SDO HMI 2014-12-06 12:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.99 | 0.00 | 10.90 | -14.78 | 36.37 | 8.50 | 208.19 | 0.2982 | -488.4 | -494.5 | |
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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 | 0.60 | 0.00 | 0.32 | -13.80 | 43.27 | 15.40 | 226.83 | 0.3551 | 816.0 | 566.0 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -20.84 | 43.42 | 15.55 | 214.91 | 0.4396 | -976.0 | -804.4 | |
| 0.00 | 1.28 | 0.00 | 0.67 | -14.92 | 39.60 | 11.73 | 216.99 | 0.3280 | 765.0 | 546.0 | |
| 0.00 | 1.54 | 0.00 | 0.80 | -15.16 | 37.75 | 9.88 | 212.00 | 0.3138 | 778.0 | 702.9 | |
| 0.00 | 0.85 | 0.00 | 0.44 | -13.97 | 36.83 | 8.96 | 211.69 | 0.2890 | -724.0 | -521.4 | |
| 0.00 | 3.24 | 0.00 | 1.67 | -13.08 | 35.76 | 7.89 | 210.17 | 0.2671 | -867.0 | -729.7 | |
| 0.00 | 1.19 | 0.00 | 0.61 | -13.45 | 35.74 | 7.87 | 209.42 | 0.2722 | -843.0 | -674.9 | |
| 0.00 | 2.39 | 0.00 | 1.23 | -14.54 | 35.44 | 7.56 | 206.59 | 0.2860 | -1114.0 | -855.5 | |
| 0.00 | 2.30 | 0.00 | 1.19 | -15.10 | 35.42 | 7.55 | 205.68 | 0.2941 | -563.0 | -580.5 | |
| 0.00 | 1.62 | 0.00 | 0.84 | -15.16 | 35.18 | 7.31 | 204.87 | 0.2933 | -911.0 | -700.6 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -14.70 | 34.95 | 7.08 | 204.86 | 0.2847 | -889.0 | -733.2 | |
| 0.00 | 2.05 | 0.00 | 1.06 | -14.97 | 34.90 | 7.02 | 204.29 | 0.2885 | -883.0 | -715.5 | |
| 0.00 | 1.71 | 0.00 | 0.87 | -13.11 | 31.16 | 3.29 | 193.62 | 0.2380 | -938.0 | -701.0 | |
| 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. | |