SDO HMI 2014-05-23 00:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.15 | 125.80 | 25.71 | 101.76 | -10.90 | 65.16 | -51.73 | 102.44 | 0.7907 | 500.9 | 237.8 | |
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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 | 0.90 | 0.00 | 0.70 | -8.76 | 67.07 | -49.82 | 99.96 | 0.7689 | -238.0 | -228.7 | |
| 20.80 | 98.52 | 16.25 | 77.07 | -10.54 | 66.65 | -50.24 | 102.19 | 0.7754 | 966.8 | 316.7 | |
| 0.27 | -2.00 | 0.21 | -2.00 | -10.87 | 66.33 | -50.56 | 102.57 | 0.7793 | 347.0 | 999999 | |
| 0.00 | 1.89 | 0.00 | 1.51 | -12.59 | 65.89 | -51.00 | 104.69 | 0.7863 | 535.0 | 461.5 | |
| 0.00 | 0.90 | 0.00 | 0.73 | -8.86 | 64.79 | -52.10 | 99.84 | 0.7935 | 461.0 | 394.2 | |
| 4.68 | 6.66 | 4.15 | 5.91 | -11.02 | 61.21 | -55.68 | 102.11 | 0.8312 | 687.7 | 482.5 | |
| 0.00 | 1.89 | 0.00 | 1.70 | -11.57 | 60.83 | -56.06 | 102.72 | 0.8354 | 413.0 | 319.0 | |
| 0.00 | 2.61 | 0.00 | 2.42 | -12.78 | 59.68 | -57.21 | 104.02 | 0.8470 | -294.0 | -246.3 | |
| 3.24 | 10.18 | 3.05 | 9.60 | -12.76 | 59.11 | -57.78 | 103.93 | 0.8522 | -654.7 | -404.2 | |
| 0.00 | 2.25 | 0.00 | 2.12 | -12.26 | 59.05 | -57.84 | 103.34 | 0.8523 | -565.0 | -432.1 | |
| 2.16 | -9.00 | 2.05 | -9.00 | -12.60 | 58.87 | -58.02 | 103.72 | 0.8541 | -447.4 | 999999 | |
| 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. | |