SDO HMI 2014-12-05 07:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.34 | 21.09 | 0.18 | 10.89 | -14.33 | 37.26 | -6.52 | 156.39 | 0.2831 | -340.5 | -177.7 | |
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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 | 1.71 | 0.00 | 0.88 | -16.23 | 42.47 | -1.31 | 175.60 | 0.2875 | 1054.0 | 857.2 | |
| 0.00 | 1.54 | 0.00 | 0.80 | -18.09 | 41.46 | -2.32 | 173.06 | 0.3201 | 430.0 | 653.8 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -16.04 | 39.98 | -3.80 | 167.28 | 0.2907 | 1010.0 | 799.8 | |
| 0.00 | 2.30 | 0.00 | 1.18 | -13.14 | 39.70 | -4.08 | 163.45 | 0.2445 | 765.0 | 644.1 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -14.33 | 39.58 | -4.20 | 164.37 | 0.2643 | 686.0 | 573.9 | |
| 0.00 | 1.45 | 0.00 | 0.75 | -14.26 | 37.69 | -6.09 | 157.82 | 0.2737 | -964.0 | -701.8 | |
| 0.34 | 1.71 | 0.18 | 0.88 | -14.29 | 36.67 | -7.11 | 154.63 | 0.2811 | -956.2 | -800.8 | |
| 0.00 | 1.79 | 0.00 | 0.92 | -12.71 | 36.54 | -7.24 | 151.45 | 0.2584 | -798.0 | -614.5 | |
| 0.00 | 1.20 | 0.00 | 0.62 | -13.71 | 35.37 | -8.41 | 149.69 | 0.2827 | -855.0 | -718.6 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -15.09 | 35.01 | -8.77 | 151.05 | 0.3056 | -976.0 | -826.7 | |
| 0.00 | 1.96 | 0.00 | 1.02 | -15.15 | 34.73 | -9.05 | 150.39 | 0.3087 | -1013.0 | -871.3 | |
| 0.00 | 1.37 | 0.00 | 0.71 | -15.18 | 34.54 | -9.24 | 149.94 | 0.3107 | -1028.0 | -806.8 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -15.64 | 34.42 | -9.35 | 150.39 | 0.3182 | -746.0 | -572.8 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -8.17 | 34.18 | -9.60 | 131.89 | 0.2228 | -761.0 | -542.2 | |
| 0.00 | 1.20 | 0.00 | 0.62 | -11.14 | 31.02 | -12.76 | 132.57 | 0.2956 | -845.0 | -642.8 | |
| 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. | |