SDO HMI 2014-08-11 20:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.11 | 0.00 | 12.60 | 11.46 | 171.57 | 44.27 | 280.07 | 0.6913 | 5.4 | -64.9 | |
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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 | 1.35 | 0.00 | 1.10 | 13.59 | 180.33 | 53.04 | 282.18 | 0.7968 | -497.0 | -369.5 | |
| 0.00 | 0.45 | 0.00 | 0.36 | 9.50 | 179.18 | 51.88 | 277.02 | 0.7841 | -468.0 | -435.0 | |
| 0.00 | 0.99 | 0.00 | 0.80 | 11.55 | 179.62 | 52.33 | 279.63 | 0.7888 | -366.0 | -380.8 | |
| 0.00 | 2.62 | 0.00 | 2.07 | 12.30 | 178.87 | 51.57 | 280.60 | 0.7809 | -495.0 | -397.6 | |
| 0.00 | 0.72 | 0.00 | 0.57 | 13.26 | 179.15 | 51.85 | 281.83 | 0.7843 | -398.0 | -443.5 | |
| 0.00 | 1.53 | 0.00 | 1.10 | 9.38 | 173.80 | 46.50 | 276.81 | 0.7231 | 654.0 | 518.2 | |
| 0.00 | 1.17 | 0.00 | 0.84 | 9.71 | 173.82 | 46.52 | 277.27 | 0.7233 | 455.0 | 398.5 | |
| 0.00 | 0.90 | 0.00 | 0.64 | 9.27 | 173.56 | 46.26 | 276.67 | 0.7202 | 177.0 | 256.5 | |
| 0.00 | 0.27 | 0.00 | 0.19 | 9.88 | 173.67 | 46.37 | 277.51 | 0.7215 | 339.0 | 336.3 | |
| 0.00 | 0.99 | 0.00 | 0.64 | 7.17 | 167.19 | 39.90 | 273.45 | 0.6398 | 625.0 | 445.8 | |
| 0.00 | 1.08 | 0.00 | 0.66 | 11.12 | 163.04 | 35.75 | 280.09 | 0.5844 | 545.0 | 469.8 | |
| 0.00 | 1.08 | 0.00 | 0.65 | 11.60 | 161.75 | 34.45 | 281.12 | 0.5669 | -607.0 | -538.8 | |
| 0.00 | 2.07 | 0.00 | 1.25 | 13.92 | 162.04 | 34.74 | 285.10 | 0.5751 | 887.0 | 629.1 | |
| 0.00 | 2.89 | 0.00 | 1.73 | 11.90 | 161.41 | 34.12 | 281.71 | 0.5626 | -776.0 | -601.8 | |
| 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. | |