SDO HMI 2011-06-06 13:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.53 | 174.90 | 21.90 | 90.35 | 9.37 | 336.34 | -13.51 | 54.56 | 0.2838 | -723.9 | -325.7 | |
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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 |
| 34.02 | 138.23 | 17.52 | 71.22 | 9.33 | 336.91 | -12.94 | 53.62 | 0.2757 | -1258.9 | -377.1 | |
| 3.62 | 16.92 | 1.86 | 8.71 | 8.16 | 336.35 | -13.50 | 58.32 | 0.2727 | -1137.9 | -914.4 | |
| 3.44 | -2.00 | 1.77 | -2.00 | 8.46 | 336.18 | -13.67 | 57.67 | 0.2778 | -837.5 | 999999 | |
| 1.45 | -2.00 | 0.75 | -2.00 | 8.25 | 336.09 | -13.76 | 58.50 | 0.2772 | -972.1 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 8.13 | 335.88 | -13.97 | 59.27 | 0.2793 | -815.0 | -543.1 | |
| 0.00 | 2.44 | 0.00 | 1.26 | 8.13 | 335.15 | -14.70 | 60.51 | 0.2899 | -551.0 | -557.2 | |
| 0.00 | 1.99 | 0.00 | 1.04 | 9.51 | 334.67 | -15.17 | 57.26 | 0.3083 | -926.0 | -712.2 | |
| 0.00 | 1.81 | 0.00 | 0.94 | 9.39 | 333.91 | -15.94 | 58.83 | 0.3180 | -849.0 | -762.1 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 10.38 | 333.09 | -16.76 | 57.48 | 0.3379 | 767.0 | 587.7 | |
| 0.00 | 4.89 | 0.00 | 2.57 | 10.25 | 332.84 | -17.01 | 58.17 | 0.3403 | 786.0 | 763.3 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 12.61 | 330.98 | -18.86 | 55.22 | 0.3858 | 919.0 | 787.0 | |
| 0.00 | 1.00 | 0.00 | 0.54 | 12.83 | 330.67 | -19.18 | 55.18 | 0.3918 | 900.0 | 757.3 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 14.15 | 329.09 | -20.76 | 54.50 | 0.4239 | 828.0 | 633.4 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 13.61 | 329.14 | -20.71 | 55.51 | 0.4187 | 762.0 | 564.8 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 9.79 | 328.35 | -21.50 | 64.69 | 0.4012 | 746.0 | 527.0 | |
| 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. | |