SDO HMI 2014-01-13 02:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.29 | 0.00 | 10.84 | 16.65 | 24.26 | -6.08 | 15.69 | 0.3750 | 439.2 | 291.9 | |
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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 | 1.19 | 0.00 | 0.63 | 16.12 | 27.98 | -2.36 | 6.47 | 0.3534 | -962.0 | -806.1 | |
| 0.00 | 2.72 | 0.00 | 1.45 | 16.75 | 27.54 | -2.80 | 7.41 | 0.3646 | -881.0 | -646.9 | |
| 0.00 | 1.44 | 0.00 | 0.77 | 16.86 | 26.18 | -4.16 | 10.87 | 0.3698 | 690.0 | 544.1 | |
| 0.00 | 1.44 | 0.00 | 0.76 | 15.54 | 25.63 | -4.72 | 13.12 | 0.3506 | -831.0 | -613.5 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 16.90 | 24.58 | -5.77 | 14.88 | 0.3763 | 730.0 | 588.7 | |
| 0.00 | 0.68 | 0.00 | 0.36 | 17.38 | 24.00 | -6.34 | 15.92 | 0.3862 | 614.0 | 448.2 | |
| 0.00 | 1.87 | 0.00 | 0.99 | 15.87 | 23.80 | -6.54 | 17.62 | 0.3637 | 923.0 | 757.3 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 16.12 | 23.80 | -6.55 | 17.42 | 0.3676 | 913.0 | 684.1 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 16.79 | 22.97 | -7.38 | 18.86 | 0.3821 | 864.0 | 577.8 | |
| 0.00 | 1.95 | 0.00 | 1.05 | 17.02 | 22.68 | -7.67 | 19.33 | 0.3871 | 909.0 | 750.8 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 17.50 | 22.19 | -8.16 | 20.02 | 0.3970 | 779.0 | 567.6 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 16.52 | 22.23 | -8.11 | 20.84 | 0.3820 | 786.0 | 653.4 | |
| 0.00 | 1.10 | 0.00 | 0.59 | 17.05 | 22.18 | -8.17 | 20.45 | 0.3904 | 740.0 | 652.5 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 16.74 | 21.97 | -8.37 | 21.22 | 0.3869 | 746.0 | 636.0 | |
| 0.00 | 0.93 | 0.00 | 0.50 | 17.00 | 21.71 | -8.63 | 21.57 | 0.3922 | 568.0 | 529.9 | |
| 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. | |