SDO HMI 2014-09-06 16:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.50 | 89.59 | 22.22 | 47.96 | -14.88 | 148.93 | 2.97 | 187.64 | 0.3813 | -78.0 | -42.4 | |
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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 | 1.07 | 0.00 | 0.58 | -16.62 | 149.77 | 3.81 | 188.95 | 0.4108 | -744.0 | -610.0 | |
| 0.00 | 0.98 | 0.00 | 0.53 | -16.18 | 149.39 | 3.42 | 188.21 | 0.4031 | -863.0 | -628.8 | |
| 17.94 | 47.03 | 9.50 | 24.92 | -13.31 | 149.22 | 3.26 | 188.95 | 0.3567 | 1124.1 | 616.5 | |
| 8.92 | 34.18 | 4.84 | 18.54 | -16.68 | 149.17 | 3.21 | 187.54 | 0.4104 | -962.7 | -822.4 | |
| 2.50 | -3.00 | 1.33 | -3.00 | -13.73 | 149.01 | 3.04 | 188.20 | 0.3629 | 880.5 | 999999 | |
| 2.23 | -3.00 | 1.18 | -3.00 | -13.67 | 148.76 | 2.79 | 187.56 | 0.3613 | 927.2 | 999999 | |
| 9.55 | -4.00 | 5.18 | -4.00 | -16.61 | 148.70 | 2.73 | 186.45 | 0.4084 | -1097.5 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -16.64 | 148.19 | 2.23 | 185.26 | 0.4081 | -822.0 | -614.8 | |
| 0.00 | 1.25 | 0.00 | 0.67 | -16.04 | 147.81 | 1.85 | 184.48 | 0.3980 | -734.0 | -601.7 | |
| 0.00 | 0.98 | 0.00 | 0.52 | -14.40 | 147.42 | 1.46 | 183.83 | 0.3711 | 739.0 | 602.7 | |
| 0.00 | 0.80 | 0.00 | 0.43 | -15.87 | 147.34 | 1.37 | 183.36 | 0.3948 | -812.0 | -640.4 | |
| 0.36 | 1.07 | 0.19 | 0.57 | -15.38 | 147.18 | 1.21 | 183.04 | 0.3867 | -848.8 | -785.9 | |
| 0.00 | 1.34 | 0.00 | 0.72 | -15.67 | 145.49 | -0.48 | 178.82 | 0.3910 | -709.0 | -543.3 | |
| 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. | |