SDO HMI 2014-12-05 20:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.73 | 0.00 | 9.63 | 13.85 | 16.94 | -19.70 | 54.55 | 0.4052 | -692.6 | -530.7 | |
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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 | 0.43 | 0.00 | 0.22 | 13.07 | 26.06 | -10.58 | 38.99 | 0.2856 | -765.0 | -625.0 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 14.38 | 21.91 | -14.73 | 45.36 | 0.3477 | -828.0 | -649.2 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 17.29 | 20.05 | -16.59 | 43.01 | 0.4014 | -832.0 | -641.3 | |
| 0.00 | 0.60 | 0.00 | 0.31 | 7.49 | 20.05 | -16.59 | 66.13 | 0.3109 | -821.0 | -604.0 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 7.31 | 19.96 | -16.67 | 66.77 | 0.3111 | -863.0 | -636.9 | |
| 0.00 | 1.88 | 0.00 | 1.01 | 13.89 | 18.67 | -17.97 | 51.87 | 0.3824 | -978.0 | -817.1 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 13.65 | 17.95 | -18.68 | 53.43 | 0.3893 | -816.0 | -643.9 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 9.76 | 17.68 | -18.96 | 62.81 | 0.3615 | -934.0 | -781.5 | |
| 0.00 | 1.62 | 0.00 | 0.86 | 9.79 | 17.40 | -19.24 | 63.07 | 0.3659 | -738.0 | -593.8 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 13.22 | 16.90 | -19.74 | 55.77 | 0.3995 | -836.0 | -659.1 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 13.43 | 15.52 | -21.12 | 57.03 | 0.4196 | -690.0 | -448.8 | |
| 0.00 | 0.68 | 0.00 | 0.38 | 16.30 | 14.19 | -22.45 | 53.02 | 0.4606 | -742.0 | -557.8 | |
| 0.00 | 2.56 | 0.00 | 1.44 | 16.79 | 13.09 | -23.55 | 53.39 | 0.4785 | -631.0 | -591.7 | |
| 0.00 | 1.45 | 0.00 | 0.86 | 19.55 | 9.25 | -27.39 | 52.71 | 0.5471 | 778.0 | 595.2 | |
| 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. | |