SDO HMI 2014-11-09 19:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.28 | 0.00 | 8.57 | -15.72 | 18.96 | -0.94 | 178.16 | 0.3373 | -56.0 | -116.1 | |
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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 | 1.03 | 0.00 | 0.54 | -14.26 | 26.38 | 6.48 | 199.78 | 0.3249 | 759.0 | 578.7 | |
| 0.00 | 1.29 | 0.00 | 0.67 | -13.59 | 23.58 | 3.68 | 191.99 | 0.3013 | 917.0 | 743.9 | |
| 0.00 | 1.29 | 0.00 | 0.67 | -13.12 | 23.36 | 3.46 | 191.61 | 0.2929 | 1066.0 | 875.3 | |
| 0.00 | 1.64 | 0.00 | 0.85 | -14.55 | 23.25 | 3.35 | 190.37 | 0.3160 | 927.0 | 743.2 | |
| 0.00 | 1.55 | 0.00 | 0.81 | -14.08 | 22.17 | 2.27 | 187.27 | 0.3055 | 966.0 | 750.3 | |
| 0.00 | 1.29 | 0.00 | 0.68 | -16.30 | 17.00 | -2.90 | 171.83 | 0.3433 | -791.0 | -559.6 | |
| 0.00 | 1.72 | 0.00 | 0.90 | -15.45 | 17.01 | -2.89 | 171.49 | 0.3294 | -810.0 | -557.2 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -16.27 | 16.69 | -3.21 | 170.96 | 0.3436 | -822.0 | -720.3 | |
| 0.00 | 3.02 | 0.00 | 1.62 | -18.50 | 15.24 | -4.66 | 168.35 | 0.3836 | -1061.0 | -885.8 | |
| 0.00 | 1.46 | 0.00 | 0.79 | -18.69 | 14.98 | -4.92 | 167.84 | 0.3875 | -914.0 | -760.8 | |
| 0.00 | 0.78 | 0.00 | 0.40 | -12.95 | 12.58 | -7.32 | 156.26 | 0.3098 | -853.0 | -644.4 | |
| 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. | |