SDO HMI 2014-04-19 07:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.15 | 152.50 | 18.54 | 107.56 | -9.16 | 247.92 | 45.43 | 262.26 | 0.7113 | 452.5 | 189.0 | |
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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 |
| 7.45 | 103.83 | 5.40 | 75.19 | -8.91 | 249.65 | 47.15 | 262.72 | 0.7325 | 866.8 | 229.3 | |
| 12.50 | -1.00 | 9.01 | -1.00 | -8.84 | 249.32 | 46.83 | 262.81 | 0.7286 | 1033.2 | 999999 | |
| 0.00 | 4.43 | 0.00 | 3.16 | -8.79 | 248.74 | 46.24 | 262.86 | 0.7216 | 848.0 | 659.2 | |
| 1.06 | 2.13 | 0.75 | 1.50 | -8.94 | 248.23 | 45.73 | 262.63 | 0.7156 | 732.8 | 622.3 | |
| 0.00 | 0.71 | 0.00 | 0.47 | -10.22 | 244.77 | 42.27 | 260.58 | 0.6734 | -525.0 | -440.6 | |
| 0.00 | 2.22 | 0.00 | 1.47 | -10.06 | 244.34 | 41.84 | 260.78 | 0.6676 | -744.0 | -534.5 | |
| 0.00 | 3.72 | 0.00 | 2.47 | -10.37 | 244.34 | 41.84 | 260.33 | 0.6680 | -750.0 | -616.6 | |
| 0.00 | 1.06 | 0.00 | 0.70 | -9.00 | 243.81 | 41.31 | 262.34 | 0.6602 | 502.0 | 515.5 | |
| 3.81 | 25.09 | 2.51 | 16.57 | -10.03 | 243.88 | 41.38 | 260.79 | 0.6617 | -851.8 | 95.4 | |
| 0.80 | 2.13 | 0.52 | 1.40 | -10.37 | 243.73 | 41.23 | 260.26 | 0.6601 | -772.0 | -672.3 | |
| 0.53 | 1.68 | 0.35 | 1.10 | -9.84 | 243.48 | 40.98 | 261.04 | 0.6565 | -687.8 | -539.1 | |
| 0.00 | 2.22 | 0.00 | 1.43 | -9.24 | 242.39 | 39.89 | 261.88 | 0.6417 | 664.0 | 690.9 | |
| 0.00 | 2.22 | 0.00 | 1.43 | -9.46 | 242.22 | 39.72 | 261.52 | 0.6396 | 696.0 | 564.8 | |
| 0.00 | 1.06 | 0.00 | 0.67 | -11.79 | 240.25 | 37.75 | 257.55 | 0.6159 | 699.0 | 524.5 | |
| 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. | |