SDO HMI 2014-04-12 00:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.34 | 0.00 | 9.30 | -14.03 | 304.36 | 5.59 | 210.10 | 0.2013 | 17.1 | 34.4 | |
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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 | 2.29 | 0.00 | 1.18 | -14.99 | 311.54 | 12.77 | 232.98 | 0.2686 | 831.0 | 679.6 | |
| 0.00 | 1.94 | 0.00 | 1.00 | -15.03 | 311.19 | 12.42 | 232.13 | 0.2643 | 768.0 | 614.7 | |
| 0.00 | 2.38 | 0.00 | 1.21 | -12.13 | 310.57 | 11.80 | 240.92 | 0.2298 | 826.0 | 616.3 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -18.70 | 307.69 | 8.92 | 213.32 | 0.2684 | 755.0 | 598.9 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -7.80 | 306.42 | 7.65 | 255.31 | 0.1369 | 742.0 | 525.3 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -4.71 | 305.98 | 7.21 | 278.84 | 0.1272 | 821.0 | 717.1 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -12.56 | 305.72 | 6.95 | 225.18 | 0.1673 | 773.0 | 598.3 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -16.33 | 300.41 | 1.63 | 188.55 | 0.1846 | -780.0 | -537.6 | |
| 0.00 | 3.00 | 0.00 | 1.50 | -13.54 | 298.44 | -0.33 | 177.58 | 0.1342 | -930.0 | -818.2 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -17.07 | 297.52 | -1.25 | 173.86 | 0.1963 | -791.0 | -614.3 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -16.85 | 297.34 | -1.44 | 172.81 | 0.1930 | -904.0 | -706.1 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -17.21 | 295.66 | -3.11 | 165.25 | 0.2045 | -985.0 | -853.3 | |
| 0.00 | 0.71 | 0.00 | 0.35 | -13.67 | 294.70 | -4.08 | 153.08 | 0.1532 | -904.0 | -793.9 | |
| 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. | |