SDO HMI 2014-12-07 13:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.10 | 352.47 | 28.08 | 179.57 | -3.61 | 1.08 | -13.07 | 105.94 | 0.2359 | 1054.4 | 434.1 | |
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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 | 1.02 | 0.00 | 0.51 | -5.16 | 5.41 | -8.74 | 121.12 | 0.1775 | 744.0 | 607.3 | |
| 0.00 | 1.45 | 0.00 | 0.74 | -6.53 | 2.43 | -11.72 | 119.67 | 0.2333 | -976.0 | -840.3 | |
| 24.31 | 333.97 | 12.37 | 170.12 | -3.80 | 1.45 | -12.70 | 107.12 | 0.2305 | 1464.4 | 446.3 | |
| 0.26 | -3.00 | 0.13 | -3.00 | -3.38 | 1.37 | -12.78 | 105.28 | 0.2300 | 1169.0 | 999999 | |
| 28.83 | -3.00 | 14.70 | -3.00 | -3.50 | 0.82 | -13.33 | 105.17 | 0.2395 | 1358.1 | 999999 | |
| 0.00 | 4.69 | 0.00 | 2.40 | -2.32 | 0.26 | -13.89 | 99.88 | 0.2446 | 891.0 | 728.1 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -1.64 | 0.26 | -13.88 | 97.11 | 0.2428 | 877.0 | 603.7 | |
| 0.85 | 2.64 | 0.44 | 1.35 | -4.72 | 0.06 | -14.08 | 109.00 | 0.2576 | 888.6 | 679.1 | |
| 0.51 | 2.30 | 0.26 | 1.18 | -4.57 | 359.76 | -14.38 | 108.09 | 0.2617 | 778.2 | 542.8 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -1.40 | 359.81 | -14.34 | 95.94 | 0.2501 | -798.0 | -690.1 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -4.42 | 359.61 | -14.53 | 107.38 | 0.2634 | 700.0 | 534.7 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -1.82 | 359.16 | -14.98 | 97.27 | 0.2617 | -786.0 | -641.0 | |
| 0.34 | 2.05 | 0.18 | 1.05 | -1.43 | 358.92 | -15.22 | 95.71 | 0.2650 | -936.0 | -688.3 | |
| 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. | |