SDO HMI 2014-08-07 11:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.72 | 16.79 | 0.45 | 10.42 | -19.86 | 158.81 | -26.35 | 135.81 | 0.6001 | 483.7 | 457.1 | |
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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 | 0.54 | 0.00 | 0.31 | -17.07 | 164.10 | -21.06 | 138.49 | 0.5204 | 642.0 | 504.5 | |
| 0.00 | 0.63 | 0.00 | 0.38 | -19.70 | 162.74 | -22.42 | 140.08 | 0.5616 | 616.0 | 530.7 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -17.12 | 162.13 | -23.03 | 136.04 | 0.5406 | 648.0 | 550.1 | |
| 0.00 | 1.08 | 0.00 | 0.67 | -20.25 | 159.53 | -25.63 | 137.02 | 0.5975 | 678.0 | 467.2 | |
| 0.00 | 0.27 | 0.00 | 0.17 | -21.08 | 159.27 | -25.89 | 137.73 | 0.6080 | 616.0 | 567.0 | |
| 0.00 | 1.54 | 0.00 | 0.93 | -17.66 | 159.75 | -25.41 | 133.98 | 0.5704 | 724.0 | 559.7 | |
| 0.72 | 5.33 | 0.45 | 3.32 | -20.48 | 158.98 | -26.18 | 136.71 | 0.6049 | 970.5 | 693.2 | |
| 0.00 | 1.08 | 0.00 | 0.69 | -22.27 | 158.19 | -26.97 | 137.98 | 0.6292 | 524.0 | 351.8 | |
| 0.00 | 1.90 | 0.00 | 1.15 | -17.20 | 158.97 | -26.19 | 132.52 | 0.5742 | 592.0 | 519.7 | |
| 0.00 | 0.90 | 0.00 | 0.56 | -19.68 | 158.19 | -26.97 | 134.89 | 0.6050 | 535.0 | 446.9 | |
| 0.00 | 0.45 | 0.00 | 0.30 | -21.99 | 154.46 | -30.70 | 134.07 | 0.6612 | -504.0 | -435.8 | |
| 0.00 | 0.81 | 0.00 | 0.55 | -24.46 | 153.78 | -31.38 | 136.27 | 0.6881 | 392.0 | 350.3 | |
| 0.00 | 0.99 | 0.00 | 0.65 | -21.04 | 154.31 | -30.85 | 132.81 | 0.6548 | -364.0 | -431.6 | |
| 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. | |