SDO HMI 2011-01-07 09:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.10 | 27.16 | 0.67 | 16.64 | -13.96 | 205.84 | 34.96 | 251.20 | 0.5895 | -645.0 | -553.6 | |
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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 | 1.27 | 0.00 | 0.84 | -15.89 | 210.73 | 39.85 | 249.92 | 0.6586 | 712.0 | 495.3 | |
| 0.00 | 0.85 | 0.00 | 0.53 | -13.91 | 208.08 | 37.20 | 252.08 | 0.6191 | -590.0 | -488.4 | |
| 0.00 | 2.04 | 0.00 | 1.26 | -13.45 | 206.71 | 35.83 | 252.36 | 0.5997 | -568.0 | -429.5 | |
| 0.00 | 0.85 | 0.00 | 0.53 | -13.93 | 206.75 | 35.88 | 251.60 | 0.6018 | -657.0 | -569.6 | |
| 0.00 | 1.27 | 0.00 | 0.79 | -14.06 | 206.59 | 35.71 | 251.33 | 0.6000 | -654.0 | -521.0 | |
| 0.00 | 0.85 | 0.00 | 0.52 | -13.76 | 206.50 | 35.62 | 251.78 | 0.5978 | -678.0 | -498.7 | |
| 0.00 | 2.12 | 0.00 | 1.30 | -13.72 | 205.90 | 35.02 | 251.63 | 0.5897 | -759.0 | -591.9 | |
| 0.00 | 1.61 | 0.00 | 0.98 | -13.65 | 205.44 | 34.56 | 251.58 | 0.5833 | -769.0 | -735.3 | |
| 0.00 | 2.46 | 0.00 | 1.50 | -13.95 | 205.34 | 34.47 | 251.03 | 0.5830 | -923.0 | -775.2 | |
| 0.00 | 1.19 | 0.00 | 0.72 | -13.33 | 205.16 | 34.29 | 252.02 | 0.5786 | -721.0 | -562.4 | |
| 0.00 | 1.19 | 0.00 | 0.72 | -13.75 | 205.16 | 34.28 | 251.31 | 0.5799 | -925.0 | -795.4 | |
| 0.00 | 2.97 | 0.00 | 1.81 | -14.23 | 205.24 | 34.37 | 250.54 | 0.5826 | -716.0 | -597.8 | |
| 0.00 | 4.08 | 0.00 | 2.47 | -13.46 | 204.93 | 34.05 | 251.71 | 0.5758 | -750.0 | -622.6 | |
| 1.10 | 1.95 | 0.67 | 1.18 | -13.85 | 204.92 | 34.04 | 251.05 | 0.5770 | -908.8 | -743.0 | |
| 0.00 | 1.02 | 0.00 | 0.62 | -16.01 | 205.13 | 34.25 | 247.53 | 0.5877 | -713.0 | -498.8 | |
| 0.00 | 1.44 | 0.00 | 0.87 | -13.95 | 204.72 | 33.84 | 250.80 | 0.5745 | -787.0 | -622.8 | |
| 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. | |