SDO HMI 2014-01-14 15:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 94.59 | 466.68 | 47.95 | 236.59 | -16.44 | 12.83 | 2.76 | 192.42 | 0.2144 | 1072.5 | 407.5 | |
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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 |
| 50.06 | 291.28 | 25.41 | 147.79 | -16.61 | 13.60 | 3.53 | 195.69 | 0.2193 | 1382.8 | 441.4 | |
| 4.67 | -1.00 | 2.37 | -1.00 | -16.67 | 12.96 | 2.89 | 192.86 | 0.2176 | 1163.7 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -16.10 | 12.46 | 2.39 | 191.23 | 0.2063 | 709.0 | 632.5 | |
| 0.00 | 2.46 | 0.00 | 1.25 | -16.83 | 12.43 | 2.36 | 190.46 | 0.2184 | 531.0 | 494.6 | |
| 0.00 | 0.76 | 0.00 | 0.39 | -15.38 | 12.42 | 2.35 | 191.80 | 0.1940 | -550.0 | -320.6 | |
| 0.00 | 1.61 | 0.00 | 0.81 | -15.17 | 12.29 | 2.22 | 191.42 | 0.1901 | 948.0 | 768.7 | |
| 0.00 | 1.44 | 0.00 | 0.74 | -18.67 | 12.21 | 2.14 | 188.20 | 0.2488 | 712.0 | 532.2 | |
| 8.50 | 160.47 | 4.30 | 81.22 | -16.40 | 12.03 | 1.96 | 189.02 | 0.2101 | 1109.1 | 402.7 | |
| 31.36 | -8.00 | 15.87 | -8.00 | -16.10 | 11.84 | 1.77 | 188.39 | 0.2045 | 1345.6 | 999999 | |
| 0.00 | 0.93 | 0.00 | 0.47 | -14.72 | 11.83 | 1.76 | 189.50 | 0.1810 | -805.0 | -582.8 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -15.79 | 6.91 | -3.16 | 164.85 | 0.2041 | -862.0 | -686.2 | |
| 0.00 | 1.27 | 0.00 | 0.64 | -15.46 | 6.91 | -3.16 | 164.43 | 0.1986 | -796.0 | -614.5 | |
| 0.00 | 2.21 | 0.00 | 1.13 | -18.55 | 4.36 | -5.71 | 158.82 | 0.2622 | -893.0 | -621.8 | |
| 0.00 | 1.87 | 0.00 | 0.94 | -12.92 | 3.25 | -6.82 | 141.81 | 0.1881 | -864.0 | -714.7 | |
| 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. | |