SDO HMI 2014-07-03 00:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.72 | 0.00 | 8.06 | 6.79 | 270.72 | -23.53 | 81.11 | 0.3999 | -106.6 | -98.1 | |
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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 | 2.00 | 0.00 | 1.02 | 4.70 | 279.76 | -14.49 | 83.10 | 0.2523 | -998.0 | -763.1 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 3.57 | 279.37 | -14.88 | 87.65 | 0.2577 | -755.0 | -603.2 | |
| 0.00 | 0.82 | 0.00 | 0.42 | 7.28 | 279.00 | -15.26 | 73.89 | 0.2729 | -774.0 | -621.2 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 3.49 | 278.20 | -16.05 | 88.03 | 0.2774 | -722.0 | -605.0 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 0.93 | 278.13 | -16.12 | 97.22 | 0.2811 | -804.0 | -649.3 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 4.83 | 276.22 | -18.03 | 83.81 | 0.3116 | -855.0 | -658.3 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 5.17 | 276.18 | -18.07 | 82.75 | 0.3128 | -724.0 | -694.4 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 10.58 | 267.57 | -26.68 | 72.84 | 0.4638 | 830.0 | 768.4 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 10.98 | 266.59 | -27.66 | 72.49 | 0.4798 | 856.0 | 724.7 | |
| 0.00 | 0.82 | 0.00 | 0.46 | 11.35 | 266.31 | -27.95 | 71.90 | 0.4853 | 768.0 | 607.7 | |
| 0.00 | 1.18 | 0.00 | 0.71 | 9.23 | 260.53 | -33.72 | 78.02 | 0.5623 | 714.0 | 565.9 | |
| 0.00 | 1.27 | 0.00 | 0.76 | 8.60 | 260.08 | -34.18 | 79.23 | 0.5675 | 513.0 | 469.2 | |
| 0.00 | 0.82 | 0.00 | 0.56 | 9.06 | 250.59 | -43.67 | 80.09 | 0.6945 | 565.0 | 432.1 | |
| 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. | |