SDO HMI 2014-12-02 05:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.24 | 21.44 | 4.40 | 15.92 | -15.37 | 38.67 | -45.74 | 111.75 | 0.7450 | 45.6 | -145.4 | |
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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 | 0.85 | 0.00 | 0.61 | -19.03 | 42.21 | -42.19 | 117.82 | 0.7203 | 437.0 | 334.7 | |
| 5.13 | 7.09 | 3.56 | 4.93 | -16.46 | 42.79 | -41.62 | 114.68 | 0.7033 | 855.5 | 568.3 | |
| 0.00 | 0.26 | 0.00 | 0.19 | -20.00 | 39.36 | -45.05 | 117.80 | 0.7541 | 183.0 | 284.0 | |
| 0.68 | 2.22 | 0.51 | 1.64 | -15.24 | 38.60 | -45.80 | 111.43 | 0.7455 | 649.6 | 481.9 | |
| 0.00 | 1.45 | 0.00 | 1.09 | -15.76 | 38.09 | -46.31 | 111.94 | 0.7526 | 322.0 | 323.3 | |
| 0.43 | 3.67 | 0.33 | 2.84 | -14.43 | 36.22 | -48.19 | 109.64 | 0.7687 | -749.6 | -579.8 | |
| 0.00 | 1.11 | 0.00 | 0.86 | -14.21 | 36.24 | -48.17 | 109.37 | 0.7680 | -435.0 | -478.2 | |
| 0.00 | 1.54 | 0.00 | 1.17 | -12.66 | 36.47 | -47.93 | 107.45 | 0.7616 | -596.0 | -503.7 | |
| 0.00 | 0.34 | 0.00 | 0.27 | -15.20 | 35.66 | -48.74 | 110.45 | 0.7766 | -618.0 | -559.8 | |
| 0.00 | 0.94 | 0.00 | 0.75 | -16.23 | 35.04 | -49.36 | 111.54 | 0.7856 | -489.0 | -437.0 | |
| 0.00 | 1.97 | 0.00 | 1.57 | -13.77 | 34.40 | -50.01 | 108.31 | 0.7861 | -573.0 | -432.7 | |
| 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. | |