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 |
| 45.05 | 95.23 | 24.31 | 51.28 | -19.12 | 107.70 | 11.75 | 209.16 | 0.3946 | 6.8 | -13.9 | |
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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 |
| 0.60 | 1.97 | 0.33 | 1.07 | -19.30 | 110.72 | 14.77 | 214.97 | 0.4217 | 957.7 | 871.6 | |
| 6.15 | 8.03 | 3.36 | 4.39 | -19.65 | 110.59 | 14.64 | 214.24 | 0.4249 | 992.4 | 739.7 | |
| 3.25 | 34.28 | 1.77 | 18.63 | -19.61 | 110.13 | 14.18 | 213.46 | 0.4204 | 1006.3 | 519.9 | |
| 5.56 | -3.00 | 3.02 | -3.00 | -19.29 | 109.68 | 13.74 | 213.08 | 0.4124 | 1137.5 | 999999 | |
| 4.87 | -3.00 | 2.65 | -3.00 | -19.55 | 109.71 | 13.76 | 212.77 | 0.4159 | 1109.6 | 999999 | |
| 2.65 | -3.00 | 1.44 | -3.00 | -19.45 | 109.15 | 13.20 | 211.85 | 0.4099 | 538.9 | 999999 | |
| 0.00 | 1.20 | 0.00 | 0.64 | -17.84 | 108.01 | 12.06 | 211.83 | 0.3787 | -812.0 | -657.6 | |
| 0.00 | 1.71 | 0.00 | 0.92 | -18.22 | 107.81 | 11.86 | 210.88 | 0.3821 | -891.0 | -725.7 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -17.78 | 107.72 | 11.77 | 211.31 | 0.3753 | -706.0 | -626.3 | |
| 3.68 | 8.38 | 1.97 | 4.49 | -18.69 | 107.40 | 11.45 | 209.36 | 0.3851 | 1023.0 | 768.3 | |
| 0.00 | 0.68 | 0.00 | 0.36 | -16.81 | 106.68 | 10.73 | 210.45 | 0.3533 | 534.0 | 405.1 | |
| 0.00 | 2.14 | 0.00 | 1.13 | -17.77 | 106.17 | 10.22 | 207.89 | 0.3628 | -919.0 | -867.5 | |
| 18.29 | 33.59 | 9.77 | 17.94 | -19.15 | 105.20 | 9.25 | 203.95 | 0.3758 | -1128.5 | -726.0 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -16.89 | 103.27 | 7.32 | 201.82 | 0.3297 | -781.0 | -560.0 | |
| 0.00 | 1.20 | 0.00 | 0.63 | -17.08 | 103.22 | 7.27 | 201.45 | 0.3322 | -738.0 | -455.1 | |
| 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. | |