SDO HMI 2014-03-06 05:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.07 | 26.30 | 8.72 | 21.02 | -10.76 | 11.66 | -52.29 | 97.99 | 0.7871 | 220.5 | -30.9 | |
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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 | 0.52 | 0.00 | 0.40 | -10.80 | 12.94 | -51.02 | 98.04 | 0.7734 | 519.0 | 514.7 | |
| 9.43 | 18.00 | 7.42 | 14.17 | -10.30 | 12.42 | -51.53 | 97.40 | 0.7791 | 730.4 | 283.6 | |
| 0.00 | 0.43 | 0.00 | 0.34 | -10.82 | 12.20 | -51.75 | 98.07 | 0.7814 | 548.0 | 487.6 | |
| 1.64 | -2.00 | 1.30 | -2.00 | -10.17 | 12.06 | -51.89 | 97.25 | 0.7830 | 183.7 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.99 | -10.45 | 10.64 | -53.31 | 97.64 | 0.7979 | 316.0 | 239.6 | |
| 0.00 | 1.21 | 0.00 | 1.01 | -12.73 | 9.89 | -54.06 | 100.50 | 0.8054 | -619.0 | -518.3 | |
| 0.00 | 1.12 | 0.00 | 0.93 | -12.07 | 9.89 | -54.07 | 99.67 | 0.8055 | -718.0 | -613.5 | |
| 0.00 | 1.04 | 0.00 | 0.87 | -12.22 | 9.63 | -54.32 | 99.86 | 0.8081 | -513.0 | -465.2 | |
| 0.00 | 1.21 | 0.00 | 1.01 | -11.90 | 9.73 | -54.23 | 99.46 | 0.8071 | -594.0 | -478.4 | |
| 0.00 | 0.87 | 0.00 | 0.72 | -12.05 | 9.68 | -54.27 | 99.64 | 0.8075 | -583.0 | -564.9 | |
| 0.00 | 0.69 | 0.00 | 0.58 | -11.65 | 9.64 | -54.31 | 99.15 | 0.8079 | -107.0 | -253.4 | |
| 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. | |