SDO HMI 2014-07-18 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.51 | 70.81 | 10.80 | 37.20 | 6.95 | 112.42 | 19.43 | 277.77 | 0.3347 | -34.2 | 163.6 | |
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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 |
| 3.99 | 12.17 | 2.12 | 6.45 | 7.39 | 113.86 | 20.87 | 278.60 | 0.3588 | -979.5 | -640.8 | |
| 0.00 | 2.36 | 0.00 | 1.25 | 7.63 | 113.87 | 20.88 | 279.28 | 0.3595 | -867.0 | -705.2 | |
| 0.64 | 1.82 | 0.34 | 0.96 | 6.84 | 113.80 | 20.81 | 277.09 | 0.3570 | -860.6 | -754.7 | |
| 4.18 | -1.00 | 2.21 | -1.00 | 7.24 | 113.66 | 20.66 | 278.26 | 0.3552 | -1092.8 | 999999 | |
| 0.45 | 9.71 | 0.24 | 5.13 | 7.03 | 113.38 | 20.39 | 277.75 | 0.3505 | -918.6 | -546.8 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 6.73 | 113.34 | 20.34 | 276.90 | 0.3493 | -759.0 | -554.0 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 7.05 | 112.83 | 19.84 | 277.96 | 0.3415 | 700.0 | 536.7 | |
| 0.00 | 2.54 | 0.00 | 1.34 | 6.72 | 112.59 | 19.59 | 277.06 | 0.3370 | -493.0 | -255.5 | |
| 0.54 | 1.18 | 0.29 | 0.62 | 7.82 | 112.51 | 19.51 | 280.34 | 0.3378 | -939.0 | -803.7 | |
| 6.72 | 29.50 | 3.52 | 15.43 | 6.71 | 111.84 | 18.84 | 277.24 | 0.3248 | 956.7 | 644.1 | |
| 3.45 | -10.00 | 1.80 | -10.00 | 6.90 | 111.52 | 18.53 | 277.93 | 0.3199 | 1033.6 | 999999 | |
| 0.00 | 3.72 | 0.00 | 1.94 | 6.58 | 111.12 | 18.13 | 277.02 | 0.3128 | 1277.0 | 917.5 | |
| 0.54 | 4.54 | 0.28 | 2.37 | 6.82 | 111.00 | 18.01 | 277.85 | 0.3112 | 1079.3 | 796.4 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 6.87 | 110.62 | 17.62 | 278.12 | 0.3049 | 817.0 | 571.2 | |
| 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. | |