SDO HMI 2014-11-09 15:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.14 | 0.00 | 8.61 | -10.01 | 338.36 | -43.74 | 107.72 | 0.7157 | -23.4 | -63.5 | |
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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 | 0.86 | 0.00 | 0.55 | -9.93 | 344.92 | -37.19 | 110.26 | 0.6370 | 437.0 | 447.5 | |
| 0.00 | 1.03 | 0.00 | 0.68 | -9.89 | 343.54 | -38.56 | 109.56 | 0.6541 | -479.0 | -410.3 | |
| 0.00 | 1.03 | 0.00 | 0.68 | -8.30 | 342.16 | -39.95 | 106.67 | 0.6656 | 488.0 | 475.7 | |
| 0.00 | 0.69 | 0.00 | 0.46 | -9.80 | 341.84 | -40.27 | 108.70 | 0.6748 | 577.0 | 485.8 | |
| 0.00 | 0.86 | 0.00 | 0.56 | -5.73 | 342.27 | -39.83 | 102.92 | 0.6562 | 592.0 | 367.9 | |
| 0.00 | 1.81 | 0.00 | 1.26 | -11.72 | 339.65 | -42.46 | 110.47 | 0.7079 | 539.0 | 436.7 | |
| 0.00 | 0.86 | 0.00 | 0.65 | -11.90 | 335.60 | -46.51 | 109.17 | 0.7539 | -642.0 | -601.2 | |
| 0.00 | 0.86 | 0.00 | 0.65 | -11.54 | 335.32 | -46.78 | 108.62 | 0.7558 | -531.0 | -452.3 | |
| 0.00 | 1.21 | 0.00 | 0.90 | -10.02 | 335.28 | -46.82 | 106.64 | 0.7518 | -559.0 | -562.3 | |
| 0.00 | 1.29 | 0.00 | 0.97 | -9.75 | 335.11 | -46.99 | 106.24 | 0.7530 | -382.0 | -385.2 | |
| 0.00 | 1.64 | 0.00 | 1.25 | -9.74 | 334.04 | -48.07 | 105.90 | 0.7647 | -297.0 | -210.1 | |
| 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. | |