SDO HMI 2011-11-27 22:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.25 | 24.81 | 1.69 | 12.95 | 17.61 | 214.86 | 8.56 | 333.33 | 0.3178 | 384.2 | 243.4 | |
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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 | 1.11 | 0.00 | 0.59 | 18.25 | 218.26 | 11.96 | 325.97 | 0.3532 | 848.0 | 724.0 | |
| 0.00 | 4.62 | 0.00 | 2.42 | 16.32 | 217.82 | 11.52 | 323.49 | 0.3236 | -1010.0 | -839.8 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 17.61 | 217.64 | 11.35 | 326.24 | 0.3390 | 881.0 | 748.3 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 19.65 | 217.21 | 10.91 | 330.47 | 0.3632 | 890.0 | 673.3 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 17.15 | 215.70 | 9.40 | 330.23 | 0.3157 | -847.0 | -652.9 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 15.62 | 215.00 | 8.70 | 329.46 | 0.2881 | -881.0 | -624.0 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 17.22 | 214.04 | 7.74 | 334.83 | 0.3040 | 701.0 | 585.9 | |
| 1.71 | 9.92 | 0.89 | 5.16 | 17.99 | 213.10 | 6.81 | 338.55 | 0.3095 | 733.2 | 850.6 | |
| 0.00 | 0.60 | 0.00 | 0.31 | 17.35 | 213.02 | 6.72 | 337.97 | 0.2990 | 802.0 | 564.0 | |
| 1.54 | -8.00 | 0.80 | -8.00 | 17.90 | 212.94 | 6.65 | 338.89 | 0.3071 | 913.1 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 17.96 | 212.70 | 6.40 | 339.68 | 0.3066 | 862.0 | 653.2 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 19.98 | 212.11 | 5.81 | 343.43 | 0.3352 | 862.0 | 730.0 | |
| 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. | |