SDO HMI 2014-11-29 10:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.82 | 0.00 | 13.33 | -22.95 | 93.99 | -27.22 | 133.99 | 0.5872 | -275.8 | -97.3 | |
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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 | 0.86 | 0.00 | 0.50 | -24.03 | 101.18 | -20.03 | 143.56 | 0.5288 | 692.0 | 634.3 | |
| 0.00 | 1.20 | 0.00 | 0.71 | -22.28 | 96.90 | -24.31 | 136.05 | 0.5511 | 723.0 | 617.6 | |
| 0.00 | 1.37 | 0.00 | 0.81 | -21.96 | 96.89 | -24.32 | 135.60 | 0.5481 | 579.0 | 445.2 | |
| 0.00 | 0.94 | 0.00 | 0.56 | -21.57 | 96.54 | -24.67 | 134.68 | 0.5481 | -790.0 | -609.2 | |
| 0.00 | 4.45 | 0.00 | 2.71 | -23.66 | 94.81 | -26.41 | 135.66 | 0.5852 | 780.0 | 721.3 | |
| 0.00 | 0.60 | 0.00 | 0.36 | -22.20 | 94.97 | -26.24 | 133.88 | 0.5702 | -660.0 | -553.1 | |
| 0.00 | 1.54 | 0.00 | 0.91 | -20.25 | 94.93 | -26.29 | 131.07 | 0.5534 | -751.0 | -519.6 | |
| 0.00 | 2.14 | 0.00 | 1.32 | -24.02 | 93.60 | -27.62 | 134.94 | 0.6005 | -678.0 | -407.6 | |
| 0.00 | 2.14 | 0.00 | 1.33 | -24.26 | 92.77 | -28.45 | 134.46 | 0.6108 | -773.0 | -604.2 | |
| 0.00 | 0.77 | 0.00 | 0.48 | -24.17 | 92.50 | -28.72 | 134.09 | 0.6127 | -555.0 | -412.9 | |
| 0.00 | 1.37 | 0.00 | 0.86 | -23.78 | 91.92 | -29.29 | 133.07 | 0.6151 | -767.0 | -681.5 | |
| 0.00 | 0.94 | 0.00 | 0.57 | -20.30 | 92.57 | -28.65 | 128.89 | 0.5799 | -619.0 | -497.5 | |
| 0.00 | 1.62 | 0.00 | 1.00 | -19.93 | 91.38 | -29.84 | 127.31 | 0.5903 | -483.0 | -434.7 | |
| 0.00 | 1.88 | 0.00 | 1.21 | -24.88 | 90.05 | -31.16 | 132.85 | 0.6427 | -559.0 | -420.1 | |
| 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. | |