SDO HMI 2014-09-06 04:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.33 | 36.17 | 3.91 | 19.44 | -15.05 | 147.97 | -4.58 | 168.52 | 0.3886 | -207.9 | -51.3 | |
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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 | 2.05 | 0.00 | 1.11 | -15.97 | 148.80 | -3.75 | 170.93 | 0.4008 | -950.0 | -793.0 | |
| 4.47 | 15.99 | 2.38 | 8.52 | -13.85 | 148.50 | -4.06 | 169.19 | 0.3679 | 1017.9 | 774.7 | |
| 0.00 | 1.88 | 0.00 | 1.02 | -16.31 | 148.45 | -4.11 | 170.23 | 0.4070 | -891.0 | -735.7 | |
| 0.00 | 0.98 | 0.00 | 0.53 | -15.95 | 148.08 | -4.48 | 169.20 | 0.4024 | -906.0 | -740.1 | |
| 1.97 | -2.00 | 1.05 | -2.00 | -14.18 | 148.08 | -4.47 | 168.31 | 0.3744 | 875.1 | 999999 | |
| 0.00 | 1.16 | 0.00 | 0.63 | -16.31 | 147.91 | -4.64 | 168.99 | 0.4086 | -801.0 | -610.4 | |
| 0.00 | 2.50 | 0.00 | 1.35 | -15.36 | 147.90 | -4.65 | 168.49 | 0.3936 | -185.0 | -121.8 | |
| 0.89 | 3.66 | 0.48 | 1.99 | -16.25 | 147.63 | -4.93 | 168.30 | 0.4085 | -1020.9 | -777.6 | |
| 0.00 | 1.25 | 0.00 | 0.67 | -14.45 | 147.64 | -4.91 | 167.34 | 0.3801 | 345.0 | 197.0 | |
| 0.00 | 1.52 | 0.00 | 0.81 | -14.71 | 147.57 | -4.98 | 167.32 | 0.3845 | 806.0 | 583.1 | |
| 0.00 | 1.25 | 0.00 | 0.68 | -16.28 | 147.47 | -5.09 | 167.96 | 0.4095 | -788.0 | -596.9 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -16.12 | 147.16 | -5.40 | 167.15 | 0.4081 | -800.0 | -617.4 | |
| 0.00 | 3.04 | 0.00 | 1.65 | -16.46 | 146.29 | -6.26 | 165.39 | 0.4166 | -760.0 | -548.6 | |
| 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. | |