SDO HMI 2014-11-11 16:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.73 | 83.60 | 15.36 | 49.92 | -8.74 | 323.29 | -31.90 | 110.89 | 0.5613 | 878.0 | 490.6 | |
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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 | 0.78 | -10.75 | 323.55 | -31.64 | 114.40 | 0.5681 | 715.0 | 614.1 | |
| 0.00 | 0.95 | 0.00 | 0.57 | -12.32 | 323.28 | -31.91 | 116.74 | 0.5805 | 670.0 | 583.0 | |
| 5.17 | 78.35 | 3.07 | 46.75 | -8.62 | 323.60 | -31.59 | 110.88 | 0.5564 | 1246.0 | 488.4 | |
| 11.36 | -3.00 | 6.78 | -3.00 | -8.69 | 323.38 | -31.80 | 110.86 | 0.5597 | 1050.2 | 999999 | |
| 2.32 | -3.00 | 1.39 | -3.00 | -8.96 | 323.22 | -31.97 | 111.23 | 0.5633 | 695.1 | 999999 | |
| 5.85 | -3.00 | 3.50 | -3.00 | -8.66 | 323.10 | -32.09 | 110.66 | 0.5634 | 836.0 | 999999 | |
| 1.03 | -3.00 | 0.62 | -3.00 | -8.39 | 323.02 | -32.17 | 110.16 | 0.5632 | 711.4 | 999999 | |
| 0.00 | 0.69 | 0.00 | 0.41 | -9.18 | 322.94 | -32.24 | 111.44 | 0.5681 | 410.0 | 331.4 | |
| 0.00 | 0.60 | 0.00 | 0.37 | -8.67 | 321.92 | -33.27 | 110.01 | 0.5793 | 355.0 | 237.1 | |
| 0.00 | 0.86 | 0.00 | 0.52 | -7.67 | 321.91 | -33.28 | 108.35 | 0.5751 | 764.0 | 686.8 | |
| 0.00 | 0.86 | 0.00 | 0.52 | -7.66 | 321.45 | -33.74 | 108.10 | 0.5814 | 561.0 | 442.0 | |
| 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. | |