SDO HMI 2014-04-22 18:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.85 | 0.00 | 9.45 | -9.21 | 137.79 | -19.04 | 106.28 | 0.3384 | 792.1 | 635.8 | |
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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 | 0.89 | 0.00 | 0.45 | -13.88 | 149.42 | -7.42 | 141.13 | 0.2005 | 889.0 | 757.8 | |
| 0.00 | 1.33 | 0.00 | 0.67 | -14.22 | 149.31 | -7.52 | 141.79 | 0.2061 | 826.0 | 648.9 | |
| 0.00 | 0.98 | 0.00 | 0.49 | -6.81 | 146.24 | -10.59 | 100.37 | 0.1863 | 975.0 | 785.5 | |
| 0.00 | 0.80 | 0.00 | 0.40 | -6.99 | 146.05 | -10.78 | 101.14 | 0.1900 | 784.0 | 604.7 | |
| 0.00 | 1.24 | 0.00 | 0.64 | -10.02 | 143.40 | -13.43 | 111.50 | 0.2470 | 798.0 | 601.7 | |
| 0.00 | 2.22 | 0.00 | 1.14 | -9.62 | 141.65 | -15.18 | 107.98 | 0.2727 | 959.0 | 785.5 | |
| 0.00 | 2.31 | 0.00 | 1.22 | -6.80 | 136.99 | -19.84 | 96.25 | 0.3405 | 914.0 | 586.0 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -8.93 | 136.36 | -20.47 | 102.12 | 0.3549 | 773.0 | 618.2 | |
| 0.00 | 0.98 | 0.00 | 0.52 | -9.23 | 136.31 | -20.52 | 102.93 | 0.3566 | 797.0 | 691.1 | |
| 0.00 | 1.33 | 0.00 | 0.72 | -2.60 | 132.99 | -23.84 | 85.16 | 0.4070 | 759.0 | 669.4 | |
| 0.00 | 1.07 | 0.00 | 0.59 | -13.57 | 131.72 | -25.11 | 110.87 | 0.4433 | 809.0 | 659.4 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -6.04 | 129.98 | -26.85 | 93.55 | 0.4519 | 822.0 | 704.3 | |
| 0.00 | 1.33 | 0.00 | 0.75 | -11.10 | 128.54 | -28.29 | 104.09 | 0.4814 | 461.0 | 402.7 | |
| 0.00 | 1.24 | 0.00 | 0.71 | -10.85 | 127.09 | -29.74 | 103.12 | 0.5022 | 523.0 | 451.1 | |
| 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. | |