SDO HMI 2014-07-07 20:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.13 | 163.15 | 20.48 | 90.33 | 6.64 | 203.88 | -26.41 | 82.27 | 0.4476 | -752.7 | -357.8 | |
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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 | 2.54 | 0.00 | 1.36 | 6.57 | 207.80 | -22.50 | 81.47 | 0.3860 | -755.0 | -629.6 | |
| 0.00 | 1.09 | 0.00 | 0.60 | 6.33 | 205.46 | -24.83 | 82.65 | 0.4226 | -849.0 | -661.2 | |
| 7.44 | 9.99 | 4.08 | 5.47 | 7.18 | 205.11 | -25.18 | 80.75 | 0.4295 | -1043.6 | -669.4 | |
| 28.69 | 134.27 | 15.84 | 74.12 | 6.45 | 204.16 | -26.13 | 82.64 | 0.4431 | -1314.7 | -404.5 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 7.05 | 203.82 | -26.47 | 81.37 | 0.4493 | -468.0 | -344.6 | |
| 1.00 | 4.09 | 0.56 | 2.27 | 8.79 | 203.50 | -26.80 | 77.66 | 0.4580 | -775.4 | -694.7 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 8.35 | 203.04 | -27.25 | 78.76 | 0.4638 | -686.0 | -603.8 | |
| 0.00 | 1.18 | 0.00 | 0.68 | 7.22 | 200.14 | -30.15 | 81.77 | 0.5055 | 663.0 | 498.3 | |
| 0.00 | 1.18 | 0.00 | 0.69 | 6.14 | 198.53 | -31.76 | 84.11 | 0.5282 | 582.0 | 446.8 | |
| 0.00 | 1.00 | 0.00 | 0.59 | 8.35 | 198.11 | -32.19 | 80.01 | 0.5372 | 852.0 | 625.1 | |
| 0.00 | 2.00 | 0.00 | 1.19 | 9.08 | 196.79 | -33.51 | 78.98 | 0.5575 | 578.0 | 534.0 | |
| 0.00 | 1.36 | 0.00 | 0.81 | 7.00 | 196.83 | -33.46 | 82.71 | 0.5539 | 729.0 | 510.9 | |
| 0.00 | 1.00 | 0.00 | 0.60 | 9.04 | 196.57 | -33.73 | 79.10 | 0.5606 | 566.0 | 399.4 | |
| 0.00 | 1.00 | 0.00 | 0.59 | 5.99 | 196.72 | -33.57 | 84.55 | 0.5546 | 609.0 | 490.5 | |
| 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. | |