SDO HMI 2014-10-03 04:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.87 | 69.37 | 7.99 | 37.50 | -10.35 | 139.86 | -16.28 | 136.15 | 0.4001 | 333.3 | 373.6 | |
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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 | 0.76 | -11.60 | 141.15 | -14.99 | 140.64 | 0.4013 | 818.0 | 659.1 | |
| 6.07 | 52.11 | 3.26 | 27.98 | -9.90 | 140.35 | -15.79 | 136.27 | 0.3894 | 1122.3 | 598.0 | |
| 5.81 | -2.00 | 3.11 | -2.00 | -9.24 | 140.35 | -15.79 | 135.07 | 0.3818 | 1070.8 | 999999 | |
| 2.64 | -2.00 | 1.42 | -2.00 | -9.62 | 140.30 | -15.84 | 135.67 | 0.3867 | 1145.1 | 999999 | |
| 0.00 | 2.73 | 0.00 | 1.49 | -12.01 | 140.13 | -16.00 | 139.46 | 0.4166 | 868.0 | 697.8 | |
| 0.00 | 1.41 | 0.00 | 0.77 | -11.96 | 139.82 | -16.32 | 138.82 | 0.4192 | 897.0 | 740.1 | |
| 0.00 | 0.97 | 0.00 | 0.54 | -15.42 | 138.72 | -17.42 | 142.07 | 0.4714 | -973.0 | -790.5 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -8.57 | 138.83 | -17.31 | 131.15 | 0.3923 | 654.0 | 594.5 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -14.32 | 137.93 | -18.20 | 139.30 | 0.4661 | -823.0 | -642.9 | |
| 0.35 | 1.41 | 0.20 | 0.79 | -14.03 | 137.92 | -18.21 | 138.87 | 0.4629 | -926.0 | -795.3 | |
| 0.00 | 3.70 | 0.00 | 2.05 | -12.91 | 138.01 | -18.12 | 137.32 | 0.4491 | -883.0 | -791.3 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -14.58 | 137.65 | -18.49 | 139.24 | 0.4720 | -767.0 | -632.8 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -14.59 | 137.42 | -18.72 | 138.91 | 0.4744 | -756.0 | -676.7 | |
| 0.00 | 0.70 | 0.00 | 0.39 | -12.66 | 136.96 | -19.17 | 135.32 | 0.4577 | -717.0 | -574.4 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -8.24 | 132.50 | -23.64 | 121.90 | 0.4694 | 840.0 | 698.2 | |
| 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. | |