SDO HMI 2014-06-29 21:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.76 | 272.72 | 104.52 | 694.34 | -20.19 | 259.04 | -76.58 | 111.27 | 0.9801 | -111.9 | -150.5 | |
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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 |
| 4.36 | 12.26 | 7.94 | 22.30 | -21.20 | 263.66 | -71.97 | 112.92 | 0.9637 | 474.1 | 305.7 | |
| 5.36 | 110.76 | 10.58 | 249.64 | -21.32 | 262.39 | -73.23 | 112.85 | 0.9690 | 47.9 | -357.1 | |
| 0.00 | 1.82 | 0.00 | 4.34 | -22.74 | 259.77 | -75.85 | 113.93 | 0.9793 | -244.0 | -291.7 | |
| 0.00 | 1.00 | 0.00 | 2.36 | -22.44 | 259.87 | -75.75 | 113.63 | 0.9788 | -438.0 | -439.5 | |
| 4.18 | 7.26 | 10.19 | 17.73 | -22.39 | 259.39 | -76.24 | 113.52 | 0.9803 | -282.7 | -188.2 | |
| 3.90 | -2.00 | 9.17 | -2.00 | -21.74 | 259.92 | -75.70 | 112.93 | 0.9783 | -440.9 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.57 | -20.32 | 261.36 | -74.27 | 111.68 | 0.9724 | -112.0 | -150.3 | |
| 4.90 | -2.00 | 11.02 | -2.00 | -20.60 | 260.34 | -75.29 | 111.83 | 0.9763 | -603.3 | 999999 | |
| 0.00 | 3.72 | 0.00 | 8.96 | -20.28 | 259.32 | -76.30 | 111.38 | 0.9796 | -157.0 | -177.6 | |
| 0.00 | 0.36 | 0.00 | 1.24 | -20.92 | 255.53 | -80.10 | 111.60 | 0.9903 | -89.0 | -112.0 | |
| 20.06 | 133.00 | 55.62 | 378.63 | -19.32 | 257.60 | -78.02 | 110.20 | 0.9845 | -32.5 | -25.2 | |
| 0.00 | 1.00 | 0.00 | 3.55 | -20.51 | 255.28 | -80.34 | 111.16 | 0.9907 | -189.0 | -188.4 | |
| 0.00 | 1.27 | 0.00 | 5.02 | -20.42 | 254.46 | -81.17 | 110.99 | 0.9924 | -144.0 | -133.4 | |
| 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. | |