SDO HMI 2011-11-23 09:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.68 | 274.72 | 32.00 | 193.20 | 17.45 | 223.01 | -43.17 | 67.00 | 0.7113 | -527.7 | -217.2 | |
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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 |
| 34.28 | 250.90 | 23.91 | 175.86 | 17.41 | 223.42 | -42.75 | 66.91 | 0.7065 | -1008.7 | -281.9 | |
| 1.46 | -1.00 | 1.03 | -1.00 | 17.40 | 222.83 | -43.35 | 67.14 | 0.7132 | -273.0 | 999999 | |
| 7.71 | -1.00 | 5.48 | -1.00 | 17.95 | 222.49 | -43.69 | 66.52 | 0.7188 | -632.5 | 999999 | |
| 2.23 | 2.91 | 1.58 | 2.06 | 16.25 | 222.18 | -44.00 | 68.93 | 0.7171 | -408.4 | -343.8 | |
| 0.00 | 1.46 | 0.00 | 1.05 | 18.05 | 221.54 | -44.63 | 66.71 | 0.7296 | -422.0 | -293.6 | |
| 0.00 | 0.94 | 0.00 | 0.68 | 17.18 | 221.38 | -44.80 | 67.92 | 0.7288 | 708.0 | 577.5 | |
| 0.00 | 8.48 | 0.00 | 6.08 | 16.57 | 221.52 | -44.66 | 68.70 | 0.7254 | 368.0 | 304.9 | |
| 0.00 | 0.86 | 0.00 | 0.62 | 16.80 | 220.71 | -45.47 | 68.64 | 0.7351 | 763.0 | 612.9 | |
| 0.00 | 1.54 | 0.00 | 1.12 | 16.15 | 220.68 | -45.50 | 69.51 | 0.7337 | 788.0 | 694.0 | |
| 0.00 | 2.23 | 0.00 | 1.63 | 16.36 | 220.31 | -45.87 | 69.35 | 0.7384 | 713.0 | 612.0 | |
| 0.00 | 0.51 | 0.00 | 0.39 | 18.38 | 219.46 | -46.71 | 66.96 | 0.7530 | 549.0 | 568.3 | |
| 0.00 | 1.80 | 0.00 | 1.35 | 17.57 | 219.20 | -46.98 | 68.09 | 0.7536 | 611.0 | 465.7 | |
| 0.00 | 1.29 | 0.00 | 0.95 | 15.80 | 219.76 | -46.41 | 70.25 | 0.7429 | 522.0 | 473.7 | |
| 0.00 | 0.86 | 0.00 | 0.64 | 17.35 | 219.18 | -47.00 | 68.38 | 0.7532 | 668.0 | 578.3 | |
| 0.00 | 0.94 | 0.00 | 0.77 | 20.88 | 215.47 | -50.71 | 65.03 | 0.7999 | 551.0 | 512.5 | |
| 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. | |