SDO HMI 2014-04-08 09:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.40 | 0.00 | 10.50 | -9.12 | 10.42 | 23.78 | 260.88 | 0.4052 | 662.8 | 626.7 | |
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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 | 1.15 | 0.00 | 0.63 | -10.56 | 12.12 | 25.48 | 258.26 | 0.4338 | -712.0 | -586.9 | |
| 0.00 | 1.32 | 0.00 | 0.72 | -8.16 | 11.90 | 25.27 | 263.79 | 0.4268 | 759.0 | 558.5 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -8.34 | 11.88 | 25.25 | 263.36 | 0.4266 | 750.0 | 588.1 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -8.04 | 11.76 | 25.12 | 264.04 | 0.4245 | 771.0 | 660.2 | |
| 0.00 | 4.76 | 0.00 | 2.59 | -8.36 | 11.35 | 24.71 | 263.23 | 0.4183 | 990.0 | 815.0 | |
| 0.00 | 1.50 | 0.00 | 0.82 | -8.61 | 11.23 | 24.59 | 262.62 | 0.4167 | 894.0 | 777.3 | |
| 0.00 | 2.73 | 0.00 | 1.48 | -8.80 | 10.94 | 24.31 | 262.10 | 0.4124 | 569.0 | 685.9 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -8.72 | 10.77 | 24.13 | 262.27 | 0.4096 | 886.0 | 764.1 | |
| 0.00 | 1.50 | 0.00 | 0.81 | -9.05 | 10.63 | 23.99 | 261.42 | 0.4078 | 922.0 | 677.1 | |
| 0.00 | 1.15 | 0.00 | 0.62 | -10.53 | 9.21 | 22.57 | 257.28 | 0.3885 | 682.0 | 627.2 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -11.75 | 4.53 | 17.89 | 251.03 | 0.3195 | 668.0 | 610.4 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -11.85 | 4.09 | 17.45 | 250.32 | 0.3131 | 774.0 | 606.5 | |
| 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. | |