SDO HMI 2011-11-27 06:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.10 | 25.25 | 5.80 | 19.12 | 8.82 | 263.36 | 48.27 | 280.74 | 0.7449 | -187.2 | -122.2 | |
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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 | 1.88 | 0.00 | 1.75 | 10.01 | 272.57 | 57.48 | 280.96 | 0.8479 | -425.0 | -313.2 | |
| 0.00 | 1.71 | 0.00 | 1.54 | 10.60 | 271.46 | 56.37 | 281.78 | 0.8381 | -585.0 | -405.6 | |
| 0.00 | 0.94 | 0.00 | 0.84 | 11.45 | 271.00 | 55.91 | 282.85 | 0.8346 | -439.0 | -337.4 | |
| 7.10 | 8.99 | 5.80 | 7.34 | 8.37 | 267.56 | 52.47 | 279.46 | 0.7976 | -552.0 | -482.3 | |
| 0.00 | 1.03 | 0.00 | 0.84 | 9.56 | 267.71 | 52.61 | 280.94 | 0.8003 | -468.0 | -355.9 | |
| 0.00 | 0.94 | 0.00 | 0.71 | 9.39 | 263.86 | 48.77 | 281.22 | 0.7588 | -550.0 | -344.0 | |
| 0.00 | 0.94 | 0.00 | 0.66 | 9.17 | 259.44 | 44.35 | 281.63 | 0.7069 | -656.0 | -577.5 | |
| 0.00 | 1.63 | 0.00 | 1.10 | 6.36 | 257.67 | 42.58 | 277.87 | 0.6812 | -631.0 | -447.4 | |
| 0.00 | 1.20 | 0.00 | 0.74 | 8.67 | 251.07 | 35.98 | 282.72 | 0.5977 | 610.0 | 407.7 | |
| 0.00 | 0.34 | 0.00 | 0.21 | 8.40 | 250.75 | 35.66 | 282.37 | 0.5926 | 638.0 | 474.5 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 7.99 | 250.41 | 35.32 | 281.77 | 0.5871 | 498.0 | 475.4 | |
| 0.00 | 1.88 | 0.00 | 1.16 | 11.01 | 250.44 | 35.35 | 286.80 | 0.5955 | 356.0 | 381.7 | |
| 0.00 | 1.80 | 0.00 | 1.06 | 6.42 | 247.58 | 32.48 | 279.71 | 0.5436 | 765.0 | 579.3 | |
| 0.00 | 1.03 | 0.00 | 0.60 | 6.26 | 246.48 | 31.38 | 279.67 | 0.5273 | 570.0 | 430.3 | |
| 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. | |