SDO HMI 2011-12-23 13:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.88 | 262.00 | 88.82 | 816.18 | 19.04 | 307.81 | 79.13 | 289.71 | 0.9853 | -42.7 | 14.3 | |
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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 |
| 0.00 | 7.56 | 0.00 | 18.51 | 16.49 | 305.91 | 77.23 | 287.27 | 0.9803 | 293.0 | 92.4 | |
| 10.54 | 110.74 | 41.92 | 486.10 | 19.10 | 310.36 | 81.68 | 289.53 | 0.9926 | -431.6 | -69.1 | |
| 0.00 | 1.78 | 0.00 | 4.22 | 16.84 | 305.40 | 76.72 | 287.68 | 0.9787 | -129.0 | -10.1 | |
| 0.00 | 2.63 | 0.00 | 6.48 | 17.97 | 305.85 | 77.17 | 288.79 | 0.9806 | 206.0 | 67.8 | |
| 0.00 | 6.54 | 0.00 | 21.03 | 20.20 | 308.42 | 79.74 | 290.79 | 0.9886 | -442.0 | -406.8 | |
| 4.16 | 129.78 | 9.10 | 273.25 | 18.51 | 304.17 | 75.49 | 289.51 | 0.9750 | -350.0 | 209.0 | |
| 9.86 | -6.00 | 20.90 | -6.00 | 18.50 | 303.78 | 75.10 | 289.54 | 0.9735 | 535.1 | 999999 | |
| 0.00 | 1.10 | 0.00 | 2.55 | 19.66 | 304.74 | 76.06 | 290.62 | 0.9775 | -181.0 | -183.9 | |
| 0.00 | 1.87 | 0.00 | 4.04 | 19.97 | 303.77 | 75.09 | 291.05 | 0.9742 | 384.0 | 174.4 | |
| 3.40 | -6.00 | 6.86 | -6.00 | 19.78 | 302.80 | 74.11 | 290.97 | 0.9704 | 324.9 | 999999 | |
| 0.76 | -6.00 | 1.51 | -6.00 | 19.80 | 302.48 | 73.79 | 291.03 | 0.9691 | -58.2 | 999999 | |
| 4.16 | -6.00 | 8.53 | -6.00 | 20.30 | 303.00 | 74.32 | 291.47 | 0.9714 | 442.0 | 999999 | |
| 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. | |