SDO HMI 2014-11-22 09:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.43 | 23.41 | 0.23 | 12.30 | -13.09 | 226.02 | 12.00 | 217.55 | 0.3330 | 48.2 | 18.6 | |
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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 | 1.11 | 0.00 | 0.59 | -9.32 | 232.38 | 18.36 | 238.01 | 0.3681 | -840.0 | -668.9 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -12.77 | 228.86 | 14.84 | 224.57 | 0.3575 | 647.0 | 514.8 | |
| 0.00 | 2.32 | 0.00 | 1.23 | -13.41 | 228.36 | 14.34 | 222.35 | 0.3593 | 674.0 | 534.7 | |
| 0.43 | 1.29 | 0.23 | 0.68 | -13.50 | 227.71 | 13.69 | 220.87 | 0.3532 | 921.4 | 807.0 | |
| 0.00 | 1.29 | 0.00 | 0.68 | -13.22 | 227.60 | 13.58 | 221.18 | 0.3487 | 913.0 | 744.9 | |
| 0.00 | 4.03 | 0.00 | 2.13 | -13.65 | 227.50 | 13.48 | 220.15 | 0.3528 | 759.0 | 738.4 | |
| 0.00 | 0.94 | 0.00 | 0.50 | -12.12 | 227.35 | 13.33 | 222.90 | 0.3327 | 854.0 | 642.0 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -12.48 | 226.94 | 12.92 | 221.25 | 0.3324 | 946.0 | 785.8 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -16.84 | 223.85 | 9.83 | 206.89 | 0.3628 | -711.0 | -565.2 | |
| 0.00 | 0.86 | 0.00 | 0.44 | -11.96 | 223.43 | 9.40 | 213.61 | 0.2901 | -626.0 | -616.8 | |
| 0.00 | 3.00 | 0.00 | 1.57 | -14.05 | 223.35 | 9.33 | 209.70 | 0.3187 | -645.0 | -634.9 | |
| 0.00 | 1.46 | 0.00 | 0.75 | -12.11 | 222.79 | 8.77 | 211.51 | 0.2864 | -821.0 | -745.8 | |
| 0.00 | 2.57 | 0.00 | 1.33 | -12.02 | 222.60 | 8.58 | 211.14 | 0.2834 | -750.0 | -791.2 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -13.77 | 222.63 | 8.61 | 208.21 | 0.3088 | -847.0 | -662.6 | |
| 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. | |