SDO HMI 2014-09-13 06:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.30 | 41.75 | 9.52 | 60.39 | 13.67 | 348.07 | -70.95 | 78.04 | 0.9385 | -111.9 | 175.2 | |
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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 | 0.27 | 0.00 | 0.30 | 12.86 | 353.90 | -65.12 | 79.17 | 0.9023 | -318.0 | -255.7 | |
| 0.00 | 0.89 | 0.00 | 1.09 | 16.09 | 351.94 | -67.08 | 75.57 | 0.9156 | -155.0 | -166.0 | |
| 5.07 | 9.52 | 5.85 | 11.00 | 12.48 | 353.56 | -65.46 | 79.58 | 0.9048 | -414.1 | -107.7 | |
| 0.00 | 0.98 | 0.00 | 1.12 | 11.72 | 353.92 | -65.10 | 80.44 | 0.9025 | -378.0 | -290.8 | |
| 0.00 | 1.51 | 0.00 | 1.86 | 15.47 | 351.78 | -67.24 | 76.23 | 0.9167 | -70.0 | -115.2 | |
| 0.00 | 2.49 | 0.00 | 2.86 | 8.71 | 353.91 | -65.11 | 83.77 | 0.9038 | -480.0 | -334.6 | |
| 0.71 | 4.98 | 1.07 | 7.46 | 14.33 | 347.06 | -71.96 | 77.29 | 0.9458 | 446.6 | 422.2 | |
| 0.45 | 10.59 | 0.67 | 16.33 | 13.98 | 346.93 | -72.09 | 77.66 | 0.9466 | 476.0 | 346.4 | |
| 0.00 | 1.34 | 0.00 | 2.16 | 14.98 | 345.66 | -73.36 | 76.53 | 0.9531 | 10.0 | 29.7 | |
| 0.00 | 1.34 | 0.00 | 2.26 | 14.52 | 344.71 | -74.31 | 76.96 | 0.9579 | 386.0 | 302.9 | |
| 0.00 | 3.83 | 0.00 | 6.69 | 14.38 | 344.26 | -74.76 | 77.09 | 0.9601 | 404.0 | 244.4 | |
| 1.07 | 4.01 | 1.93 | 7.26 | 14.24 | 343.65 | -75.37 | 77.19 | 0.9630 | 137.9 | 133.6 | |
| 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. | |