SDO HMI 2014-09-19 01:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.57 | 51.18 | 9.14 | 34.18 | -21.12 | 310.76 | -31.79 | 132.91 | 0.6726 | -291.9 | -233.8 | |
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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 | 1.51 | 0.00 | 0.96 | -20.51 | 315.16 | -27.39 | 136.32 | 0.6261 | 779.0 | 531.1 | |
| 0.00 | 4.79 | 0.00 | 3.07 | -20.07 | 313.53 | -29.02 | 134.18 | 0.6376 | 792.0 | 656.8 | |
| 0.00 | 1.95 | 0.00 | 1.25 | -19.23 | 313.04 | -29.51 | 132.70 | 0.6350 | 659.0 | 545.4 | |
| 1.06 | 2.75 | 0.69 | 1.79 | -20.30 | 312.56 | -29.99 | 133.53 | 0.6489 | 795.3 | 611.3 | |
| 0.71 | 2.48 | 0.46 | 1.61 | -19.89 | 312.65 | -29.90 | 133.13 | 0.6446 | 795.1 | 672.5 | |
| 0.00 | 0.98 | 0.00 | 0.63 | -18.94 | 312.37 | -30.19 | 131.71 | 0.6393 | 439.0 | 399.1 | |
| 0.00 | 1.24 | 0.00 | 0.83 | -21.72 | 311.14 | -31.41 | 133.90 | 0.6742 | -726.0 | -573.4 | |
| 0.00 | 1.69 | 0.00 | 1.13 | -21.63 | 310.48 | -32.07 | 133.22 | 0.6796 | -802.0 | -725.4 | |
| 6.39 | 14.90 | 4.32 | 10.07 | -21.57 | 309.96 | -32.59 | 132.70 | 0.6840 | -916.2 | -749.7 | |
| 3.02 | 6.12 | 2.03 | 4.12 | -20.98 | 310.03 | -32.52 | 132.08 | 0.6787 | -916.9 | -691.9 | |
| 0.00 | 2.75 | 0.00 | 1.88 | -22.10 | 309.74 | -32.81 | 133.12 | 0.6901 | -725.0 | -579.1 | |
| 0.00 | 0.35 | 0.00 | 0.24 | -21.20 | 309.82 | -32.73 | 132.16 | 0.6824 | -419.0 | -399.0 | |
| 1.15 | 9.67 | 0.79 | 6.60 | -21.89 | 309.29 | -33.26 | 132.51 | 0.6927 | -573.0 | -505.6 | |
| 1.24 | -13.00 | 0.85 | -13.00 | -21.61 | 309.33 | -33.22 | 132.22 | 0.6902 | -859.2 | 999999 | |
| 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. | |