SDO HMI 2014-01-08 06:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.78 | 0.00 | 9.22 | -19.00 | 68.49 | -25.51 | 126.51 | 0.4843 | -131.6 | -82.9 | |
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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 |
| 0.00 | 1.19 | 0.00 | 0.62 | -19.44 | 82.76 | -11.25 | 145.75 | 0.3282 | 765.0 | 618.1 | |
| 0.00 | 3.31 | 0.00 | 1.74 | -19.51 | 81.76 | -12.24 | 143.65 | 0.3387 | 846.0 | 721.5 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -13.08 | 79.97 | -14.04 | 124.52 | 0.2880 | -937.0 | -800.4 | |
| 0.00 | 1.53 | 0.00 | 0.82 | -13.83 | 74.34 | -19.67 | 118.48 | 0.3735 | -928.0 | -811.6 | |
| 0.00 | 1.10 | 0.00 | 0.61 | -20.18 | 73.55 | -20.46 | 131.02 | 0.4367 | 866.0 | 708.5 | |
| 0.00 | 1.44 | 0.00 | 0.80 | -20.51 | 73.10 | -20.91 | 131.05 | 0.4451 | 804.0 | 601.9 | |
| 0.00 | 2.72 | 0.00 | 1.51 | -12.64 | 68.71 | -25.29 | 110.90 | 0.4482 | -752.0 | -632.2 | |
| 0.00 | 0.68 | 0.00 | 0.47 | -22.93 | 53.33 | -40.68 | 119.67 | 0.6932 | -366.0 | -444.4 | |
| 0.00 | 0.42 | 0.00 | 0.30 | -23.53 | 52.55 | -41.46 | 120.13 | 0.7042 | -596.0 | -525.2 | |
| 0.00 | 1.44 | 0.00 | 1.01 | -23.24 | 52.40 | -41.60 | 119.67 | 0.7046 | -667.0 | -587.7 | |
| 0.00 | 0.93 | 0.00 | 0.81 | -26.92 | 41.66 | -52.35 | 120.46 | 0.8212 | -483.0 | -405.7 | |
| 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. | |