SDO HMI 2014-09-08 13:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.20 | 155.79 | 31.53 | 158.32 | -16.43 | 64.57 | -56.63 | 113.46 | 0.8742 | 206.8 | 34.9 | |
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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 |
| 20.96 | 107.82 | 20.22 | 104.00 | -16.37 | 66.43 | -54.77 | 114.02 | 0.8601 | 667.1 | 182.9 | |
| 1.87 | -1.00 | 1.83 | -1.00 | -16.77 | 66.04 | -55.16 | 114.32 | 0.8644 | -366.8 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.95 | -15.00 | 65.67 | -55.54 | 112.23 | 0.8624 | -252.0 | -276.4 | |
| 0.00 | 0.98 | 0.00 | 1.00 | -16.66 | 64.68 | -56.53 | 113.71 | 0.8748 | 356.0 | 315.1 | |
| 0.62 | 3.21 | 0.63 | 3.24 | -16.20 | 64.71 | -56.49 | 113.22 | 0.8733 | 165.1 | 261.4 | |
| 0.62 | 1.69 | 0.64 | 1.75 | -16.59 | 64.07 | -57.14 | 113.43 | 0.8793 | -28.3 | 37.2 | |
| 0.00 | 0.80 | 0.00 | 0.90 | -16.48 | 61.33 | -59.88 | 112.41 | 0.8990 | -653.0 | -593.6 | |
| 3.12 | 38.97 | 3.58 | 44.89 | -16.55 | 60.65 | -60.56 | 112.28 | 0.9039 | -532.7 | -280.5 | |
| 2.41 | -8.00 | 2.75 | -8.00 | -16.26 | 60.68 | -60.53 | 111.97 | 0.9031 | -703.0 | 999999 | |
| 0.00 | 0.98 | 0.00 | 1.16 | -17.33 | 60.09 | -61.12 | 112.93 | 0.9093 | -345.0 | -378.2 | |
| 0.80 | -8.00 | 0.94 | -8.00 | -16.77 | 60.21 | -61.00 | 112.37 | 0.9073 | -212.7 | 999999 | |
| 0.80 | -8.00 | 0.94 | -8.00 | -16.55 | 60.13 | -61.07 | 112.12 | 0.9074 | -261.7 | 999999 | |
| 0.00 | 0.36 | 0.00 | 0.43 | -17.66 | 59.49 | -61.71 | 113.10 | 0.9139 | -167.0 | -175.2 | |
| 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. | |