SDO HMI 2011-10-20 07:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.32 | 39.14 | 4.37 | 23.26 | -21.10 | 334.72 | -20.85 | 143.11 | 0.5547 | 15.6 | -100.3 | |
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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 |
| 1.13 | 1.83 | 0.66 | 1.06 | -20.37 | 337.29 | -18.28 | 145.74 | 0.5242 | 838.8 | 748.0 | |
| 0.00 | 4.10 | 0.00 | 2.39 | -20.52 | 336.80 | -18.76 | 145.21 | 0.5301 | 876.0 | 675.1 | |
| 0.00 | 1.31 | 0.00 | 0.77 | -20.86 | 336.58 | -18.98 | 145.30 | 0.5359 | 770.0 | 644.8 | |
| 0.00 | 1.22 | 0.00 | 0.72 | -20.67 | 336.10 | -19.46 | 144.42 | 0.5379 | 810.0 | 708.2 | |
| 0.00 | 1.57 | 0.00 | 0.92 | -20.84 | 336.04 | -19.52 | 144.54 | 0.5403 | 667.0 | 548.3 | |
| 0.00 | 1.39 | 0.00 | 0.81 | -20.08 | 336.04 | -19.52 | 143.65 | 0.5315 | 751.0 | 658.6 | |
| 0.00 | 1.31 | 0.00 | 0.77 | -20.95 | 335.79 | -19.77 | 144.32 | 0.5437 | 652.0 | 509.4 | |
| 0.00 | 1.66 | 0.00 | 0.98 | -20.32 | 334.93 | -20.63 | 142.42 | 0.5441 | 647.0 | 484.1 | |
| 0.00 | 0.96 | 0.00 | 0.57 | -21.58 | 334.16 | -21.40 | 142.90 | 0.5648 | -716.0 | -581.9 | |
| 2.53 | 8.45 | 1.51 | 5.04 | -21.08 | 334.17 | -21.40 | 142.33 | 0.5592 | -775.1 | -476.9 | |
| 0.00 | 2.09 | 0.00 | 1.26 | -21.93 | 333.69 | -21.88 | 142.72 | 0.5728 | -750.0 | -629.5 | |
| 1.92 | 6.62 | 1.15 | 3.97 | -21.36 | 333.74 | -21.82 | 142.13 | 0.5661 | -922.1 | -858.9 | |
| 0.00 | 0.61 | 0.00 | 0.37 | -21.47 | 333.52 | -22.04 | 141.98 | 0.5692 | -507.0 | -435.0 | |
| 1.74 | 4.45 | 1.05 | 2.69 | -21.84 | 333.39 | -22.17 | 142.25 | 0.5744 | -726.0 | -545.1 | |
| 0.00 | 1.57 | 0.00 | 0.94 | -21.34 | 333.40 | -22.16 | 141.68 | 0.5689 | -521.0 | -454.6 | |
| 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. | |