SDO HMI 2014-09-06 15:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.19 | 38.27 | 20.77 | 59.75 | -20.37 | 79.36 | -67.16 | 114.36 | 0.9496 | -165.0 | -168.4 | |
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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 |
| 0.62 | 1.61 | 0.86 | 2.21 | -20.64 | 82.28 | -64.23 | 115.44 | 0.9348 | 329.9 | 273.6 | |
| 0.62 | 1.87 | 0.88 | 2.64 | -20.44 | 81.68 | -64.84 | 115.07 | 0.9378 | 258.1 | 239.6 | |
| 1.25 | 3.21 | 1.92 | 4.94 | -21.70 | 80.12 | -66.39 | 115.91 | 0.9480 | 452.1 | 377.3 | |
| 0.89 | 2.41 | 1.29 | 3.47 | -20.41 | 81.17 | -65.34 | 114.89 | 0.9405 | 174.2 | 107.9 | |
| 3.12 | 4.46 | 4.83 | 6.90 | -21.33 | 79.89 | -66.63 | 115.47 | 0.9485 | 16.0 | -83.4 | |
| 0.00 | 2.05 | 0.00 | 3.02 | -20.27 | 80.65 | -65.86 | 114.60 | 0.9430 | -232.0 | -253.2 | |
| 0.00 | 1.96 | 0.00 | 2.93 | -19.21 | 80.08 | -66.44 | 113.37 | 0.9443 | -161.0 | -228.6 | |
| 0.00 | 2.32 | 0.00 | 3.66 | -20.12 | 79.14 | -67.37 | 114.04 | 0.9504 | -417.0 | -448.6 | |
| 0.00 | 0.71 | 0.00 | 1.10 | -19.78 | 79.44 | -67.08 | 113.78 | 0.9485 | -567.0 | -532.9 | |
| 0.00 | 0.36 | 0.00 | 0.56 | -19.92 | 79.15 | -67.36 | 113.84 | 0.9501 | -490.0 | -499.5 | |
| 6.69 | 17.31 | 10.99 | 28.32 | -20.06 | 78.25 | -68.27 | 113.76 | 0.9547 | -370.0 | -266.8 | |
| 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. | |