SDO HMI 2014-07-07 23:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.82 | 15.63 | 1.10 | 9.51 | -21.78 | 203.43 | -25.21 | 137.13 | 0.5824 | -57.8 | 177.3 | |
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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 | 0.64 | 0.00 | 0.38 | -23.83 | 206.82 | -21.82 | 143.33 | 0.5713 | -666.0 | -630.4 | |
| 0.00 | 5.08 | 0.00 | 3.03 | -21.32 | 205.29 | -23.35 | 138.45 | 0.5587 | 848.0 | 706.9 | |
| 1.82 | 4.00 | 1.10 | 2.43 | -23.00 | 204.66 | -23.97 | 139.81 | 0.5817 | -904.7 | -712.5 | |
| 0.00 | 0.82 | 0.00 | 0.49 | -21.41 | 204.41 | -24.22 | 137.56 | 0.5681 | 515.0 | 492.3 | |
| 0.00 | 1.18 | 0.00 | 0.72 | -21.83 | 203.83 | -24.80 | 137.44 | 0.5778 | 758.0 | 631.4 | |
| 0.00 | 1.18 | 0.00 | 0.71 | -21.60 | 203.80 | -24.83 | 137.11 | 0.5758 | 748.0 | 586.8 | |
| 0.00 | 0.64 | 0.00 | 0.39 | -22.30 | 202.83 | -25.80 | 136.94 | 0.5920 | 588.0 | 472.0 | |
| 0.00 | 0.82 | 0.00 | 0.52 | -18.35 | 196.12 | -32.51 | 125.53 | 0.6292 | -729.0 | -629.2 | |
| 0.00 | 0.73 | 0.00 | 0.48 | -21.33 | 195.30 | -33.33 | 128.81 | 0.6592 | -641.0 | -522.0 | |
| 0.00 | 0.27 | 0.00 | 0.18 | -20.86 | 195.34 | -33.29 | 128.24 | 0.6554 | -495.0 | -473.7 | |
| 0.00 | 0.27 | 0.00 | 0.18 | -21.18 | 194.74 | -33.89 | 128.20 | 0.6638 | -572.0 | -573.0 | |
| 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. | |