SDO HMI 2014-11-11 00:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.68 | 0.00 | 7.03 | 18.37 | 341.35 | -22.60 | 53.93 | 0.4518 | -179.2 | -176.2 | |
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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 | 1.29 | 0.00 | 0.70 | 18.67 | 344.15 | -19.80 | 50.19 | 0.4196 | -939.0 | -724.0 | |
| 0.00 | 1.21 | 0.00 | 0.66 | 18.88 | 344.06 | -19.90 | 49.90 | 0.4228 | -889.0 | -724.8 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 16.40 | 344.27 | -19.68 | 54.65 | 0.3978 | -969.0 | -844.8 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 16.60 | 343.69 | -20.26 | 54.95 | 0.4072 | -861.0 | -678.7 | |
| 0.00 | 1.72 | 0.00 | 0.93 | 16.33 | 343.59 | -20.36 | 55.66 | 0.4062 | -743.0 | -626.5 | |
| 0.00 | 0.78 | 0.00 | 0.42 | 17.17 | 342.86 | -21.09 | 54.78 | 0.4226 | -704.0 | -616.3 | |
| 0.00 | 0.95 | 0.00 | 0.54 | 21.84 | 340.83 | -23.12 | 48.58 | 0.4880 | 648.0 | 528.6 | |
| 0.00 | 0.60 | 0.00 | 0.34 | 22.02 | 340.77 | -23.19 | 48.35 | 0.4905 | 499.0 | 639.0 | |
| 0.00 | 1.21 | 0.00 | 0.67 | 18.13 | 340.41 | -23.54 | 55.60 | 0.4619 | 565.0 | 431.5 | |
| 0.00 | 1.64 | 0.00 | 0.95 | 19.53 | 336.92 | -27.03 | 56.37 | 0.5164 | 824.0 | 633.0 | |
| 0.00 | 0.78 | 0.00 | 0.47 | 18.98 | 331.41 | -32.54 | 61.32 | 0.5821 | 598.0 | 464.2 | |
| 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. | |