SDO HMI 2011-05-05 16:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.83 | 323.03 | 24.78 | 174.67 | 17.93 | 61.01 | 9.52 | 336.88 | 0.4024 | -804.6 | -391.7 | |
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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 | 1.25 | 0.00 | 0.71 | 23.65 | 62.52 | 11.02 | 339.11 | 0.4932 | -657.0 | -494.9 | |
| 39.49 | 307.31 | 21.35 | 166.16 | 17.82 | 61.22 | 9.73 | 336.30 | 0.4019 | -1430.7 | -433.1 | |
| 4.73 | -2.00 | 2.56 | -2.00 | 18.27 | 60.86 | 9.37 | 337.54 | 0.4063 | -989.7 | 999999 | |
| 1.61 | -2.00 | 0.87 | -2.00 | 18.40 | 60.55 | 9.05 | 338.35 | 0.4062 | -620.8 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 19.51 | 60.38 | 8.89 | 339.72 | 0.4217 | -720.0 | -562.4 | |
| 0.00 | 1.34 | 0.00 | 0.73 | 19.47 | 59.44 | 7.94 | 341.68 | 0.4162 | -675.0 | -530.1 | |
| 0.00 | 1.16 | 0.00 | 0.63 | 19.27 | 59.27 | 7.77 | 341.89 | 0.4123 | -515.0 | -465.2 | |
| 0.00 | 1.34 | 0.00 | 0.72 | 17.56 | 57.88 | 6.38 | 343.71 | 0.3796 | 810.0 | 661.7 | |
| 0.00 | 1.88 | 0.00 | 1.01 | 17.92 | 57.80 | 6.30 | 344.18 | 0.3847 | 790.0 | 617.3 | |
| 0.00 | 0.89 | 0.00 | 0.48 | 17.72 | 57.60 | 6.10 | 344.51 | 0.3808 | 875.0 | 725.5 | |
| 0.00 | 1.61 | 0.00 | 0.86 | 17.56 | 57.50 | 6.00 | 344.64 | 0.3778 | 837.0 | 630.2 | |
| 0.00 | 1.07 | 0.00 | 0.58 | 18.47 | 57.50 | 6.00 | 345.28 | 0.3920 | 821.0 | 693.2 | |
| 0.00 | 1.97 | 0.00 | 1.05 | 17.85 | 57.35 | 5.85 | 345.21 | 0.3817 | 767.0 | 652.7 | |
| 0.00 | 1.16 | 0.00 | 0.62 | 18.85 | 55.59 | 4.09 | 350.03 | 0.3914 | 885.0 | 683.2 | |
| 0.00 | 1.07 | 0.00 | 0.58 | 19.34 | 54.38 | 2.88 | 353.09 | 0.3963 | 809.0 | 630.2 | |
| 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. | |