SDO HMI 2014-11-13 20:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.10 | 52.20 | 13.71 | 32.53 | 8.57 | 3.72 | 37.11 | 280.23 | 0.6084 | -17.3 | -199.0 | |
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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 |
| 0.43 | 1.89 | 0.28 | 1.22 | 8.25 | 6.13 | 39.52 | 279.30 | 0.6404 | -760.0 | -555.6 | |
| 1.03 | 3.87 | 0.66 | 2.47 | 8.37 | 5.44 | 38.83 | 279.57 | 0.6314 | -643.3 | -537.4 | |
| 0.52 | 1.98 | 0.33 | 1.25 | 7.96 | 5.01 | 38.40 | 279.00 | 0.6251 | -401.5 | -489.0 | |
| 0.00 | 2.15 | 0.00 | 1.36 | 8.11 | 4.91 | 38.30 | 279.26 | 0.6240 | -616.0 | -498.3 | |
| 0.00 | 0.86 | 0.00 | 0.54 | 8.41 | 4.95 | 38.34 | 279.73 | 0.6249 | -299.0 | -270.8 | |
| 10.06 | 22.02 | 6.31 | 13.82 | 8.16 | 4.35 | 37.74 | 279.42 | 0.6164 | -952.6 | -578.4 | |
| 0.00 | 1.46 | 0.00 | 0.91 | 9.54 | 3.49 | 36.88 | 281.82 | 0.6069 | 673.0 | 496.4 | |
| 0.00 | 1.20 | 0.00 | 0.74 | 9.15 | 2.40 | 35.79 | 281.42 | 0.5912 | 762.0 | 623.4 | |
| 0.00 | 1.12 | 0.00 | 0.68 | 9.84 | 2.26 | 35.65 | 282.61 | 0.5907 | 906.0 | 745.7 | |
| 0.86 | 2.15 | 0.53 | 1.32 | 10.06 | 2.21 | 35.60 | 282.98 | 0.5905 | 752.0 | 628.7 | |
| 0.00 | 1.20 | 0.00 | 0.74 | 9.64 | 2.12 | 35.51 | 282.30 | 0.5884 | 540.0 | 452.6 | |
| 9.20 | 12.30 | 5.60 | 7.48 | 8.99 | 1.79 | 35.18 | 281.28 | 0.5824 | 928.9 | 592.3 | |
| 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. | |