SDO HMI 2014-03-29 02:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.95 | 40.30 | 5.72 | 21.13 | 3.26 | 138.78 | 16.37 | 301.08 | 0.3296 | 221.3 | 104.1 | |
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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 | 0.88 | 0.00 | 0.47 | 2.53 | 143.47 | 21.06 | 293.06 | 0.3919 | -729.0 | -595.8 | |
| 0.00 | 3.07 | 0.00 | 1.64 | 3.29 | 141.92 | 19.51 | 296.60 | 0.3745 | -921.0 | -722.9 | |
| 2.19 | 3.50 | 1.17 | 1.88 | 4.75 | 141.89 | 19.49 | 300.01 | 0.3856 | -931.2 | -770.2 | |
| 0.00 | 2.72 | 0.00 | 1.45 | 4.01 | 141.87 | 19.46 | 298.37 | 0.3794 | -764.0 | -648.7 | |
| 0.00 | 1.31 | 0.00 | 0.70 | 4.29 | 141.85 | 19.44 | 299.03 | 0.3812 | -898.0 | -728.4 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 3.78 | 141.42 | 19.01 | 298.41 | 0.3712 | -726.0 | -636.5 | |
| 0.00 | 0.79 | 0.00 | 0.41 | 2.02 | 138.62 | 16.21 | 297.80 | 0.3169 | 639.0 | 513.0 | |
| 0.00 | 4.38 | 0.00 | 2.28 | 2.34 | 138.32 | 15.91 | 299.18 | 0.3150 | 812.0 | 600.3 | |
| 0.00 | 1.58 | 0.00 | 0.83 | 6.43 | 138.32 | 15.91 | 309.30 | 0.3535 | -864.0 | -691.1 | |
| 0.00 | 1.84 | 0.00 | 0.96 | 3.49 | 137.34 | 14.93 | 303.98 | 0.3115 | 850.0 | 682.9 | |
| 8.76 | 14.28 | 4.55 | 7.41 | 2.61 | 137.08 | 14.67 | 302.01 | 0.2996 | 1011.0 | 700.4 | |
| 0.00 | 1.31 | 0.00 | 0.68 | 3.52 | 137.06 | 14.65 | 304.55 | 0.3079 | 873.0 | 773.0 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 3.45 | 136.87 | 14.46 | 304.72 | 0.3047 | 886.0 | 707.9 | |
| 0.00 | 1.49 | 0.00 | 0.77 | 1.95 | 136.33 | 13.92 | 301.48 | 0.2831 | 720.0 | 596.6 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 4.37 | 136.15 | 13.74 | 308.59 | 0.3043 | 754.0 | 589.4 | |
| 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. | |