SDO HMI 2011-06-25 01:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.88 | 52.65 | 16.68 | 56.01 | 16.98 | 166.42 | 61.48 | 288.11 | 0.8858 | -5.1 | -260.2 | |
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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 | 1.00 | 0.00 | 1.10 | 15.97 | 167.88 | 62.94 | 286.81 | 0.8962 | -457.0 | -398.8 | |
| 1.18 | 9.90 | 1.30 | 10.92 | 16.55 | 167.65 | 62.71 | 287.47 | 0.8949 | -635.8 | -491.7 | |
| 0.82 | 1.72 | 0.99 | 2.09 | 20.03 | 169.95 | 65.01 | 291.03 | 0.9140 | 211.7 | 288.5 | |
| 0.00 | 2.72 | 0.00 | 2.94 | 16.09 | 167.12 | 62.18 | 287.02 | 0.8905 | -590.0 | -521.7 | |
| 0.00 | 1.54 | 0.00 | 1.66 | 16.29 | 166.88 | 61.94 | 287.27 | 0.8889 | -656.0 | -553.5 | |
| 0.27 | 8.17 | 0.29 | 8.56 | 16.03 | 166.14 | 61.20 | 287.07 | 0.8829 | -100.7 | -268.6 | |
| 2.72 | -6.00 | 2.84 | -6.00 | 16.04 | 165.94 | 61.00 | 287.10 | 0.8814 | 246.2 | 999999 | |
| 0.00 | 1.45 | 0.00 | 1.61 | 19.24 | 167.52 | 62.58 | 290.48 | 0.8964 | -486.0 | -354.0 | |
| 0.00 | 1.36 | 0.00 | 1.42 | 16.74 | 165.85 | 60.91 | 287.90 | 0.8813 | -22.0 | -90.5 | |
| 2.63 | 21.52 | 2.73 | 22.33 | 17.06 | 165.77 | 60.83 | 288.27 | 0.8810 | -393.1 | -83.4 | |
| 0.00 | 1.18 | 0.00 | 1.24 | 17.78 | 165.98 | 61.04 | 289.06 | 0.8834 | 216.0 | 140.6 | |
| 6.99 | -10.00 | 7.21 | -10.00 | 17.06 | 165.51 | 60.57 | 288.31 | 0.8789 | 370.0 | 999999 | |
| 1.27 | -10.00 | 1.32 | -10.00 | 17.51 | 165.62 | 60.68 | 288.80 | 0.8803 | 314.9 | 999999 | |
| 0.00 | 1.09 | 0.00 | 1.15 | 19.00 | 165.85 | 60.91 | 290.45 | 0.8837 | 292.0 | 272.3 | |
| 0.00 | 1.00 | 0.00 | 0.99 | 18.81 | 163.73 | 58.79 | 290.57 | 0.8667 | -391.0 | -335.6 | |
| 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. | |