SDO HMI 2011-11-27 20:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.82 | 30.35 | 1.47 | 15.81 | 17.77 | 214.74 | 7.34 | 336.82 | 0.3115 | 40.1 | 369.5 | |
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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 | 0.60 | 0.00 | 0.31 | 17.34 | 218.83 | 11.42 | 325.58 | 0.3359 | 808.0 | 588.4 | |
| 0.77 | 5.04 | 0.40 | 2.63 | 16.36 | 217.76 | 10.36 | 326.36 | 0.3129 | -915.4 | -786.0 | |
| 0.68 | -2.00 | 0.36 | -2.00 | 16.24 | 217.72 | 10.32 | 326.23 | 0.3109 | -1048.1 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 17.62 | 217.64 | 10.24 | 328.86 | 0.3292 | 934.0 | 746.0 | |
| 0.00 | 2.65 | 0.00 | 1.40 | 19.60 | 217.13 | 9.73 | 333.09 | 0.3532 | 869.0 | 713.4 | |
| 0.00 | 0.68 | 0.00 | 0.35 | 16.58 | 215.71 | 8.31 | 332.23 | 0.2986 | -882.0 | -717.6 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 17.16 | 215.67 | 8.27 | 333.25 | 0.3068 | -890.0 | -706.7 | |
| 0.00 | 0.68 | 0.00 | 0.36 | 16.86 | 215.57 | 8.16 | 333.07 | 0.3015 | -772.0 | -623.6 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 15.61 | 214.93 | 7.52 | 332.90 | 0.2781 | -940.0 | -623.0 | |
| 0.60 | 13.00 | 0.31 | 6.75 | 18.00 | 213.11 | 5.71 | 341.73 | 0.3033 | 780.1 | 840.1 | |
| 0.77 | -10.00 | 0.40 | -10.00 | 17.94 | 212.96 | 5.55 | 342.14 | 0.3015 | 1009.1 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 17.97 | 212.71 | 5.30 | 342.92 | 0.3007 | 884.0 | 697.9 | |
| 0.00 | 2.31 | 0.00 | 1.21 | 20.02 | 212.17 | 4.77 | 346.29 | 0.3311 | 841.0 | 664.9 | |
| 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. | |