SDO HMI 2011-05-27 10:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73.24 | 147.57 | 39.40 | 79.45 | 20.65 | 130.52 | 6.69 | 343.96 | 0.3914 | 38.3 | -80.4 | |
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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 |
| 21.56 | 67.30 | 11.70 | 36.52 | 21.12 | 132.85 | 9.02 | 338.97 | 0.4092 | -1103.8 | -406.0 | |
| 5.41 | -1.00 | 2.93 | -1.00 | 20.92 | 132.57 | 8.74 | 339.37 | 0.4047 | -1212.6 | 999999 | |
| 0.36 | 9.83 | 0.20 | 5.32 | 21.21 | 131.24 | 7.41 | 342.52 | 0.4021 | -951.8 | -789.5 | |
| 1.35 | 1.80 | 0.73 | 0.97 | 20.39 | 131.20 | 7.37 | 341.93 | 0.3894 | -852.1 | -821.2 | |
| 5.32 | -3.00 | 2.88 | -3.00 | 21.34 | 131.08 | 7.25 | 342.97 | 0.4034 | -925.5 | 999999 | |
| 1.08 | 2.98 | 0.58 | 1.59 | 19.96 | 130.07 | 6.24 | 344.22 | 0.3776 | 624.8 | 563.5 | |
| 0.00 | 2.07 | 0.00 | 1.11 | 19.51 | 129.70 | 5.87 | 344.78 | 0.3688 | 952.0 | 691.2 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 19.86 | 129.00 | 5.17 | 346.76 | 0.3716 | 761.0 | 465.9 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 21.01 | 128.81 | 4.98 | 347.92 | 0.3890 | -253.0 | -263.7 | |
| 0.99 | 20.84 | 0.53 | 11.16 | 20.65 | 128.73 | 4.90 | 347.90 | 0.3830 | 592.4 | 376.0 | |
| 0.00 | 2.44 | 0.00 | 1.29 | 19.44 | 128.69 | 4.86 | 347.25 | 0.3638 | 1141.0 | 955.3 | |
| 8.30 | -10.00 | 4.44 | -10.00 | 20.45 | 128.50 | 4.67 | 348.35 | 0.3791 | 948.4 | 999999 | |
| 15.79 | 34.91 | 8.44 | 18.63 | 20.42 | 127.78 | 3.95 | 350.08 | 0.3764 | 878.2 | 868.2 | |
| 13.08 | -13.00 | 6.97 | -13.00 | 19.99 | 127.67 | 3.84 | 350.13 | 0.3693 | 1131.2 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.77 | 20.25 | 126.61 | 2.78 | 352.92 | 0.3709 | 608.0 | 460.8 | |
| 0.00 | 1.71 | 0.00 | 0.89 | 15.39 | 126.13 | 2.30 | 352.32 | 0.2903 | -719.0 | -659.3 | |
| 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. | |