SDO HMI 2011-06-25 05:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.45 | 58.22 | 11.92 | 66.27 | 16.97 | 166.34 | 63.59 | 287.83 | 0.9014 | -124.7 | -235.0 | |
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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 | 1.91 | 0.00 | 2.27 | 15.89 | 167.76 | 65.02 | 286.49 | 0.9109 | -277.0 | -305.5 | |
| 0.00 | 0.64 | 0.00 | 0.74 | 14.84 | 167.07 | 64.33 | 285.40 | 0.9054 | -514.0 | -473.3 | |
| 0.00 | 1.09 | 0.00 | 1.28 | 15.99 | 167.45 | 64.70 | 286.64 | 0.9088 | -604.0 | -563.9 | |
| 2.18 | 11.62 | 2.59 | 13.78 | 16.40 | 167.63 | 64.88 | 287.07 | 0.9103 | -574.6 | -540.1 | |
| 2.09 | -4.00 | 2.49 | -4.00 | 16.65 | 167.71 | 64.97 | 287.33 | 0.9111 | -469.7 | 999999 | |
| 0.00 | 1.09 | 0.00 | 1.27 | 15.98 | 167.07 | 64.32 | 286.65 | 0.9061 | -584.0 | -490.3 | |
| 0.00 | 1.82 | 0.00 | 2.15 | 16.91 | 167.58 | 64.83 | 287.63 | 0.9103 | -540.0 | -490.8 | |
| 0.00 | 1.63 | 0.00 | 2.14 | 19.92 | 169.76 | 67.01 | 290.66 | 0.9267 | 301.0 | 283.9 | |
| 0.00 | 1.73 | 0.00 | 1.99 | 16.14 | 166.94 | 64.20 | 286.84 | 0.9054 | -590.0 | -490.9 | |
| 0.91 | 5.27 | 1.01 | 5.90 | 16.02 | 165.86 | 63.11 | 286.82 | 0.8974 | 186.8 | -173.4 | |
| 0.00 | 3.72 | 0.00 | 4.14 | 16.53 | 165.73 | 62.99 | 287.40 | 0.8969 | -300.0 | -209.3 | |
| 0.00 | 0.82 | 0.00 | 0.90 | 16.73 | 165.43 | 62.68 | 287.66 | 0.8948 | 300.0 | 255.3 | |
| 5.27 | 24.52 | 5.83 | 27.29 | 17.39 | 165.55 | 62.80 | 288.38 | 0.8962 | 331.2 | -149.9 | |
| 0.00 | 1.00 | 0.00 | 1.12 | 18.02 | 165.94 | 63.19 | 289.03 | 0.8997 | 198.0 | 139.6 | |
| 0.00 | 1.36 | 0.00 | 1.30 | 19.31 | 160.40 | 57.66 | 291.33 | 0.8580 | 290.0 | 220.8 | |
| 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. | |