SDO HMI 2011-10-20 08:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.77 | 81.14 | 27.31 | 71.65 | -12.04 | 48.41 | 53.39 | 251.42 | 0.8295 | -215.5 | -286.2 | |
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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 |
| 8.02 | 16.30 | 7.98 | 16.26 | -12.05 | 52.91 | 57.89 | 252.74 | 0.8695 | 567.7 | 87.1 | |
| 0.00 | 0.96 | 0.00 | 0.93 | -12.17 | 52.15 | 57.13 | 252.40 | 0.8634 | 436.0 | 403.3 | |
| 0.00 | 0.96 | 0.00 | 0.90 | -9.98 | 51.10 | 56.09 | 254.61 | 0.8498 | 540.0 | 417.4 | |
| 0.00 | 1.48 | 0.00 | 1.38 | -10.79 | 50.89 | 55.87 | 253.62 | 0.8497 | 677.0 | 531.5 | |
| 0.00 | 0.70 | 0.00 | 0.66 | -13.35 | 50.61 | 55.59 | 250.62 | 0.8530 | 499.0 | 494.4 | |
| 0.00 | 1.92 | 0.00 | 1.69 | -12.02 | 48.43 | 53.42 | 251.48 | 0.8304 | -398.0 | -306.0 | |
| 2.27 | 3.14 | 1.98 | 2.74 | -12.02 | 47.97 | 52.95 | 251.35 | 0.8261 | -591.2 | -554.1 | |
| 0.00 | 1.13 | 0.00 | 0.99 | -12.16 | 47.75 | 52.74 | 251.12 | 0.8245 | -447.0 | -388.0 | |
| 0.00 | 1.31 | 0.00 | 1.13 | -12.17 | 47.50 | 52.49 | 251.02 | 0.8222 | -503.0 | -359.3 | |
| 0.00 | 1.57 | 0.00 | 1.33 | -11.25 | 46.86 | 51.84 | 251.90 | 0.8135 | -523.0 | -453.7 | |
| 0.00 | 1.13 | 0.00 | 0.96 | -11.59 | 46.84 | 51.83 | 251.49 | 0.8144 | -359.0 | -319.5 | |
| 1.57 | 3.92 | 1.35 | 3.37 | -12.60 | 47.07 | 52.06 | 250.37 | 0.8193 | -391.8 | -332.6 | |
| 6.71 | 43.66 | 5.72 | 36.82 | -12.24 | 46.82 | 51.81 | 250.72 | 0.8159 | -480.1 | -508.5 | |
| 2.09 | 2.96 | 1.76 | 2.49 | -11.50 | 46.48 | 51.46 | 251.48 | 0.8106 | -618.7 | -588.6 | |
| 10.11 | -13.00 | 8.52 | -13.00 | -12.05 | 46.37 | 51.36 | 250.79 | 0.8111 | -791.4 | 999999 | |
| 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. | |