SDO HMI 2014-05-17 05:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.31 | 0.00 | 8.59 | -20.91 | 163.87 | -29.64 | 125.15 | 0.5669 | -586.1 | -475.2 | |
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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 | 1.17 | 0.00 | 0.63 | -18.19 | 174.77 | -18.74 | 131.88 | 0.4117 | 728.0 | 544.0 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -23.40 | 172.10 | -21.41 | 137.10 | 0.4941 | -781.0 | -609.6 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -29.55 | 169.70 | -23.81 | 142.59 | 0.5801 | -658.0 | -561.1 | |
| 0.00 | 1.80 | 0.00 | 1.02 | -15.11 | 166.70 | -26.81 | 117.20 | 0.4915 | -761.0 | -534.2 | |
| 0.00 | 1.26 | 0.00 | 0.77 | -23.76 | 163.48 | -30.02 | 128.85 | 0.5903 | -672.0 | -574.2 | |
| 0.00 | 1.26 | 0.00 | 0.77 | -21.87 | 161.85 | -31.66 | 124.82 | 0.5954 | -770.0 | -554.9 | |
| 0.00 | 0.54 | 0.00 | 0.33 | -21.74 | 161.54 | -31.97 | 124.39 | 0.5982 | -590.0 | -506.7 | |
| 0.00 | 1.71 | 0.00 | 1.05 | -21.42 | 161.54 | -31.97 | 123.91 | 0.5961 | -837.0 | -574.1 | |
| 0.00 | 1.35 | 0.00 | 0.83 | -20.56 | 160.60 | -32.91 | 121.97 | 0.6019 | -880.0 | -688.3 | |
| 0.00 | 1.17 | 0.00 | 0.73 | -20.55 | 160.06 | -33.45 | 121.60 | 0.6082 | -688.0 | -573.5 | |
| 0.00 | 2.43 | 0.00 | 1.51 | -20.29 | 160.00 | -33.50 | 121.18 | 0.6074 | -538.0 | -462.5 | |
| 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. | |