SDO HMI 2014-03-06 10:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.75 | 122.45 | 32.38 | 124.38 | -9.99 | 359.64 | -61.58 | 97.44 | 0.8754 | 512.2 | 248.6 | |
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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 | 0.43 | 0.00 | 0.46 | -19.35 | 358.05 | -63.18 | 108.09 | 0.8877 | 139.0 | 186.0 | |
| 16.09 | 103.57 | 16.20 | 103.85 | -10.37 | 359.96 | -61.26 | 97.85 | 0.8726 | 733.6 | 323.5 | |
| 10.21 | -2.00 | 10.22 | -2.00 | -9.55 | 0.17 | -61.05 | 96.90 | 0.8713 | 730.3 | 999999 | |
| 0.00 | 3.29 | 0.00 | 3.33 | -8.23 | 359.92 | -61.30 | 95.40 | 0.8740 | -484.0 | -356.1 | |
| 0.69 | 1.82 | 0.75 | 1.96 | -10.89 | 357.80 | -63.42 | 98.55 | 0.8900 | 416.2 | 359.5 | |
| 0.00 | 0.61 | 0.00 | 0.66 | -9.27 | 357.63 | -63.59 | 96.74 | 0.8920 | 185.0 | 133.1 | |
| 3.89 | 6.84 | 4.24 | 7.46 | -9.05 | 357.57 | -63.65 | 96.50 | 0.8926 | 367.9 | 188.2 | |
| 0.87 | 3.46 | 0.97 | 3.87 | -10.16 | 356.76 | -64.46 | 97.79 | 0.8983 | -556.7 | -484.0 | |
| 0.00 | 0.78 | 0.00 | 0.87 | -9.23 | 356.74 | -64.48 | 96.75 | 0.8988 | 188.0 | 135.7 | |
| 0.00 | 1.30 | 0.00 | 1.49 | -9.56 | 355.98 | -65.24 | 97.17 | 0.9044 | -620.0 | -488.8 | |
| 0.00 | 0.35 | 0.00 | 0.43 | -14.38 | 353.44 | -67.79 | 102.58 | 0.9205 | -430.0 | -428.2 | |
| 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. | |