SDO HMI 2014-12-01 08:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.38 | 215.82 | 51.81 | 271.58 | 3.26 | 162.70 | 66.75 | 273.20 | 0.9198 | -315.2 | -105.9 | |
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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 |
| 15.30 | 183.77 | 20.17 | 238.26 | 2.53 | 163.92 | 67.97 | 272.38 | 0.9285 | -487.8 | -132.1 | |
| 20.69 | -1.00 | 26.38 | -1.00 | 3.34 | 163.08 | 67.13 | 273.27 | 0.9230 | -545.8 | 999999 | |
| 0.00 | 1.20 | 0.00 | 1.49 | 2.08 | 162.48 | 66.53 | 271.89 | 0.9189 | -503.0 | -402.4 | |
| 0.00 | 1.03 | 0.00 | 1.27 | 4.36 | 162.41 | 66.46 | 274.38 | 0.9185 | -335.0 | -287.8 | |
| 0.00 | 0.26 | 0.00 | 0.31 | 3.09 | 161.77 | 65.82 | 273.01 | 0.9140 | -605.0 | -585.3 | |
| 0.00 | 4.70 | 0.00 | 5.31 | 3.89 | 159.97 | 64.02 | 273.91 | 0.9008 | -673.0 | -520.6 | |
| 0.00 | 0.94 | 0.00 | 1.06 | 4.40 | 159.77 | 63.83 | 274.48 | 0.8994 | 173.0 | 61.6 | |
| 0.00 | 1.79 | 0.00 | 2.00 | 4.46 | 159.51 | 63.56 | 274.56 | 0.8974 | 474.0 | 304.2 | |
| 0.00 | 0.60 | 0.00 | 0.64 | 3.44 | 158.38 | 62.43 | 273.43 | 0.8884 | 296.0 | 245.0 | |
| 0.00 | 1.88 | 0.00 | 1.95 | 3.42 | 157.42 | 61.48 | 273.43 | 0.8806 | 514.0 | 387.8 | |
| 0.00 | 1.88 | 0.00 | 1.88 | 5.75 | 156.17 | 60.22 | 276.14 | 0.8706 | 520.0 | 400.6 | |
| 5.13 | 16.92 | 5.01 | 16.59 | 6.33 | 155.38 | 59.43 | 276.84 | 0.8640 | 661.6 | 281.2 | |
| 0.00 | 0.85 | 0.00 | 0.82 | 4.17 | 154.98 | 59.03 | 274.34 | 0.8597 | 572.0 | 531.4 | |
| 0.26 | -12.00 | 0.25 | -12.00 | 6.60 | 155.32 | 59.37 | 277.16 | 0.8635 | 552.7 | 999999 | |
| 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. | |