SDO HMI 2014-09-06 00:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 80.18 | 447.31 | 101.27 | 565.17 | 14.89 | 86.76 | -67.99 | 76.85 | 0.9216 | 119.6 | -142.9 | |
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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 |
| 53.30 | 429.99 | 65.00 | 542.20 | 15.35 | 87.70 | -67.05 | 76.39 | 0.9154 | 600.1 | -140.5 | |
| 0.00 | 0.98 | 0.00 | 1.28 | 16.46 | 85.98 | -68.77 | 75.13 | 0.9265 | 151.0 | 104.4 | |
| 0.00 | 4.20 | 0.00 | 5.59 | 15.91 | 85.51 | -69.24 | 75.72 | 0.9295 | -260.0 | -232.8 | |
| 0.00 | 2.59 | 0.00 | 3.24 | 13.22 | 87.03 | -67.72 | 78.69 | 0.9203 | -260.0 | -215.4 | |
| 0.00 | 0.98 | 0.00 | 1.23 | 12.92 | 87.12 | -67.63 | 79.02 | 0.9198 | -407.0 | -347.1 | |
| 0.00 | 1.07 | 0.00 | 1.35 | 12.82 | 86.84 | -67.91 | 79.11 | 0.9217 | -582.0 | -552.3 | |
| 0.00 | 0.71 | 0.00 | 0.98 | 15.94 | 84.75 | -70.00 | 75.66 | 0.9341 | -350.0 | -329.4 | |
| 0.00 | 2.41 | 0.00 | 3.30 | 15.67 | 84.78 | -69.97 | 75.96 | 0.9340 | -417.0 | -409.7 | |
| 7.95 | -1.00 | 10.63 | -1.00 | 14.18 | 85.40 | -69.35 | 77.58 | 0.9306 | -754.7 | 999999 | |
| 2.68 | -1.00 | 3.57 | -1.00 | 13.85 | 85.53 | -69.22 | 77.94 | 0.9299 | -681.5 | 999999 | |
| 9.46 | -1.00 | 12.91 | -1.00 | 14.59 | 84.94 | -69.82 | 77.12 | 0.9333 | -711.2 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.35 | 12.62 | 85.93 | -68.82 | 79.28 | 0.9277 | -435.0 | -383.3 | |
| 6.79 | -1.00 | 9.16 | -1.00 | 13.42 | 85.28 | -69.48 | 78.39 | 0.9316 | -377.2 | 999999 | |
| 0.00 | 1.16 | 0.00 | 1.54 | 12.92 | 85.58 | -69.17 | 78.94 | 0.9298 | -352.0 | -336.0 | |
| 0.00 | 2.95 | 0.00 | 4.11 | 14.28 | 84.41 | -70.34 | 77.43 | 0.9365 | 309.0 | 259.6 | |
| 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. | |