SDO HMI 2014-10-10 12:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.02 | 0.00 | 10.94 | -20.32 | 73.51 | 14.11 | 207.19 | 0.5089 | 225.7 | 163.2 | |
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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 | 1.05 | 0.00 | 0.66 | -23.26 | 83.48 | 24.08 | 217.80 | 0.6137 | 670.0 | 552.5 | |
| 0.00 | 1.49 | 0.00 | 0.87 | -19.14 | 79.19 | 19.79 | 217.18 | 0.5314 | 684.0 | 454.8 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -17.03 | 78.91 | 19.51 | 219.44 | 0.5048 | 809.0 | 648.4 | |
| 0.00 | 1.23 | 0.00 | 0.73 | -21.45 | 79.36 | 19.96 | 214.76 | 0.5595 | 797.0 | 620.8 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -18.61 | 78.29 | 18.89 | 216.55 | 0.5173 | 622.0 | 459.9 | |
| 0.00 | 2.02 | 0.00 | 1.14 | -16.88 | 76.62 | 17.22 | 216.20 | 0.4817 | 546.0 | 579.9 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -17.45 | 76.21 | 16.82 | 214.84 | 0.4851 | 619.0 | 486.6 | |
| 0.00 | 1.05 | 0.00 | 0.59 | -16.64 | 75.46 | 16.06 | 214.61 | 0.4685 | 674.0 | 560.8 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -17.06 | 75.30 | 15.90 | 213.83 | 0.4723 | 643.0 | 567.9 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -23.34 | 68.60 | 9.20 | 196.63 | 0.5151 | -743.0 | -493.1 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -16.07 | 68.13 | 8.73 | 201.13 | 0.4064 | 769.0 | 638.7 | |
| 0.00 | 1.84 | 0.00 | 1.06 | -23.64 | 68.26 | 8.86 | 195.87 | 0.5180 | -677.0 | -535.5 | |
| 0.00 | 1.75 | 0.00 | 1.01 | -23.77 | 67.87 | 8.47 | 195.14 | 0.5183 | -717.0 | -604.8 | |
| 0.00 | 1.05 | 0.00 | 0.61 | -23.94 | 67.48 | 8.08 | 194.39 | 0.5192 | -599.0 | -441.9 | |
| 0.00 | 1.31 | 0.00 | 0.76 | -24.75 | 62.79 | 3.39 | 185.97 | 0.5188 | -711.0 | -619.2 | |
| 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. | |