SDO HMI 2014-09-06 18:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 101.80 | 634.78 | 93.93 | 584.31 | 14.95 | 86.60 | -58.25 | 76.84 | 0.8457 | 172.1 | -116.8 | |
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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 | 0.27 | 0.00 | 0.23 | 15.45 | 89.94 | -54.92 | 76.15 | 0.8146 | -313.0 | -301.3 | |
| 0.00 | 2.68 | 0.00 | 2.33 | 12.23 | 88.93 | -55.93 | 80.11 | 0.8239 | -672.0 | -533.7 | |
| 65.39 | 624.15 | 59.00 | 574.38 | 15.51 | 87.47 | -57.38 | 76.17 | 0.8380 | 806.9 | -111.8 | |
| 0.00 | 1.25 | 0.00 | 1.17 | 16.69 | 85.96 | -58.89 | 74.82 | 0.8519 | 500.0 | 439.4 | |
| 0.98 | -3.00 | 0.90 | -3.00 | 14.66 | 86.77 | -58.08 | 77.19 | 0.8442 | -406.8 | 999999 | |
| 0.00 | 1.16 | 0.00 | 1.07 | 12.71 | 86.65 | -58.21 | 79.52 | 0.8453 | -742.0 | -617.5 | |
| 0.00 | 1.61 | 0.00 | 1.49 | 12.90 | 86.40 | -58.46 | 79.29 | 0.8475 | -613.0 | -517.2 | |
| 20.97 | -3.00 | 20.17 | -3.00 | 14.36 | 85.08 | -59.78 | 77.57 | 0.8593 | -849.5 | 999999 | |
| 1.96 | -3.00 | 1.88 | -3.00 | 13.83 | 85.30 | -59.55 | 78.19 | 0.8573 | -852.7 | 999999 | |
| 9.46 | -3.00 | 9.03 | -3.00 | 13.52 | 85.31 | -59.55 | 78.55 | 0.8573 | -743.6 | 999999 | |
| 1.43 | -3.00 | 1.37 | -3.00 | 13.22 | 85.12 | -59.74 | 78.90 | 0.8589 | -403.0 | 999999 | |
| 1.61 | -3.00 | 1.58 | -3.00 | 14.59 | 84.34 | -60.52 | 77.30 | 0.8656 | -372.6 | 999999 | |
| 0.00 | 1.16 | 0.00 | 1.13 | 11.95 | 84.74 | -60.12 | 80.37 | 0.8624 | -357.0 | -282.5 | |
| 0.00 | 0.98 | 0.00 | 0.99 | 13.89 | 83.56 | -61.30 | 78.11 | 0.8721 | -324.0 | -277.9 | |
| 0.00 | 1.52 | 0.00 | 1.52 | 13.35 | 83.73 | -61.12 | 78.73 | 0.8707 | -586.0 | -496.2 | |
| 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. | |