| 0.00 | 0.87 | 0.00 | 0.52 | -23.41 | 95.78 | -21.91 | 143.29 | 0.5751 | -539.0 | -480.1 | |
| 0.00 | 1.56 | 0.00 | 0.91 | -18.07 | 94.25 | -23.44 | 134.68 | 0.5340 | -321.0 | -455.3 | |
| 0.00 | 1.30 | 0.00 | 0.76 | -18.39 | 94.17 | -23.52 | 135.03 | 0.5380 | -591.0 | -595.4 | |
| 0.00 | 1.13 | 0.00 | 0.66 | -17.85 | 94.18 | -23.51 | 134.28 | 0.5325 | -789.0 | -617.9 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -17.53 | 94.06 | -23.64 | 133.68 | 0.5308 | -794.0 | -663.5 | |
| 0.00 | 3.64 | 0.00 | 2.14 | -18.73 | 93.85 | -23.85 | 135.11 | 0.5447 | -770.0 | -660.5 | |
| 0.00 | 0.78 | 0.00 | 0.46 | -17.73 | 93.82 | -23.87 | 133.69 | 0.5352 | -726.0 | -577.6 | |
| 0.00 | 1.99 | 0.00 | 1.20 | -19.44 | 91.79 | -25.91 | 133.77 | 0.5728 | -749.0 | -586.1 | |
| 0.00 | 1.04 | 0.00 | 0.61 | -17.02 | 91.86 | -25.83 | 130.49 | 0.5500 | -822.0 | -549.2 | |
| 0.00 | 0.35 | 0.00 | 0.21 | -19.49 | 91.07 | -26.62 | 133.10 | 0.5807 | -498.0 | -543.0 | |
| 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. | |