SDO HMI 2014-07-02 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 |
| 40.31 | 266.85 | 83.83 | 590.95 | -8.08 | 220.19 | -76.28 | 99.05 | 0.9737 | 247.6 | 47.9 | |
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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 |
| 1.36 | 229.07 | 2.72 | 461.50 | -9.00 | 221.59 | -74.88 | 100.11 | 0.9696 | 194.5 | 107.9 | |
| 35.68 | -1.00 | 70.80 | -1.00 | -8.38 | 221.59 | -74.88 | 99.47 | 0.9693 | 428.6 | 999999 | |
| 0.00 | 3.45 | 0.00 | 8.46 | -8.94 | 218.71 | -77.77 | 99.77 | 0.9805 | -588.0 | -469.0 | |
| 0.00 | 1.09 | 0.00 | 2.50 | -7.75 | 219.51 | -76.96 | 98.63 | 0.9773 | -382.0 | -376.8 | |
| 0.00 | 3.09 | 0.00 | 7.21 | -6.93 | 219.14 | -77.34 | 97.76 | 0.9784 | -171.0 | -178.0 | |
| 0.00 | 1.73 | 0.00 | 4.27 | -7.61 | 218.58 | -77.89 | 98.41 | 0.9806 | -316.0 | -348.9 | |
| 0.00 | 1.73 | 0.00 | 4.79 | -6.51 | 217.21 | -79.26 | 97.18 | 0.9847 | -418.0 | -379.1 | |
| 0.91 | 5.54 | 3.04 | 18.59 | -8.17 | 215.58 | -80.90 | 98.74 | 0.9895 | -330.0 | -296.9 | |
| 0.00 | 1.18 | 0.00 | 3.65 | -7.21 | 216.20 | -80.28 | 97.82 | 0.9877 | -422.0 | -381.8 | |
| 2.36 | 5.81 | 7.27 | 17.97 | -6.81 | 216.12 | -80.35 | 97.41 | 0.9879 | -571.0 | -499.4 | |
| 0.00 | 0.82 | 0.00 | 2.66 | -6.62 | 215.68 | -80.79 | 97.18 | 0.9890 | -390.0 | -385.3 | |
| 0.00 | 3.36 | 0.00 | 12.75 | -6.48 | 214.30 | -82.18 | 96.94 | 0.9922 | -74.0 | -75.7 | |
| 0.00 | 1.54 | 0.00 | 7.27 | -6.52 | 212.98 | -83.49 | 96.89 | 0.9948 | 89.0 | 99.1 | |
| 0.00 | 8.44 | 0.00 | 39.33 | -6.06 | 212.88 | -83.59 | 96.43 | 0.9949 | 189.0 | 115.6 | |
| 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. | |