SDO HMI 2014-10-06 06:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.43 | 0.00 | 12.12 | -17.51 | 101.78 | -13.68 | 152.15 | 0.4718 | -86.1 | -47.4 | |
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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 | 1.05 | 0.00 | 0.59 | -19.93 | 110.82 | -4.63 | 170.30 | 0.4523 | 667.0 | 594.8 | |
| 0.00 | 1.58 | 0.00 | 0.84 | -13.69 | 110.77 | -4.69 | 166.99 | 0.3546 | 717.0 | 602.7 | |
| 0.00 | 1.93 | 0.00 | 1.11 | -23.34 | 109.36 | -6.09 | 168.89 | 0.5079 | 758.0 | 581.2 | |
| 0.00 | 1.58 | 0.00 | 0.85 | -15.08 | 109.18 | -6.28 | 163.92 | 0.3831 | 844.0 | 639.4 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -14.92 | 108.96 | -6.50 | 163.28 | 0.3816 | 847.0 | 642.0 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -14.70 | 108.84 | -6.61 | 162.82 | 0.3787 | 717.0 | 629.0 | |
| 0.00 | 1.58 | 0.00 | 0.87 | -16.94 | 106.23 | -9.22 | 158.83 | 0.4262 | 868.0 | 790.0 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -9.65 | 102.96 | -12.50 | 142.18 | 0.3494 | -839.0 | -643.4 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -17.56 | 99.89 | -15.57 | 147.59 | 0.4793 | -935.0 | -825.5 | |
| 0.00 | 1.32 | 0.00 | 0.75 | -17.70 | 98.36 | -17.09 | 145.31 | 0.4940 | -803.0 | -552.5 | |
| 0.00 | 3.08 | 0.00 | 1.76 | -16.29 | 95.83 | -19.62 | 139.73 | 0.5007 | -797.0 | -587.7 | |
| 0.00 | 1.49 | 0.00 | 0.91 | -21.99 | 93.85 | -21.60 | 143.95 | 0.5823 | -662.0 | -573.2 | |
| 0.00 | 0.88 | 0.00 | 0.54 | -22.39 | 93.30 | -22.16 | 143.70 | 0.5913 | -686.0 | -531.1 | |
| 0.00 | 1.05 | 0.00 | 0.63 | -19.18 | 93.52 | -21.93 | 140.30 | 0.5545 | -770.0 | -595.2 | |
| 0.00 | 0.44 | 0.00 | 0.26 | -15.16 | 92.18 | -23.28 | 133.30 | 0.5262 | -662.0 | -510.8 | |
| 0.00 | 0.88 | 0.00 | 0.54 | -19.03 | 89.76 | -25.70 | 135.68 | 0.5889 | -641.0 | -497.9 | |
| 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. | |