SDO HMI 2011-10-22 04:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.61 | 37.88 | 1.34 | 19.39 | 18.38 | 324.08 | -6.75 | 25.50 | 0.2542 | 557.1 | 339.8 | |
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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 | 1.22 | 0.00 | 0.61 | 14.88 | 327.60 | -3.22 | 18.10 | 0.1755 | 848.0 | 589.1 | |
| 0.00 | 7.92 | 0.00 | 4.02 | 16.97 | 326.70 | -4.13 | 18.83 | 0.2143 | -1298.0 | -954.6 | |
| 0.61 | 2.18 | 0.31 | 1.10 | 17.12 | 326.35 | -4.48 | 20.03 | 0.2187 | -1081.0 | -898.1 | |
| 0.00 | 1.22 | 0.00 | 0.62 | 18.21 | 325.19 | -5.64 | 22.68 | 0.2431 | 886.0 | 729.0 | |
| 2.00 | 4.79 | 1.03 | 2.46 | 18.82 | 324.02 | -6.80 | 25.62 | 0.2604 | 1100.7 | 899.5 | |
| 0.00 | 7.75 | 0.00 | 3.97 | 18.45 | 323.88 | -6.94 | 26.75 | 0.2559 | 862.0 | 1069.4 | |
| 0.00 | 1.92 | 0.00 | 0.98 | 18.66 | 323.68 | -7.14 | 27.01 | 0.2606 | 734.0 | 588.3 | |
| 0.00 | 1.22 | 0.00 | 0.62 | 18.50 | 323.56 | -7.26 | 27.68 | 0.2592 | 882.0 | 699.7 | |
| 0.00 | 2.44 | 0.00 | 1.26 | 19.05 | 322.68 | -8.15 | 29.38 | 0.2742 | 892.0 | 629.4 | |
| 0.00 | 2.00 | 0.00 | 1.03 | 18.58 | 322.60 | -8.22 | 30.50 | 0.2682 | 936.0 | 749.3 | |
| 0.00 | 1.31 | 0.00 | 0.68 | 21.40 | 320.80 | -10.02 | 30.24 | 0.3232 | 854.0 | 650.7 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 21.80 | 320.74 | -10.09 | 29.72 | 0.3294 | 742.0 | 631.1 | |
| 0.00 | 0.87 | 0.00 | 0.45 | 20.24 | 319.84 | -10.98 | 34.64 | 0.3159 | 846.0 | 671.1 | |
| 0.00 | 1.13 | 0.00 | 0.59 | 20.51 | 319.40 | -11.42 | 35.15 | 0.3236 | 742.0 | 573.5 | |
| 0.00 | 0.87 | 0.00 | 0.45 | 19.51 | 319.12 | -11.71 | 37.77 | 0.3136 | 903.0 | 733.8 | |
| 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. | |