SDO HMI 2014-04-14 10:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.80 | 86.98 | 17.84 | 47.30 | -9.37 | 242.72 | -24.16 | 100.28 | 0.4124 | 458.1 | 153.8 | |
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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 | 1.24 | 0.00 | 0.65 | -11.18 | 248.71 | -18.18 | 108.28 | 0.3237 | 886.0 | 645.4 | |
| 0.00 | 1.59 | 0.00 | 0.85 | -9.87 | 245.68 | -21.21 | 102.66 | 0.3668 | 676.0 | 475.9 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -10.61 | 245.13 | -21.75 | 104.34 | 0.3776 | 808.0 | 565.3 | |
| 0.00 | 1.59 | 0.00 | 0.85 | -9.20 | 244.77 | -22.11 | 100.52 | 0.3796 | 890.0 | 726.5 | |
| 0.00 | 0.80 | 0.00 | 0.43 | -10.09 | 244.15 | -22.74 | 102.55 | 0.3915 | 726.0 | 639.7 | |
| 0.00 | 1.15 | 0.00 | 0.62 | -5.57 | 244.28 | -22.60 | 90.90 | 0.3842 | 835.0 | 702.8 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -10.02 | 243.29 | -23.60 | 102.05 | 0.4048 | 646.0 | 447.1 | |
| 18.12 | 26.52 | 9.83 | 14.38 | -8.38 | 242.87 | -24.01 | 97.90 | 0.4081 | 1009.0 | 662.3 | |
| 1.50 | 47.74 | 0.82 | 26.04 | -10.06 | 242.68 | -24.20 | 101.92 | 0.4143 | -893.2 | -145.5 | |
| 0.00 | 2.03 | 0.00 | 1.11 | -8.51 | 242.46 | -24.42 | 98.14 | 0.4148 | 568.0 | 500.7 | |
| 10.26 | -9.00 | 5.59 | -9.00 | -9.83 | 242.33 | -24.55 | 101.26 | 0.4192 | -1003.5 | 999999 | |
| 1.24 | -9.00 | 0.68 | -9.00 | -10.00 | 241.98 | -24.90 | 101.54 | 0.4250 | 1028.3 | 999999 | |
| 1.68 | -9.00 | 0.92 | -9.00 | -9.76 | 242.00 | -24.88 | 100.98 | 0.4242 | 870.6 | 999999 | |
| 0.00 | 1.41 | 0.00 | 0.78 | -10.62 | 241.01 | -25.87 | 102.64 | 0.4414 | 823.0 | 720.8 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -11.52 | 240.69 | -26.20 | 104.51 | 0.4487 | 820.0 | 648.6 | |
| 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. | |