SDO HMI 2014-07-07 14:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.81 | 17.26 | 1.99 | 12.13 | 11.44 | 278.47 | 44.85 | 282.75 | 0.7109 | -296.4 | -216.4 | |
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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 | 1.27 | 0.00 | 0.94 | 7.27 | 281.48 | 47.86 | 276.59 | 0.7427 | -504.0 | -410.9 | |
| 0.00 | 1.45 | 0.00 | 1.08 | 11.05 | 281.51 | 47.89 | 281.68 | 0.7458 | -591.0 | -497.4 | |
| 0.00 | 1.36 | 0.00 | 0.99 | 7.66 | 280.85 | 47.23 | 277.16 | 0.7355 | -272.0 | -242.8 | |
| 0.00 | 0.27 | 0.00 | 0.19 | 10.81 | 279.28 | 45.66 | 281.64 | 0.7195 | -473.0 | -387.7 | |
| 0.00 | 0.91 | 0.00 | 0.64 | 10.88 | 278.98 | 45.36 | 281.78 | 0.7161 | -536.0 | -369.4 | |
| 2.27 | 4.00 | 1.61 | 2.83 | 11.53 | 278.98 | 45.36 | 282.69 | 0.7169 | -761.3 | -561.7 | |
| 0.00 | 0.91 | 0.00 | 0.64 | 12.79 | 278.59 | 44.97 | 284.50 | 0.7142 | -366.0 | -268.1 | |
| 0.54 | 1.27 | 0.38 | 0.89 | 11.51 | 278.05 | 44.43 | 282.80 | 0.7057 | -679.7 | -605.2 | |
| 0.00 | 0.27 | 0.00 | 0.19 | 12.53 | 278.18 | 44.56 | 284.21 | 0.7088 | -450.0 | -403.3 | |
| 0.00 | 1.36 | 0.00 | 0.95 | 12.41 | 278.11 | 44.49 | 284.05 | 0.7078 | -644.0 | -450.1 | |
| 0.00 | 0.91 | 0.00 | 0.63 | 12.50 | 277.47 | 43.85 | 284.30 | 0.7003 | -457.0 | -364.4 | |
| 0.00 | 0.64 | 0.00 | 0.43 | 12.94 | 275.81 | 42.19 | 285.28 | 0.6807 | 769.0 | 640.3 | |
| 0.00 | 0.64 | 0.00 | 0.42 | 14.22 | 274.87 | 41.24 | 287.39 | 0.6719 | 488.0 | 374.7 | |
| 0.00 | 2.00 | 0.00 | 1.31 | 14.34 | 273.56 | 39.94 | 287.92 | 0.6560 | 756.0 | 569.5 | |
| 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. | |