SDO HMI 2014-07-29 06:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.19 | 190.77 | 76.25 | 578.42 | -7.28 | 227.51 | -79.42 | 98.40 | 0.9859 | 152.9 | -56.8 | |
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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 |
| 16.95 | 117.37 | 42.68 | 304.36 | -7.49 | 229.19 | -77.74 | 98.81 | 0.9813 | 425.4 | 166.6 | |
| 0.00 | 1.81 | 0.00 | 5.84 | -9.58 | 226.88 | -80.05 | 100.62 | 0.9888 | -432.0 | -391.5 | |
| 1.99 | 9.70 | 6.40 | 32.33 | -8.94 | 226.76 | -80.16 | 99.96 | 0.9889 | -251.4 | -344.8 | |
| 0.00 | 1.63 | 0.00 | 7.05 | -9.40 | 224.58 | -82.34 | 100.16 | 0.9939 | -277.0 | -278.2 | |
| 0.00 | 2.08 | 0.00 | 9.62 | -9.12 | 224.20 | -82.72 | 99.84 | 0.9945 | -350.0 | -291.0 | |
| 0.00 | 0.82 | 0.00 | 2.59 | -5.85 | 226.57 | -80.35 | 96.84 | 0.9885 | 214.0 | 190.0 | |
| 7.25 | 36.43 | 27.17 | 146.52 | -7.28 | 225.29 | -81.64 | 98.12 | 0.9919 | -62.6 | -312.3 | |
| 0.00 | 5.44 | 0.00 | 16.59 | -4.71 | 226.84 | -80.09 | 95.73 | 0.9874 | -483.0 | -403.0 | |
| 0.00 | 0.63 | 0.00 | 2.18 | -6.04 | 225.86 | -81.07 | 96.95 | 0.9903 | -150.0 | -132.6 | |
| 0.00 | 8.61 | 0.00 | 30.57 | -5.64 | 225.51 | -81.41 | 96.51 | 0.9910 | -264.0 | -232.0 | |
| 0.00 | 6.25 | 0.00 | 20.77 | -4.29 | 226.10 | -80.83 | 95.22 | 0.9892 | -218.0 | -252.8 | |
| 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. | |