SDO HMI 2014-03-06 12:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.08 | 33.04 | 6.63 | 24.45 | -11.09 | 11.62 | -48.51 | 98.41 | 0.7452 | 273.3 | 80.4 | |
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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 | 1.73 | 0.00 | 1.24 | -10.79 | 13.33 | -46.80 | 98.02 | 0.7255 | 440.0 | 422.6 | |
| 0.00 | 1.12 | 0.00 | 0.82 | -12.53 | 12.67 | -47.46 | 100.41 | 0.7336 | 460.0 | 403.8 | |
| 0.00 | 0.87 | 0.00 | 0.62 | -10.72 | 12.94 | -47.19 | 97.93 | 0.7301 | 622.0 | 478.7 | |
| 0.00 | 3.03 | 0.00 | 2.19 | -10.88 | 12.73 | -47.40 | 98.15 | 0.7326 | 612.0 | 573.3 | |
| 7.27 | 11.59 | 5.26 | 8.39 | -10.23 | 12.82 | -47.31 | 97.26 | 0.7315 | 736.5 | 514.1 | |
| 0.00 | 0.52 | 0.00 | 0.38 | -11.64 | 12.43 | -47.70 | 99.18 | 0.7362 | 450.0 | 411.5 | |
| 0.69 | 1.82 | 0.50 | 1.32 | -10.20 | 12.51 | -47.62 | 97.22 | 0.7352 | 238.4 | 217.9 | |
| 0.00 | 1.73 | 0.00 | 1.29 | -10.31 | 11.07 | -49.06 | 97.38 | 0.7517 | 565.0 | 415.9 | |
| 0.00 | 1.12 | 0.00 | 0.86 | -12.09 | 9.89 | -50.23 | 99.74 | 0.7649 | -711.0 | -579.7 | |
| 0.00 | 1.47 | 0.00 | 1.13 | -12.27 | 9.85 | -50.28 | 99.97 | 0.7654 | -645.0 | -668.7 | |
| 1.12 | 4.24 | 0.87 | 3.27 | -12.27 | 9.51 | -50.62 | 99.96 | 0.7691 | -640.8 | -547.0 | |
| 0.00 | 2.42 | 0.00 | 1.87 | -12.01 | 9.39 | -50.74 | 99.63 | 0.7705 | -420.0 | -327.6 | |
| 0.00 | 1.38 | 0.00 | 1.07 | -12.37 | 9.29 | -50.84 | 100.09 | 0.7715 | -263.0 | -259.2 | |
| 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. | |