SDO HMI 2014-10-04 07:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.11 | 33.51 | 1.09 | 17.59 | -12.53 | 139.47 | -1.83 | 174.75 | 0.3305 | -54.5 | 189.4 | |
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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 |
| 0.00 | 2.02 | 0.00 | 1.05 | -11.42 | 142.34 | 1.04 | 183.31 | 0.3106 | 926.0 | 711.2 | |
| 0.00 | 0.62 | 0.00 | 0.33 | -16.03 | 140.42 | -0.88 | 177.81 | 0.3860 | 745.0 | 610.6 | |
| 2.11 | 13.81 | 1.09 | 7.14 | -10.00 | 140.39 | -0.91 | 176.86 | 0.2868 | 1155.2 | 845.5 | |
| 0.00 | 2.29 | 0.00 | 1.23 | -16.19 | 140.20 | -1.10 | 177.28 | 0.3888 | 816.0 | 689.9 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -15.99 | 140.17 | -1.13 | 177.18 | 0.3857 | 766.0 | 701.2 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -15.22 | 139.06 | -2.24 | 174.19 | 0.3745 | -888.0 | -793.6 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -14.74 | 138.91 | -2.39 | 173.66 | 0.3669 | -933.0 | -756.6 | |
| 0.00 | 1.14 | 0.00 | 0.59 | -8.42 | 138.58 | -2.72 | 169.69 | 0.2638 | 789.0 | 580.6 | |
| 0.00 | 2.11 | 0.00 | 1.13 | -15.51 | 138.40 | -2.90 | 172.61 | 0.3804 | -828.0 | -658.2 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -15.29 | 138.34 | -2.96 | 172.38 | 0.3769 | -818.0 | -653.2 | |
| 0.00 | 3.52 | 0.00 | 1.87 | -14.65 | 137.70 | -3.60 | 170.46 | 0.3682 | -896.0 | -692.8 | |
| 0.00 | 1.94 | 0.00 | 1.03 | -14.94 | 137.69 | -3.60 | 170.58 | 0.3728 | -763.0 | -544.1 | |
| 0.00 | 1.58 | 0.00 | 0.83 | -12.01 | 135.68 | -5.62 | 163.24 | 0.3336 | -888.0 | -774.0 | |
| 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. | |