SDO HMI 2014-12-06 10:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.60 | 23.12 | 0.31 | 12.02 | 12.91 | 17.76 | -11.20 | 39.82 | 0.2942 | -705.6 | -557.5 | |
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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 | 1.19 | 0.00 | 0.60 | 10.43 | 27.14 | -1.82 | 10.01 | 0.1811 | -749.0 | -524.5 | |
| 0.00 | 0.85 | 0.00 | 0.44 | 14.82 | 24.51 | -4.45 | 16.56 | 0.2644 | -712.0 | -658.6 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 13.67 | 21.88 | -7.09 | 27.25 | 0.2630 | -782.0 | -599.8 | |
| 0.00 | 1.02 | 0.00 | 0.53 | 13.34 | 21.52 | -7.45 | 29.04 | 0.2609 | -846.0 | -644.9 | |
| 0.00 | 0.43 | 0.00 | 0.22 | 12.97 | 21.32 | -7.65 | 30.42 | 0.2574 | -334.0 | -440.8 | |
| 0.00 | 1.19 | 0.00 | 0.60 | 8.32 | 20.07 | -8.89 | 47.32 | 0.2091 | -778.0 | -667.0 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 13.31 | 19.25 | -9.72 | 35.93 | 0.2812 | -950.0 | -743.0 | |
| 0.60 | 4.01 | 0.31 | 2.05 | 10.08 | 17.96 | -11.01 | 47.63 | 0.2557 | -1098.0 | -847.0 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 9.99 | 17.62 | -11.34 | 48.73 | 0.2589 | -885.0 | -731.8 | |
| 0.00 | 1.62 | 0.00 | 0.84 | 13.37 | 17.02 | -11.94 | 41.48 | 0.3053 | -913.0 | -779.5 | |
| 0.00 | 2.22 | 0.00 | 1.15 | 11.89 | 16.72 | -12.25 | 45.71 | 0.2913 | -772.0 | -660.8 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 15.75 | 16.39 | -12.58 | 38.03 | 0.3417 | -808.0 | -643.9 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 13.49 | 15.40 | -13.57 | 44.79 | 0.3253 | -804.0 | -641.3 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 13.58 | 14.95 | -14.01 | 45.49 | 0.3315 | -848.0 | -640.0 | |
| 0.00 | 2.13 | 0.00 | 1.19 | 19.72 | 9.57 | -19.40 | 43.10 | 0.4595 | 817.0 | 633.6 | |
| 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. | |