SDO HMI 2014-11-09 13:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.44 | 0.00 | 10.59 | -23.07 | 8.27 | -14.94 | 152.22 | 0.5060 | 456.5 | 431.5 | |
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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 | 0.95 | 0.00 | 0.53 | -21.74 | 10.41 | -12.80 | 154.17 | 0.4741 | 712.0 | 544.9 | |
| 0.00 | 3.02 | 0.00 | 1.67 | -20.24 | 10.45 | -12.76 | 152.67 | 0.4533 | 877.0 | 653.1 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -22.40 | 10.25 | -12.96 | 154.53 | 0.4841 | 740.0 | 691.3 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -19.92 | 10.31 | -12.90 | 152.07 | 0.4499 | 914.0 | 759.5 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -21.39 | 9.99 | -13.22 | 153.07 | 0.4722 | 826.0 | 682.4 | |
| 0.00 | 1.55 | 0.00 | 0.86 | -19.83 | 10.09 | -13.11 | 151.57 | 0.4503 | 729.0 | 566.9 | |
| 0.00 | 2.67 | 0.00 | 1.54 | -24.45 | 9.61 | -13.60 | 155.37 | 0.5157 | 889.0 | 744.5 | |
| 0.00 | 1.03 | 0.00 | 0.60 | -24.16 | 8.70 | -14.51 | 153.69 | 0.5178 | 689.0 | 504.1 | |
| 0.00 | 0.43 | 0.00 | 0.25 | -24.37 | 8.10 | -15.11 | 152.97 | 0.5245 | 559.0 | 621.4 | |
| 0.00 | 2.41 | 0.00 | 1.40 | -24.34 | 7.87 | -15.34 | 152.59 | 0.5257 | 691.0 | 524.5 | |
| 0.00 | 1.64 | 0.00 | 0.98 | -25.18 | 4.11 | -19.09 | 148.16 | 0.5634 | -472.0 | -409.6 | |
| 0.00 | 1.38 | 0.00 | 0.85 | -26.38 | 2.25 | -20.96 | 147.05 | 0.5914 | -690.0 | -473.4 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -32.70 | 355.86 | -27.35 | 146.53 | 0.7034 | -530.0 | -417.7 | |
| 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. | |