SDO HMI 2011-06-04 20:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.06 | 146.46 | 12.28 | 78.09 | -20.97 | 18.71 | 6.28 | 196.19 | 0.3713 | 716.0 | 410.9 | |
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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 | 1.27 | 0.00 | 0.67 | -19.55 | 20.13 | 7.70 | 200.91 | 0.3551 | -749.0 | -406.0 | |
| 20.98 | 121.69 | 11.17 | 64.80 | -20.68 | 19.40 | 6.97 | 198.02 | 0.3684 | 1320.1 | 499.2 | |
| 0.00 | 3.89 | 0.00 | 2.09 | -22.51 | 18.70 | 6.26 | 194.90 | 0.3934 | 775.0 | 704.3 | |
| 0.00 | 1.18 | 0.00 | 0.63 | -21.49 | 18.36 | 5.92 | 194.84 | 0.3762 | 996.0 | 833.1 | |
| 0.00 | 1.63 | 0.00 | 0.87 | -22.12 | 18.35 | 5.91 | 194.38 | 0.3859 | 740.0 | 598.1 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -21.36 | 18.25 | 5.82 | 194.69 | 0.3738 | 687.0 | 638.2 | |
| 2.08 | 2.62 | 1.11 | 1.40 | -21.79 | 18.20 | 5.77 | 194.27 | 0.3802 | 940.1 | 964.5 | |
| 0.00 | 2.08 | 0.00 | 1.11 | -21.14 | 18.08 | 5.64 | 194.44 | 0.3695 | 868.0 | 645.4 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -25.10 | 16.03 | 3.59 | 187.69 | 0.4256 | 750.0 | 585.1 | |
| 0.00 | 2.08 | 0.00 | 1.13 | -24.40 | 11.90 | -0.54 | 178.80 | 0.4107 | -790.0 | -530.8 | |
| 0.00 | 4.43 | 0.00 | 2.35 | -21.30 | 11.19 | -1.25 | 176.77 | 0.3610 | -773.0 | -744.8 | |
| 0.00 | 0.81 | 0.00 | 0.44 | -22.74 | 10.68 | -1.75 | 175.78 | 0.3850 | -811.0 | -665.7 | |
| 0.00 | 2.80 | 0.00 | 1.53 | -24.90 | 10.15 | -2.29 | 175.04 | 0.4201 | -815.0 | -647.3 | |
| 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. | |