SDO HMI 2014-03-06 12:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.48 | 136.95 | 30.89 | 135.39 | -10.07 | 359.47 | -60.66 | 97.48 | 0.8674 | 493.4 | 223.9 | |
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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 |
| 12.28 | 111.68 | 11.90 | 108.41 | -9.56 | 0.25 | -59.88 | 96.85 | 0.8611 | 701.7 | 295.7 | |
| 15.57 | -1.00 | 15.17 | -1.00 | -10.34 | 359.95 | -60.18 | 97.77 | 0.8635 | 695.5 | 999999 | |
| 0.00 | 1.47 | 0.00 | 1.44 | -8.11 | 359.92 | -60.21 | 95.19 | 0.8647 | -388.0 | -279.4 | |
| 0.00 | 0.61 | 0.00 | 0.60 | -8.69 | 359.70 | -60.42 | 95.87 | 0.8663 | 273.0 | 244.9 | |
| 0.00 | 3.03 | 0.00 | 3.15 | -10.93 | 357.84 | -62.29 | 98.54 | 0.8809 | 469.0 | 324.6 | |
| 0.00 | 0.95 | 0.00 | 0.99 | -10.11 | 357.87 | -62.26 | 97.61 | 0.8810 | 443.0 | 414.4 | |
| 0.00 | 0.61 | 0.00 | 0.68 | -15.60 | 355.17 | -64.96 | 103.86 | 0.9006 | -314.0 | -249.1 | |
| 0.00 | 2.85 | 0.00 | 2.99 | -9.31 | 357.68 | -62.45 | 96.71 | 0.8829 | 171.0 | 204.0 | |
| 3.63 | 6.57 | 3.82 | 6.91 | -9.05 | 357.56 | -62.57 | 96.43 | 0.8840 | 336.8 | 149.9 | |
| 0.00 | 4.33 | 0.00 | 4.67 | -10.25 | 356.68 | -63.45 | 97.84 | 0.8904 | -593.0 | -455.8 | |
| 0.00 | 1.30 | 0.00 | 1.40 | -9.33 | 356.80 | -63.33 | 96.79 | 0.8899 | 50.0 | 84.3 | |
| 0.00 | 0.95 | 0.00 | 1.05 | -11.25 | 355.87 | -64.25 | 99.00 | 0.8963 | 281.0 | 239.1 | |
| 0.00 | 2.60 | 0.00 | 3.10 | -14.38 | 353.63 | -66.50 | 102.54 | 0.9118 | -404.0 | -312.1 | |
| 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. | |