SDO HMI 2014-03-06 11:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.19 | 37.20 | 5.27 | 27.89 | -11.09 | 11.50 | -49.18 | 98.40 | 0.7528 | 207.8 | -3.9 | |
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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 |
| 0.00 | 0.87 | 0.00 | 0.63 | -10.81 | 13.15 | -47.52 | 98.05 | 0.7340 | 652.0 | 550.7 | |
| 0.00 | 0.78 | 0.00 | 0.57 | -12.51 | 12.67 | -48.00 | 100.35 | 0.7399 | 616.0 | 540.2 | |
| 0.00 | 2.25 | 0.00 | 1.64 | -10.67 | 12.96 | -47.72 | 97.86 | 0.7363 | 334.0 | 272.2 | |
| 6.58 | 16.96 | 4.81 | 12.41 | -10.23 | 12.73 | -47.94 | 97.26 | 0.7389 | 725.0 | 434.6 | |
| 0.00 | 1.12 | 0.00 | 0.83 | -10.82 | 12.61 | -48.07 | 98.06 | 0.7403 | 580.0 | 542.8 | |
| 0.61 | 1.73 | 0.46 | 1.31 | -10.30 | 11.01 | -49.67 | 97.38 | 0.7586 | 465.1 | 385.7 | |
| 0.00 | 1.90 | 0.00 | 1.48 | -12.72 | 9.84 | -50.84 | 100.55 | 0.7716 | -633.0 | -508.5 | |
| 0.00 | 1.38 | 0.00 | 1.07 | -12.04 | 9.93 | -50.75 | 99.66 | 0.7706 | -610.0 | -559.2 | |
| 0.00 | 1.04 | 0.00 | 0.80 | -12.33 | 9.85 | -50.83 | 100.04 | 0.7715 | -775.0 | -616.2 | |
| 0.00 | 7.01 | 0.00 | 5.46 | -12.21 | 9.54 | -51.14 | 99.88 | 0.7748 | -730.0 | -522.3 | |
| 0.00 | 2.16 | 0.00 | 1.69 | -11.96 | 9.41 | -51.26 | 99.55 | 0.7761 | -427.0 | -335.1 | |
| 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. | |