SDO HMI 2011-12-02 00:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.91 | 157.32 | 18.43 | 121.78 | 19.25 | 104.84 | -47.64 | 65.33 | 0.7700 | -711.7 | -277.6 | |
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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 | 0.43 | 0.00 | 0.34 | 23.72 | 105.14 | -47.34 | 59.70 | 0.7821 | -581.0 | -599.4 | |
| 0.00 | 0.94 | 0.00 | 0.74 | 23.17 | 105.21 | -47.27 | 60.34 | 0.7795 | -651.0 | -561.1 | |
| 0.00 | 1.71 | 0.00 | 1.36 | 23.52 | 104.85 | -47.63 | 60.05 | 0.7841 | -481.0 | -444.5 | |
| 0.00 | 1.79 | 0.00 | 1.48 | 24.67 | 103.44 | -49.04 | 59.21 | 0.8011 | -631.0 | -481.2 | |
| 0.00 | 1.37 | 0.00 | 1.16 | 25.64 | 102.39 | -50.09 | 58.46 | 0.8136 | -581.0 | -454.6 | |
| 0.00 | 1.28 | 0.00 | 0.93 | 14.76 | 106.86 | -45.62 | 70.47 | 0.7357 | -493.0 | -370.1 | |
| 0.00 | 1.02 | 0.00 | 0.87 | 26.00 | 102.18 | -50.30 | 58.11 | 0.8166 | -486.0 | -430.7 | |
| 1.11 | 144.43 | 0.85 | 111.38 | 18.78 | 105.30 | -47.18 | 65.75 | 0.7639 | -1179.5 | -284.5 | |
| 22.80 | -8.00 | 17.58 | -8.00 | 18.94 | 104.92 | -47.56 | 65.68 | 0.7683 | -975.9 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.82 | 21.34 | 103.64 | -48.84 | 63.13 | 0.7883 | -337.0 | -205.3 | |
| 0.00 | 1.02 | 0.00 | 0.83 | 22.23 | 103.09 | -49.39 | 62.25 | 0.7964 | 643.0 | 561.8 | |
| 0.00 | 1.11 | 0.00 | 0.90 | 21.88 | 103.25 | -49.23 | 62.62 | 0.7937 | 335.0 | 276.8 | |
| 0.00 | 1.20 | 0.00 | 0.97 | 21.05 | 103.19 | -49.29 | 63.64 | 0.7918 | 475.0 | 402.9 | |
| 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. | |