SDO HMI 2011-08-31 19:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.32 | 249.70 | 21.13 | 124.71 | 13.85 | 291.42 | 2.53 | 339.48 | 0.1261 | -538.7 | -334.3 | |
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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 | 2.77 | 0.00 | 1.41 | 18.62 | 293.58 | 4.69 | 338.68 | 0.2143 | 974.0 | 760.3 | |
| 0.00 | 2.95 | 0.00 | 1.49 | 18.13 | 293.31 | 4.43 | 338.92 | 0.2048 | 946.0 | 822.5 | |
| 3.67 | 225.56 | 1.83 | 112.59 | 14.19 | 291.88 | 2.99 | 337.49 | 0.1329 | -1250.9 | -476.3 | |
| 20.94 | -3.00 | 10.45 | -3.00 | 13.37 | 291.72 | 2.83 | 336.03 | 0.1187 | -1293.3 | 999999 | |
| 11.27 | -3.00 | 5.63 | -3.00 | 13.73 | 291.66 | 2.77 | 337.67 | 0.1241 | -1370.0 | 999999 | |
| 6.44 | -3.00 | 3.22 | -3.00 | 14.04 | 291.50 | 2.62 | 339.67 | 0.1281 | -1190.4 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.63 | 15.54 | 290.49 | 1.60 | 349.53 | 0.1485 | 939.0 | 726.2 | |
| 0.00 | 2.06 | 0.00 | 1.02 | 11.10 | 289.50 | 0.61 | 351.25 | 0.0695 | 843.0 | 669.1 | |
| 0.00 | 2.33 | 0.00 | 1.16 | 15.17 | 287.70 | -1.19 | 8.22 | 0.1411 | 1111.0 | 793.5 | |
| 0.00 | 4.38 | 0.00 | 2.19 | 14.65 | 287.42 | -1.47 | 10.81 | 0.1330 | 792.0 | 656.2 | |
| 0.00 | 1.07 | 0.00 | 0.54 | 16.06 | 286.93 | -1.95 | 11.98 | 0.1585 | 885.0 | 681.2 | |
| 0.00 | 1.70 | 0.00 | 0.85 | 15.84 | 286.91 | -1.98 | 12.46 | 0.1550 | 991.0 | 870.9 | |
| 0.00 | 2.68 | 0.00 | 1.35 | 16.52 | 286.77 | -2.12 | 12.30 | 0.1669 | 789.0 | 708.1 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 15.32 | 286.31 | -2.57 | 17.00 | 0.1489 | 891.0 | 719.1 | |
| 0.00 | 1.61 | 0.00 | 0.81 | 16.45 | 286.20 | -2.68 | 15.56 | 0.1681 | 881.0 | 732.3 | |
| 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. | |