SDO HMI 2014-09-23 22:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.27 | 0.00 | 10.58 | -14.25 | 289.58 | 11.38 | 207.22 | 0.4299 | 711.4 | 578.8 | |
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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 | 2.92 | 0.00 | 1.63 | -10.15 | 299.91 | 21.71 | 231.79 | 0.4652 | 647.0 | 559.9 | |
| 0.00 | 1.24 | 0.00 | 0.69 | -9.16 | 299.62 | 21.41 | 233.13 | 0.4524 | 784.0 | 677.3 | |
| 0.00 | 2.12 | 0.00 | 1.18 | -10.38 | 299.47 | 21.26 | 230.82 | 0.4621 | 587.0 | 647.6 | |
| 0.00 | 0.71 | 0.00 | 0.38 | -11.62 | 291.70 | 13.49 | 215.85 | 0.3919 | 846.0 | 722.1 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -15.24 | 289.13 | 10.92 | 205.90 | 0.4204 | 636.0 | 510.3 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -12.22 | 286.78 | 8.57 | 203.92 | 0.3606 | 627.0 | 516.1 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -12.67 | 286.67 | 8.46 | 203.15 | 0.3666 | 647.0 | 408.2 | |
| 0.00 | 2.48 | 0.00 | 1.42 | -21.65 | 286.98 | 8.78 | 196.51 | 0.5010 | 812.0 | 616.5 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -23.35 | 282.70 | 4.49 | 188.11 | 0.5123 | 639.0 | 524.3 | |
| 0.00 | 1.33 | 0.00 | 0.70 | -13.72 | 281.94 | 3.73 | 190.13 | 0.3610 | 725.0 | 624.4 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -13.62 | 281.78 | 3.57 | 189.76 | 0.3590 | 727.0 | 532.5 | |
| 0.00 | 1.50 | 0.00 | 0.82 | -17.73 | 281.56 | 3.36 | 187.59 | 0.4239 | 773.0 | 575.5 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -14.13 | 281.32 | 3.11 | 188.31 | 0.3661 | 848.0 | 631.1 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -14.33 | 281.14 | 2.93 | 187.75 | 0.3687 | 662.0 | 458.1 | |
| 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. | |