SDO HMI 2014-06-11 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 10.25 | 0.00 | 6.75 | 5.17 | 263.01 | 40.30 | 278.00 | 0.6465 | 54.6 | 9.0 | |
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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 | 0.27 | 0.00 | 0.21 | 4.23 | 273.30 | 50.59 | 275.02 | 0.7757 | -331.0 | -364.7 | |
| 0.00 | 0.91 | 0.00 | 0.70 | 4.63 | 272.71 | 50.01 | 275.58 | 0.7695 | -516.0 | -465.2 | |
| 0.00 | 0.63 | 0.00 | 0.49 | 4.72 | 272.58 | 49.87 | 275.71 | 0.7681 | -632.0 | -480.6 | |
| 0.00 | 0.72 | 0.00 | 0.54 | 5.41 | 270.96 | 48.26 | 276.75 | 0.7503 | -537.0 | -455.2 | |
| 0.00 | 0.91 | 0.00 | 0.67 | 5.32 | 270.27 | 47.56 | 276.70 | 0.7421 | -545.0 | -496.9 | |
| 0.00 | 1.09 | 0.00 | 0.78 | -0.22 | 268.87 | 46.16 | 269.17 | 0.7237 | -600.0 | -472.2 | |
| 0.00 | 1.09 | 0.00 | 0.66 | 5.35 | 257.82 | 35.11 | 278.48 | 0.5812 | 605.0 | 500.0 | |
| 0.00 | 1.36 | 0.00 | 0.82 | 4.62 | 257.44 | 34.73 | 277.29 | 0.5747 | 558.0 | 434.0 | |
| 0.00 | 0.82 | 0.00 | 0.48 | 9.64 | 254.58 | 31.88 | 287.02 | 0.5466 | 749.0 | 626.6 | |
| 0.00 | 0.91 | 0.00 | 0.53 | 9.33 | 254.37 | 31.66 | 286.56 | 0.5425 | 675.0 | 573.5 | |
| 0.00 | 1.00 | 0.00 | 0.58 | 6.54 | 253.70 | 30.99 | 281.67 | 0.5244 | 565.0 | 358.5 | |
| 0.00 | 0.54 | 0.00 | 0.29 | 4.99 | 244.58 | 21.87 | 281.90 | 0.3808 | 664.0 | 487.5 | |
| 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. | |