SDO HMI 2011-11-29 22:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.77 | 63.48 | 14.90 | 45.50 | 17.89 | 223.84 | 43.90 | 294.03 | 0.7249 | -426.0 | -233.2 | |
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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 | 1.62 | 0.00 | 1.22 | 16.50 | 227.16 | 47.22 | 291.10 | 0.7567 | 497.0 | 328.1 | |
| 0.00 | 0.85 | 0.00 | 0.61 | 12.07 | 225.48 | 45.54 | 285.70 | 0.7274 | 548.0 | 493.2 | |
| 0.00 | 1.54 | 0.00 | 1.09 | 14.12 | 224.41 | 44.47 | 288.76 | 0.7198 | 527.0 | 415.8 | |
| 3.85 | 8.37 | 2.79 | 6.08 | 17.92 | 224.58 | 44.64 | 293.79 | 0.7330 | -644.8 | -510.2 | |
| 0.00 | 1.03 | 0.00 | 0.76 | 19.69 | 225.18 | 45.24 | 295.87 | 0.7454 | -485.0 | -364.8 | |
| 0.00 | 1.28 | 0.00 | 0.92 | 17.50 | 223.79 | 43.86 | 293.52 | 0.7230 | -705.0 | -568.3 | |
| 0.00 | 2.91 | 0.00 | 2.09 | 17.93 | 223.93 | 43.99 | 294.04 | 0.7259 | -695.0 | -578.7 | |
| 0.00 | 1.03 | 0.00 | 0.73 | 17.25 | 223.68 | 43.74 | 293.23 | 0.7209 | -720.0 | -620.5 | |
| 16.92 | 37.94 | 12.11 | 27.16 | 18.30 | 223.66 | 43.72 | 294.64 | 0.7242 | -764.3 | -337.8 | |
| 0.00 | 2.39 | 0.00 | 1.67 | 15.63 | 222.80 | 42.86 | 291.35 | 0.7057 | 622.0 | 456.1 | |
| 0.00 | 1.79 | 0.00 | 1.25 | 16.46 | 222.77 | 42.83 | 292.49 | 0.7080 | 602.0 | 421.6 | |
| 0.00 | 0.85 | 0.00 | 0.61 | 20.84 | 223.04 | 43.10 | 298.23 | 0.7272 | -568.0 | -538.2 | |
| 0.00 | 0.94 | 0.00 | 0.65 | 17.61 | 221.62 | 41.69 | 294.51 | 0.6990 | -490.0 | -443.7 | |
| 0.00 | 0.94 | 0.00 | 0.66 | 19.98 | 221.72 | 41.78 | 297.67 | 0.7094 | 461.0 | 379.1 | |
| 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. | |