SDO HMI 2011-10-22 11:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.04 | 331.71 | 105.24 | 767.44 | 7.78 | 249.07 | -77.92 | 83.20 | 0.9728 | -153.9 | -66.6 | |
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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 | 0.87 | 0.00 | 1.30 | 10.95 | 255.62 | -71.38 | 80.23 | 0.9455 | -232.0 | -209.4 | |
| 19.06 | 222.94 | 30.15 | 365.76 | 6.19 | 254.78 | -72.21 | 85.21 | 0.9513 | -563.4 | -119.3 | |
| 0.00 | 0.87 | 0.00 | 1.64 | 11.11 | 251.50 | -75.50 | 79.91 | 0.9661 | -111.0 | -128.0 | |
| 4.00 | -2.00 | 6.62 | -2.00 | 6.15 | 253.98 | -73.02 | 85.20 | 0.9556 | -312.2 | 999999 | |
| 2.44 | -2.00 | 4.15 | -2.00 | 5.99 | 253.51 | -73.49 | 85.34 | 0.9580 | -135.6 | 999999 | |
| 2.35 | -2.00 | 4.07 | -2.00 | 5.96 | 253.19 | -73.80 | 85.35 | 0.9596 | 224.8 | 999999 | |
| 0.00 | 2.26 | 0.00 | 4.13 | 7.47 | 252.21 | -74.78 | 83.71 | 0.9638 | -253.0 | -85.5 | |
| 0.00 | 1.31 | 0.00 | 2.42 | 4.60 | 252.17 | -74.82 | 86.68 | 0.9648 | 414.0 | 363.0 | |
| 6.27 | 99.46 | 20.61 | 381.26 | 10.27 | 244.93 | -82.06 | 80.39 | 0.9891 | 328.5 | -29.2 | |
| 0.00 | 1.91 | 0.00 | 4.79 | 6.60 | 247.92 | -79.08 | 84.31 | 0.9811 | 321.0 | 306.3 | |
| 3.48 | -9.00 | 12.38 | -9.00 | 9.36 | 244.26 | -82.74 | 81.26 | 0.9909 | 321.7 | 999999 | |
| 0.52 | -9.00 | 1.99 | -9.00 | 9.45 | 243.60 | -83.39 | 81.12 | 0.9923 | -190.5 | 999999 | |
| 0.70 | -9.00 | 2.67 | -9.00 | 9.30 | 243.56 | -83.43 | 81.28 | 0.9924 | -246.4 | 999999 | |
| 0.00 | 2.09 | 0.00 | 6.14 | 6.39 | 246.29 | -80.70 | 84.41 | 0.9862 | 330.0 | 331.0 | |
| 5.22 | -9.00 | 22.60 | -9.00 | 8.57 | 242.90 | -84.09 | 81.96 | 0.9939 | -380.7 | 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. | |