SDO HMI 2011-11-29 04:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.89 | 159.42 | 24.59 | 112.63 | 15.81 | 233.48 | 43.65 | 291.24 | 0.7150 | -754.2 | -327.1 | |
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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 | 0.60 | 0.00 | 0.45 | 16.59 | 236.83 | 47.00 | 291.22 | 0.7543 | 580.0 | 496.3 | |
| 0.00 | 11.89 | 0.00 | 8.71 | 17.72 | 235.13 | 45.30 | 293.24 | 0.7393 | -583.0 | -541.2 | |
| 0.00 | 1.37 | 0.00 | 1.00 | 18.19 | 234.88 | 45.06 | 293.94 | 0.7381 | -343.0 | -289.7 | |
| 26.68 | 126.31 | 18.78 | 88.95 | 15.38 | 233.40 | 43.57 | 290.69 | 0.7128 | -1005.1 | -279.1 | |
| 1.71 | 2.14 | 1.24 | 1.55 | 19.10 | 234.26 | 44.44 | 295.35 | 0.7345 | 447.4 | 413.8 | |
| 0.00 | 0.60 | 0.00 | 0.41 | 13.29 | 232.56 | 42.73 | 288.06 | 0.6970 | -576.0 | -572.7 | |
| 4.45 | 8.12 | 3.14 | 5.73 | 16.61 | 233.27 | 43.44 | 292.40 | 0.7151 | -585.5 | -553.5 | |
| 2.05 | -4.00 | 1.43 | -4.00 | 15.81 | 232.88 | 43.05 | 291.46 | 0.7081 | -849.0 | 999999 | |
| 0.00 | 3.85 | 0.00 | 2.69 | 16.24 | 232.87 | 43.04 | 292.05 | 0.7094 | -859.0 | -709.3 | |
| 0.00 | 1.11 | 0.00 | 0.76 | 14.88 | 232.01 | 42.19 | 290.46 | 0.6951 | -628.0 | -487.0 | |
| 0.00 | 1.37 | 0.00 | 0.97 | 19.31 | 232.47 | 42.64 | 296.34 | 0.7158 | -439.0 | -393.2 | |
| 0.00 | 1.20 | 0.00 | 0.84 | 19.38 | 232.19 | 42.37 | 296.55 | 0.7130 | -554.0 | -427.1 | |
| 0.00 | 0.86 | 0.00 | 0.57 | 16.50 | 229.68 | 39.85 | 293.64 | 0.6730 | -557.0 | -482.5 | |
| 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. | |