SDO HMI 2014-12-02 02:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.02 | 387.03 | 36.66 | 217.98 | 16.66 | 110.02 | 23.97 | 305.24 | 0.4786 | -1006.6 | -346.5 | |
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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 |
| 65.02 | 372.84 | 36.66 | 210.19 | 16.63 | 110.17 | 24.12 | 305.01 | 0.4801 | -1447.3 | -388.0 | |
| 0.00 | 0.68 | 0.00 | 0.38 | 16.85 | 108.48 | 22.43 | 307.27 | 0.4609 | -691.0 | -560.5 | |
| 0.00 | 1.28 | 0.00 | 0.71 | 16.67 | 107.46 | 21.41 | 308.16 | 0.4467 | 670.0 | 533.4 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 17.42 | 107.15 | 21.11 | 309.90 | 0.4497 | 779.0 | 638.6 | |
| 0.00 | 1.88 | 0.00 | 1.04 | 17.63 | 106.91 | 20.87 | 310.59 | 0.4489 | 662.0 | 561.2 | |
| 0.00 | 2.14 | 0.00 | 1.18 | 17.97 | 106.82 | 20.78 | 311.31 | 0.4511 | 710.0 | 646.6 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 17.60 | 106.74 | 20.70 | 310.76 | 0.4466 | 773.0 | 711.6 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 17.48 | 106.56 | 20.52 | 310.77 | 0.4433 | 797.0 | 726.1 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 17.40 | 104.35 | 18.31 | 313.74 | 0.4166 | 883.0 | 753.7 | |
| 0.00 | 2.31 | 0.00 | 1.25 | 17.56 | 103.98 | 17.93 | 314.59 | 0.4139 | 792.0 | 634.1 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 16.11 | 103.19 | 17.14 | 313.11 | 0.3896 | 716.0 | 507.1 | |
| 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. | |