SDO HMI 2014-10-03 08:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.58 | 0.00 | 9.78 | -5.41 | 138.20 | -15.74 | 127.17 | 0.3402 | -838.8 | -654.2 | |
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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 | 1.41 | 0.00 | 0.73 | -4.72 | 140.41 | -13.54 | 129.64 | 0.3043 | -991.0 | -711.8 | |
| 0.00 | 1.76 | 0.00 | 0.92 | -5.69 | 139.76 | -14.18 | 130.67 | 0.3229 | -1119.0 | -883.1 | |
| 0.00 | 2.99 | 0.00 | 1.56 | -4.28 | 139.64 | -14.30 | 126.96 | 0.3097 | -814.0 | -667.2 | |
| 0.00 | 1.94 | 0.00 | 1.02 | -6.37 | 138.59 | -15.36 | 129.95 | 0.3448 | -753.0 | -614.8 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -6.06 | 138.60 | -15.35 | 129.27 | 0.3415 | -879.0 | -755.5 | |
| 0.00 | 2.02 | 0.00 | 1.07 | -6.34 | 138.43 | -15.51 | 129.60 | 0.3465 | -729.0 | -582.0 | |
| 0.00 | 1.94 | 0.00 | 1.02 | -6.01 | 138.32 | -15.63 | 128.64 | 0.3445 | -767.0 | -488.2 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -5.49 | 136.32 | -17.63 | 124.11 | 0.3656 | -904.0 | -737.6 | |
| 0.00 | 1.94 | 0.00 | 1.03 | -5.28 | 136.23 | -17.71 | 123.50 | 0.3649 | -731.0 | -573.6 | |
| 0.00 | 1.94 | 0.00 | 1.03 | -4.89 | 135.93 | -18.02 | 122.15 | 0.3656 | -835.0 | -685.2 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -4.71 | 135.90 | -18.05 | 121.68 | 0.3644 | -705.0 | -593.1 | |
| 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. | |