SDO HMI 2014-11-22 11:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.43 | 24.69 | 0.23 | 13.02 | -13.19 | 225.98 | 13.05 | 219.79 | 0.3434 | 150.7 | 138.3 | |
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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 | 0.69 | 0.00 | 0.38 | -15.41 | 231.34 | 18.41 | 225.71 | 0.4272 | -768.0 | -624.4 | |
| 0.00 | 1.46 | 0.00 | 0.78 | -13.40 | 228.34 | 15.41 | 224.42 | 0.3710 | 711.0 | 563.3 | |
| 0.43 | 1.97 | 0.23 | 1.05 | -13.52 | 227.78 | 14.85 | 223.14 | 0.3661 | 943.8 | 780.4 | |
| 0.00 | 1.29 | 0.00 | 0.68 | -12.38 | 227.68 | 14.75 | 225.22 | 0.3519 | 853.0 | 701.7 | |
| 0.00 | 3.69 | 0.00 | 1.96 | -13.67 | 227.57 | 14.64 | 222.45 | 0.3655 | 766.0 | 677.4 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -12.96 | 227.06 | 14.13 | 222.83 | 0.3514 | 895.0 | 754.2 | |
| 0.00 | 1.63 | 0.00 | 0.86 | -13.11 | 226.97 | 14.04 | 222.36 | 0.3523 | 913.0 | 752.7 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -12.53 | 226.91 | 13.98 | 223.40 | 0.3447 | 920.0 | 803.8 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -13.79 | 226.92 | 13.99 | 220.95 | 0.3598 | 882.0 | 710.7 | |
| 0.00 | 2.40 | 0.00 | 1.27 | -12.77 | 226.83 | 13.90 | 222.74 | 0.3467 | 732.0 | 568.3 | |
| 0.00 | 2.57 | 0.00 | 1.35 | -13.94 | 223.37 | 10.44 | 212.73 | 0.3266 | -969.0 | -712.6 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -13.63 | 223.01 | 10.08 | 212.37 | 0.3192 | -973.0 | -824.5 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -12.10 | 222.86 | 9.93 | 214.81 | 0.2967 | -989.0 | -799.9 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -13.78 | 222.80 | 9.87 | 211.57 | 0.3195 | -835.0 | -731.1 | |
| 0.00 | 3.17 | 0.00 | 1.64 | -12.00 | 222.64 | 9.71 | 214.40 | 0.2934 | -1003.0 | -812.1 | |
| 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. | |