SDO HMI 2014-07-06 08:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.90 | 138.20 | 23.57 | 99.95 | 6.47 | 203.37 | -46.79 | 84.33 | 0.7298 | -645.0 | -246.3 | |
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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 |
| 3.27 | 13.27 | 2.31 | 9.37 | 6.75 | 204.67 | -45.49 | 83.91 | 0.7145 | -986.4 | -632.2 | |
| 4.00 | -1.00 | 2.83 | -1.00 | 6.93 | 204.52 | -45.64 | 83.67 | 0.7164 | -750.6 | 999999 | |
| 0.00 | 1.64 | 0.00 | 1.17 | 8.93 | 204.10 | -46.06 | 80.90 | 0.7227 | -603.0 | -471.3 | |
| 22.08 | 104.67 | 15.85 | 75.23 | 6.31 | 203.70 | -46.46 | 84.55 | 0.7260 | -1040.4 | -268.4 | |
| 0.00 | 1.18 | 0.00 | 0.86 | 8.37 | 203.02 | -47.14 | 81.77 | 0.7351 | -587.0 | -493.7 | |
| 2.73 | 9.27 | 1.98 | 6.75 | 7.17 | 203.05 | -47.10 | 83.40 | 0.7340 | -705.3 | -373.5 | |
| 0.82 | -6.00 | 0.60 | -6.00 | 7.04 | 202.89 | -47.27 | 83.58 | 0.7359 | -489.6 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.90 | 3.79 | 200.68 | -49.48 | 87.95 | 0.7612 | -519.0 | -411.1 | |
| 0.00 | 0.91 | 0.00 | 0.71 | 5.94 | 199.46 | -50.70 | 85.13 | 0.7747 | 648.0 | 569.8 | |
| 0.00 | 1.36 | 0.00 | 1.07 | 6.09 | 199.29 | -50.86 | 84.94 | 0.7765 | 630.0 | 548.0 | |
| 0.00 | 1.54 | 0.00 | 1.26 | 6.73 | 197.41 | -52.75 | 84.15 | 0.7969 | 525.0 | 466.8 | |
| 0.00 | 0.82 | 0.00 | 0.67 | 7.76 | 197.08 | -53.08 | 82.86 | 0.8005 | 527.0 | 444.3 | |
| 0.00 | 0.91 | 0.00 | 0.75 | 8.15 | 196.75 | -53.41 | 82.40 | 0.8040 | 540.0 | 486.4 | |
| 0.00 | 1.45 | 0.00 | 1.21 | 7.01 | 196.69 | -53.46 | 83.82 | 0.8043 | 414.0 | 387.0 | |
| 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. | |