SDO HMI 2014-01-12 07:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.66 | 110.03 | 29.95 | 57.15 | -17.86 | 29.64 | -11.15 | 142.19 | 0.3009 | 83.6 | 233.1 | |
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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 |
| 1.28 | 61.98 | 0.66 | 32.08 | -17.87 | 30.81 | -9.98 | 145.08 | 0.2894 | 847.9 | 611.3 | |
| 21.43 | -1.00 | 11.07 | -1.00 | -17.56 | 30.61 | -10.18 | 143.89 | 0.2872 | 1169.9 | 999999 | |
| 0.00 | 1.87 | 0.00 | 0.97 | -17.17 | 30.60 | -10.19 | 143.01 | 0.2822 | 978.0 | 807.4 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -18.13 | 30.32 | -10.47 | 144.36 | 0.2976 | 783.0 | 724.7 | |
| 8.25 | -1.00 | 4.27 | -1.00 | -17.68 | 30.16 | -10.63 | 142.99 | 0.2932 | 904.9 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -18.27 | 29.49 | -11.30 | 142.61 | 0.3077 | -621.0 | -584.7 | |
| 0.00 | 1.70 | 0.00 | 0.88 | -17.54 | 29.44 | -11.34 | 140.93 | 0.2989 | -92.0 | -0.5 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -18.45 | 29.07 | -11.72 | 141.98 | 0.3143 | -424.0 | -309.1 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -16.51 | 29.16 | -11.62 | 137.86 | 0.2892 | 775.0 | 586.2 | |
| 1.19 | 2.30 | 0.62 | 1.20 | -18.63 | 28.67 | -12.12 | 141.44 | 0.3205 | -1046.8 | -828.2 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -18.11 | 28.68 | -12.11 | 140.37 | 0.3140 | -377.0 | -303.8 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -17.96 | 28.62 | -12.16 | 139.92 | 0.3127 | -71.0 | -105.1 | |
| 25.51 | 35.37 | 13.33 | 18.48 | -18.28 | 28.25 | -12.54 | 139.80 | 0.3207 | -1088.1 | -744.0 | |
| 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. | |