SDO HMI 2014-10-04 14:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.39 | 0.00 | 8.30 | -18.31 | 103.31 | -34.15 | 127.35 | 0.6703 | 35.4 | -44.0 | |
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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 | 1.05 | 0.00 | 0.63 | -17.16 | 112.79 | -24.68 | 134.50 | 0.5615 | 549.0 | 428.7 | |
| 0.00 | 1.58 | 0.00 | 0.94 | -13.55 | 110.30 | -27.17 | 126.73 | 0.5560 | 443.0 | 343.7 | |
| 0.00 | 1.23 | 0.00 | 0.83 | -24.83 | 107.51 | -29.96 | 138.20 | 0.6822 | 604.0 | 474.4 | |
| 0.00 | 0.88 | 0.00 | 0.59 | -24.63 | 107.37 | -30.09 | 137.86 | 0.6816 | 386.0 | 392.9 | |
| 0.00 | 0.70 | 0.00 | 0.44 | -16.97 | 108.41 | -29.05 | 129.67 | 0.6056 | 733.0 | 581.0 | |
| 0.00 | 0.97 | 0.00 | 0.62 | -18.06 | 106.54 | -30.92 | 129.37 | 0.6343 | 609.0 | 493.1 | |
| 0.00 | 1.41 | 0.00 | 0.98 | -17.25 | 99.08 | -38.38 | 122.65 | 0.7065 | -682.0 | -604.6 | |
| 0.00 | 1.67 | 0.00 | 1.17 | -17.46 | 98.91 | -38.55 | 122.80 | 0.7096 | -516.0 | -532.1 | |
| 0.00 | 0.70 | 0.00 | 0.52 | -21.78 | 97.56 | -39.91 | 127.05 | 0.7487 | -556.0 | -461.0 | |
| 0.00 | 0.79 | 0.00 | 0.56 | -17.41 | 98.72 | -38.74 | 122.61 | 0.7112 | -695.0 | -566.3 | |
| 0.00 | 1.41 | 0.00 | 1.02 | -15.86 | 95.66 | -41.80 | 118.85 | 0.7344 | -486.0 | -364.9 | |
| 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. | |