SDO HMI 2014-09-13 10:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.64 | 0.00 | 11.30 | -20.40 | 106.75 | 49.92 | 239.50 | 0.8334 | 197.0 | 224.8 | |
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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 | 1.51 | 0.00 | 1.47 | -19.72 | 110.46 | 53.63 | 241.89 | 0.8614 | 321.0 | 325.1 | |
| 0.00 | 1.87 | 0.00 | 1.79 | -19.96 | 109.88 | 53.05 | 241.39 | 0.8576 | 354.0 | 278.1 | |
| 0.00 | 1.16 | 0.00 | 1.08 | -22.47 | 107.74 | 50.91 | 237.76 | 0.8501 | 410.0 | 317.7 | |
| 0.00 | 0.80 | 0.00 | 0.76 | -23.65 | 107.95 | 51.12 | 236.59 | 0.8562 | 412.0 | 375.9 | |
| 0.00 | 0.44 | 0.00 | 0.39 | -20.48 | 106.19 | 49.36 | 239.20 | 0.8297 | 314.0 | 328.4 | |
| 0.00 | 1.25 | 0.00 | 1.09 | -20.18 | 105.86 | 49.03 | 239.38 | 0.8258 | 502.0 | 366.4 | |
| 0.00 | 1.25 | 0.00 | 1.08 | -19.96 | 105.67 | 48.84 | 239.53 | 0.8232 | 340.0 | 376.5 | |
| 0.00 | 1.07 | 0.00 | 0.93 | -20.64 | 105.47 | 48.64 | 238.68 | 0.8244 | 562.0 | 478.5 | |
| 0.00 | 0.89 | 0.00 | 0.77 | -21.07 | 105.07 | 48.24 | 238.01 | 0.8229 | 463.0 | 434.5 | |
| 0.00 | 0.80 | 0.00 | 0.65 | -18.88 | 102.88 | 46.05 | 239.35 | 0.7940 | -348.0 | -349.1 | |
| 0.00 | 0.89 | 0.00 | 0.72 | -18.88 | 102.46 | 45.63 | 239.15 | 0.7902 | -487.0 | -422.2 | |
| 0.00 | 0.71 | 0.00 | 0.57 | -18.92 | 102.20 | 45.37 | 238.96 | 0.7880 | -479.0 | -439.5 | |
| 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. | |