SDO HMI 2011-06-13 17:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.87 | 37.32 | 5.17 | 19.56 | -15.39 | 244.99 | -9.99 | 149.38 | 0.3278 | 35.5 | -82.7 | |
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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 | 1.18 | 0.00 | 0.61 | -16.92 | 251.14 | -3.84 | 168.12 | 0.3125 | 815.0 | 651.2 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -14.96 | 248.24 | -6.74 | 157.33 | 0.2956 | 858.0 | 626.6 | |
| 0.00 | 1.09 | 0.00 | 0.56 | -14.77 | 248.09 | -6.90 | 156.61 | 0.2937 | 906.0 | 723.5 | |
| 0.00 | 1.09 | 0.00 | 0.56 | -13.98 | 248.11 | -6.87 | 155.53 | 0.2815 | 776.0 | 733.0 | |
| 0.00 | 1.63 | 0.00 | 0.85 | -15.53 | 247.52 | -7.46 | 156.01 | 0.3091 | 873.0 | 806.8 | |
| 5.16 | 7.88 | 2.68 | 4.10 | -14.71 | 246.47 | -8.51 | 151.82 | 0.3046 | 1054.6 | 820.8 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -14.58 | 246.16 | -8.83 | 150.75 | 0.3053 | 819.0 | 696.0 | |
| 0.00 | 2.26 | 0.00 | 1.18 | -14.74 | 245.99 | -8.99 | 150.56 | 0.3089 | 843.0 | 694.4 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -15.98 | 243.85 | -11.14 | 147.24 | 0.3446 | -1034.0 | -861.8 | |
| 0.00 | 1.45 | 0.00 | 0.77 | -15.98 | 243.52 | -11.46 | 146.50 | 0.3475 | -793.0 | -608.1 | |
| 4.71 | 8.24 | 2.49 | 4.35 | -15.73 | 243.31 | -11.67 | 145.60 | 0.3461 | -1089.5 | -926.6 | |
| 0.00 | 1.99 | 0.00 | 1.05 | -15.89 | 242.95 | -12.04 | 145.05 | 0.3516 | -854.0 | -694.6 | |
| 0.00 | 3.35 | 0.00 | 1.77 | -15.86 | 242.59 | -12.39 | 144.23 | 0.3546 | -1046.0 | -749.5 | |
| 0.00 | 1.99 | 0.00 | 1.06 | -15.99 | 242.49 | -12.50 | 144.22 | 0.3573 | -837.0 | -703.8 | |
| 0.00 | 1.00 | 0.00 | 0.53 | -15.76 | 242.31 | -12.68 | 143.45 | 0.3561 | -794.0 | -661.2 | |
| 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. | |