SDO HMI 2014-11-13 21:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.29 | 0.00 | 9.00 | -9.07 | 338.74 | 12.68 | 225.10 | 0.3077 | 4.6 | -70.7 | |
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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 | 1.29 | 0.00 | 0.69 | -4.34 | 346.17 | 20.11 | 249.98 | 0.3665 | 829.0 | 697.1 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -7.56 | 343.00 | 16.94 | 237.89 | 0.3426 | 804.0 | 661.9 | |
| 0.00 | 1.29 | 0.00 | 0.68 | -7.41 | 342.96 | 16.91 | 238.22 | 0.3408 | 873.0 | 574.9 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -6.79 | 342.44 | 16.38 | 239.00 | 0.3282 | 713.0 | 479.7 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -11.23 | 341.36 | 15.30 | 226.64 | 0.3575 | 714.0 | 541.8 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -9.88 | 340.85 | 14.80 | 228.63 | 0.3367 | 827.0 | 666.0 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -10.61 | 340.54 | 14.49 | 226.42 | 0.3409 | 1000.0 | 784.9 | |
| 0.00 | 1.38 | 0.00 | 0.71 | -9.87 | 337.58 | 11.52 | 221.54 | 0.2980 | -788.0 | -654.2 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -10.02 | 337.43 | 11.37 | 220.84 | 0.2982 | -748.0 | -636.0 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -8.95 | 336.35 | 10.30 | 220.53 | 0.2729 | -876.0 | -718.6 | |
| 0.00 | 1.46 | 0.00 | 0.76 | -12.49 | 336.19 | 10.14 | 212.81 | 0.3185 | -851.0 | -728.6 | |
| 0.00 | 1.29 | 0.00 | 0.66 | -8.84 | 335.01 | 8.95 | 216.89 | 0.2573 | -883.0 | -663.5 | |
| 0.00 | 1.81 | 0.00 | 0.92 | -7.51 | 334.47 | 8.41 | 218.53 | 0.2338 | -786.0 | -650.5 | |
| 0.00 | 1.89 | 0.00 | 0.97 | -10.62 | 333.90 | 7.84 | 209.67 | 0.2721 | -763.0 | -514.0 | |
| 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. | |