SDO HMI 2014-12-09 09:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.03 | 357.37 | 30.38 | 180.94 | -3.88 | 1.25 | 11.27 | 251.64 | 0.2067 | 1090.4 | 390.2 | |
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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 | 2.39 | 0.00 | 1.23 | -4.96 | 4.95 | 14.97 | 252.00 | 0.2718 | 850.0 | 713.4 | |
| 0.00 | 2.47 | 0.00 | 1.27 | -5.20 | 4.83 | 14.85 | 251.03 | 0.2711 | 1018.0 | 769.0 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -4.84 | 4.79 | 14.81 | 252.25 | 0.2687 | 918.0 | 744.1 | |
| 0.00 | 2.39 | 0.00 | 1.23 | -5.40 | 4.50 | 14.52 | 249.90 | 0.2669 | 874.0 | 589.8 | |
| 31.89 | 333.66 | 16.16 | 168.87 | -3.98 | 1.49 | 11.51 | 251.52 | 0.2109 | 1402.0 | 396.9 | |
| 9.12 | -5.00 | 4.62 | -5.00 | -4.04 | 1.16 | 11.18 | 250.75 | 0.2058 | 1413.4 | 999999 | |
| 0.00 | 3.50 | 0.00 | 1.77 | -2.44 | 1.11 | 11.13 | 258.36 | 0.1979 | 916.0 | 713.4 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -1.70 | 1.02 | 11.04 | 262.02 | 0.1942 | -624.0 | -421.4 | |
| 0.60 | 2.98 | 0.30 | 1.51 | -1.67 | 0.78 | 10.80 | 262.00 | 0.1900 | -1032.7 | -842.6 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -2.35 | 0.78 | 10.80 | 258.48 | 0.1920 | 947.0 | 747.9 | |
| 18.42 | -5.00 | 9.30 | -5.00 | -3.59 | 0.76 | 10.78 | 252.24 | 0.1970 | 1450.0 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.56 | -1.94 | 0.63 | 10.65 | 260.48 | 0.1881 | -855.0 | -613.1 | |
| 0.00 | 2.30 | 0.00 | 1.16 | -5.37 | 359.49 | 9.51 | 241.13 | 0.1887 | 806.0 | 600.9 | |
| 0.00 | 1.88 | 0.00 | 0.95 | -7.30 | 357.90 | 7.92 | 227.75 | 0.1855 | -759.0 | -521.9 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -4.15 | 357.47 | 7.49 | 241.87 | 0.1481 | 793.0 | 619.4 | |
| 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. | |