SDO HMI 2011-11-24 10:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.62 | 37.01 | 10.06 | 27.08 | 15.99 | 298.37 | 45.92 | 290.28 | 0.7386 | -332.4 | -175.2 | |
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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 | 0.77 | 0.00 | 0.60 | 10.06 | 302.26 | 49.81 | 281.65 | 0.7703 | 483.0 | 302.6 | |
| 12.25 | 15.76 | 9.08 | 11.68 | 16.00 | 299.09 | 46.64 | 290.08 | 0.7464 | -638.3 | -394.6 | |
| 0.00 | 0.86 | 0.00 | 0.63 | 15.37 | 298.63 | 46.18 | 289.37 | 0.7398 | -612.0 | -509.3 | |
| 0.00 | 3.08 | 0.00 | 2.25 | 15.56 | 298.37 | 45.92 | 289.69 | 0.7374 | -451.0 | -438.0 | |
| 0.00 | 4.97 | 0.00 | 3.59 | 15.66 | 297.79 | 45.34 | 289.99 | 0.7311 | -557.0 | -527.5 | |
| 0.00 | 1.71 | 0.00 | 1.24 | 16.24 | 297.87 | 45.42 | 290.75 | 0.7336 | 519.0 | 396.6 | |
| 0.00 | 1.20 | 0.00 | 0.87 | 16.22 | 297.60 | 45.15 | 290.79 | 0.7305 | 297.0 | 290.7 | |
| 1.37 | 2.74 | 0.98 | 1.96 | 15.89 | 297.24 | 44.79 | 290.46 | 0.7255 | -799.6 | -646.6 | |
| 0.00 | 2.74 | 0.00 | 2.00 | 17.79 | 297.68 | 45.23 | 292.85 | 0.7360 | 640.0 | 565.1 | |
| 0.00 | 1.46 | 0.00 | 1.06 | 17.70 | 297.43 | 44.98 | 292.82 | 0.7330 | 632.0 | 384.7 | |
| 0.00 | 0.69 | 0.00 | 0.48 | 16.25 | 296.22 | 43.77 | 291.27 | 0.7150 | -454.0 | -355.2 | |
| 0.00 | 1.03 | 0.00 | 0.72 | 16.26 | 295.79 | 43.34 | 291.42 | 0.7101 | -586.0 | -565.0 | |
| 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. | |