SDO HMI 2011-11-13 23:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.42 | 254.00 | 74.90 | 516.48 | 19.15 | 106.37 | 76.08 | 289.01 | 0.9703 | -300.9 | -139.9 | |
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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 |
| 7.65 | 119.73 | 17.95 | 281.83 | 19.07 | 108.43 | 78.14 | 288.86 | 0.9784 | 346.6 | 114.6 | |
| 15.22 | -1.00 | 34.35 | -1.00 | 19.06 | 107.96 | 77.67 | 288.86 | 0.9768 | -449.2 | 999999 | |
| 0.00 | 1.55 | 0.00 | 3.24 | 18.80 | 106.85 | 76.56 | 288.62 | 0.9726 | -533.0 | -524.8 | |
| 2.84 | 101.32 | 5.34 | 177.04 | 18.63 | 105.19 | 74.90 | 288.49 | 0.9659 | -411.5 | -456.7 | |
| 0.00 | 4.82 | 0.00 | 9.68 | 19.37 | 106.18 | 75.89 | 289.22 | 0.9701 | -502.0 | -433.9 | |
| 5.16 | -4.00 | 9.33 | -4.00 | 18.48 | 104.52 | 74.23 | 288.36 | 0.9629 | -639.2 | 999999 | |
| 0.00 | 0.86 | 0.00 | 1.42 | 17.07 | 102.87 | 72.58 | 286.95 | 0.9549 | -169.0 | -196.7 | |
| 1.20 | -4.00 | 2.11 | -4.00 | 18.48 | 103.94 | 73.65 | 288.38 | 0.9603 | -789.7 | 999999 | |
| 0.00 | 0.86 | 0.00 | 1.51 | 18.79 | 103.97 | 73.68 | 288.70 | 0.9605 | -624.0 | -563.4 | |
| 3.35 | -4.00 | 5.82 | -4.00 | 20.15 | 103.70 | 73.42 | 290.13 | 0.9596 | -525.6 | 999999 | |
| 0.00 | 6.71 | 0.00 | 12.56 | 21.36 | 104.97 | 74.69 | 291.32 | 0.9655 | -459.0 | -370.4 | |
| 0.00 | 10.67 | 0.00 | 17.52 | 20.55 | 102.66 | 72.37 | 290.61 | 0.9547 | -300.0 | -327.2 | |
| 0.00 | 7.48 | 0.00 | 11.68 | 20.16 | 101.69 | 71.40 | 290.25 | 0.9498 | 40.0 | -10.4 | |
| 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. | |