SDO HMI 2014-09-06 06:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.58 | 0.00 | 9.96 | 11.53 | 177.95 | 26.49 | 285.13 | 0.4499 | -89.9 | -32.8 | |
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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 | 1.25 | 0.00 | 0.77 | 7.08 | 188.54 | 37.08 | 272.14 | 0.6010 | -656.0 | -543.6 | |
| 0.00 | 1.25 | 0.00 | 0.77 | 10.97 | 187.67 | 36.21 | 278.71 | 0.5889 | -434.0 | -461.9 | |
| 0.00 | 1.34 | 0.00 | 0.82 | 11.09 | 187.65 | 36.19 | 278.92 | 0.5887 | -253.0 | -344.5 | |
| 0.00 | 0.98 | 0.00 | 0.60 | 12.83 | 187.69 | 36.23 | 281.86 | 0.5911 | -642.0 | -505.2 | |
| 0.00 | 1.07 | 0.00 | 0.65 | 10.99 | 187.37 | 35.91 | 278.78 | 0.5847 | -593.0 | -535.6 | |
| 0.00 | 0.80 | 0.00 | 0.49 | 11.00 | 187.22 | 35.76 | 278.81 | 0.5826 | -636.0 | -558.2 | |
| 0.00 | 0.89 | 0.00 | 0.54 | 11.51 | 186.91 | 35.45 | 279.72 | 0.5788 | -662.0 | -571.8 | |
| 0.00 | 0.89 | 0.00 | 0.54 | 11.07 | 186.77 | 35.31 | 278.96 | 0.5764 | -761.0 | -616.1 | |
| 0.00 | 1.16 | 0.00 | 0.70 | 11.55 | 186.01 | 34.55 | 279.88 | 0.5662 | -684.0 | -515.4 | |
| 0.00 | 1.07 | 0.00 | 0.56 | 2.45 | 169.24 | 17.78 | 255.74 | 0.3162 | 955.0 | 774.9 | |
| 0.00 | 1.07 | 0.00 | 0.55 | 12.17 | 164.90 | 13.44 | 291.44 | 0.2452 | 756.0 | 580.5 | |
| 0.00 | 3.13 | 0.00 | 1.60 | 11.97 | 164.73 | 13.27 | 290.85 | 0.2414 | 867.0 | 698.8 | |
| 0.00 | 1.61 | 0.00 | 0.83 | 18.60 | 162.24 | 10.78 | 318.31 | 0.2677 | 656.0 | 548.6 | |
| 0.00 | 1.07 | 0.00 | 0.54 | 16.02 | 161.09 | 9.63 | 313.79 | 0.2238 | 828.0 | 622.5 | |
| 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. | |