SDO HMI 2014-09-05 01:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.29 | 199.57 | 52.71 | 233.69 | -19.46 | 107.24 | -60.17 | 115.48 | 0.9077 | 689.4 | 238.9 | |
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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 |
| 0.71 | 2.14 | 0.85 | 2.55 | -21.90 | 107.67 | -59.73 | 118.16 | 0.9107 | 365.8 | 383.3 | |
| 0.00 | 0.71 | 0.00 | 0.85 | -21.68 | 107.57 | -59.84 | 117.89 | 0.9108 | 257.0 | 291.8 | |
| 6.25 | 102.56 | 7.40 | 121.44 | -20.43 | 107.30 | -60.11 | 116.51 | 0.9096 | 630.6 | 178.9 | |
| 17.60 | -3.00 | 20.82 | -3.00 | -19.98 | 107.14 | -60.27 | 115.99 | 0.9097 | 737.9 | 999999 | |
| 16.71 | 69.60 | 18.94 | 78.61 | -18.60 | 107.92 | -59.49 | 114.79 | 0.9013 | 943.3 | 416.3 | |
| 4.02 | 14.47 | 4.70 | 17.01 | -19.09 | 107.11 | -60.30 | 115.04 | 0.9078 | 476.3 | 121.4 | |
| 0.00 | 0.89 | 0.00 | 1.07 | -19.30 | 106.38 | -61.03 | 115.04 | 0.9130 | 142.0 | 161.0 | |
| 0.00 | 4.29 | 0.00 | 5.53 | -19.23 | 104.43 | -62.98 | 114.36 | 0.9250 | -81.0 | -40.8 | |
| 0.00 | 1.88 | 0.00 | 2.51 | -18.66 | 103.38 | -64.02 | 113.47 | 0.9301 | 274.0 | 267.0 | |
| 0.00 | 0.89 | 0.00 | 1.20 | -17.81 | 103.09 | -64.32 | 112.51 | 0.9304 | -331.0 | -324.2 | |
| 0.00 | 2.14 | 0.00 | 2.92 | -17.32 | 102.52 | -64.89 | 111.85 | 0.9328 | -230.0 | -312.4 | |
| 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. | |