SDO HMI 2014-04-05 01:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.36 | 176.81 | 21.88 | 95.74 | 17.39 | 30.00 | -0.62 | 1.46 | 0.4053 | -310.0 | -363.8 | |
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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 |
| 1.14 | 145.17 | 0.62 | 78.60 | 17.10 | 31.04 | 0.43 | 358.97 | 0.3995 | -1051.1 | -445.3 | |
| 14.68 | -1.00 | 7.96 | -1.00 | 17.56 | 30.92 | 0.30 | 359.28 | 0.4068 | -1076.3 | 999999 | |
| 10.82 | -1.00 | 5.85 | -1.00 | 17.36 | 30.63 | 0.02 | 359.95 | 0.4036 | -1101.7 | 999999 | |
| 0.00 | 1.49 | 0.00 | 0.81 | 17.69 | 29.69 | -0.92 | 2.16 | 0.4092 | -620.0 | -447.6 | |
| 0.00 | 1.49 | 0.00 | 0.80 | 16.06 | 29.29 | -1.32 | 3.33 | 0.3833 | -729.0 | -658.6 | |
| 0.00 | 2.99 | 0.00 | 1.60 | 15.58 | 29.14 | -1.48 | 3.80 | 0.3756 | -844.0 | -586.7 | |
| 0.00 | 0.70 | 0.00 | 0.38 | 16.37 | 27.22 | -3.39 | 8.37 | 0.3915 | 709.0 | 536.6 | |
| 6.68 | 20.31 | 3.63 | 11.03 | 17.33 | 25.73 | -4.89 | 11.46 | 0.4108 | 1004.6 | 672.5 | |
| 1.06 | -8.00 | 0.57 | -8.00 | 17.59 | 25.66 | -4.96 | 11.49 | 0.4152 | 696.0 | 999999 | |
| 5.98 | -8.00 | 3.25 | -8.00 | 17.33 | 25.51 | -5.11 | 11.96 | 0.4116 | 1053.7 | 999999 | |
| 0.00 | 2.11 | 0.00 | 1.14 | 16.81 | 25.43 | -5.19 | 12.43 | 0.4037 | 709.0 | 558.4 | |
| 0.00 | 1.76 | 0.00 | 0.96 | 18.35 | 25.16 | -5.45 | 12.20 | 0.4286 | 642.0 | 489.2 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 13.96 | 23.75 | -6.86 | 18.52 | 0.3665 | -625.0 | -455.1 | |
| 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. | |