SDO HMI 2014-08-02 09:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.13 | 105.66 | 29.33 | 282.01 | 8.91 | 172.37 | -80.01 | 82.00 | 0.9827 | 23.9 | 62.0 | |
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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 | 0.54 | 0.00 | 0.82 | 7.97 | 181.01 | -71.37 | 83.58 | 0.9458 | -461.0 | -454.8 | |
| 0.00 | 1.18 | 0.00 | 2.07 | 10.77 | 178.01 | -74.37 | 80.47 | 0.9605 | -343.0 | -331.3 | |
| 4.80 | 15.03 | 8.35 | 26.16 | 10.22 | 178.14 | -74.24 | 81.05 | 0.9601 | -537.2 | -361.8 | |
| 0.00 | 0.63 | 0.00 | 1.33 | 10.43 | 175.17 | -77.20 | 80.66 | 0.9730 | 369.0 | 329.4 | |
| 0.00 | 1.00 | 0.00 | 2.09 | 10.06 | 175.19 | -77.19 | 81.04 | 0.9730 | 407.0 | 354.6 | |
| 0.00 | 1.36 | 0.00 | 3.21 | 10.99 | 173.60 | -78.77 | 79.98 | 0.9787 | 409.0 | 421.7 | |
| 0.00 | 0.72 | 0.00 | 2.00 | 11.37 | 171.76 | -80.62 | 79.47 | 0.9846 | 289.0 | 287.9 | |
| 0.00 | 0.27 | 0.00 | 0.75 | 9.03 | 172.00 | -80.38 | 81.86 | 0.9844 | 464.0 | 457.3 | |
| 2.35 | 84.93 | 6.37 | 243.58 | 8.64 | 172.17 | -80.21 | 82.27 | 0.9840 | 392.1 | 88.6 | |
| 2.44 | -9.00 | 7.07 | -9.00 | 9.19 | 171.45 | -80.93 | 81.66 | 0.9860 | 267.9 | 999999 | |
| 2.54 | -9.00 | 7.54 | -9.00 | 8.28 | 171.33 | -81.04 | 82.57 | 0.9865 | -23.0 | 999999 | |
| 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. | |