SDO HMI 2014-01-08 15:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.45 | 0.00 | 11.92 | -20.85 | 63.42 | -25.66 | 128.79 | 0.5021 | -147.2 | -54.0 | |
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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 | 1.61 | 0.00 | 0.85 | -18.41 | 75.97 | -13.11 | 139.61 | 0.3336 | 720.0 | 406.5 | |
| 0.00 | 1.27 | 0.00 | 0.68 | -20.48 | 73.29 | -15.79 | 138.53 | 0.3866 | 738.0 | 545.2 | |
| 0.00 | 1.27 | 0.00 | 0.67 | -17.88 | 73.49 | -15.60 | 133.72 | 0.3556 | 695.0 | 516.3 | |
| 0.00 | 0.34 | 0.00 | 0.18 | -21.63 | 72.11 | -16.98 | 138.61 | 0.4123 | 386.0 | 376.5 | |
| 0.00 | 5.44 | 0.00 | 2.95 | -21.38 | 72.04 | -17.04 | 138.07 | 0.4102 | 351.0 | 526.9 | |
| 0.00 | 1.78 | 0.00 | 0.96 | -15.01 | 69.27 | -19.81 | 121.08 | 0.3839 | -765.0 | -550.7 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -14.77 | 69.14 | -19.95 | 120.36 | 0.3840 | -911.0 | -728.4 | |
| 0.00 | 1.36 | 0.00 | 0.87 | -23.05 | 53.40 | -35.68 | 122.38 | 0.6378 | -533.0 | -486.9 | |
| 0.00 | 1.10 | 0.00 | 0.72 | -24.32 | 52.91 | -36.17 | 123.90 | 0.6503 | -659.0 | -523.4 | |
| 0.00 | 1.87 | 0.00 | 1.21 | -23.52 | 52.65 | -36.43 | 122.63 | 0.6488 | -498.0 | -475.3 | |
| 0.00 | 1.02 | 0.00 | 0.66 | -23.51 | 52.38 | -36.71 | 122.45 | 0.6519 | -632.0 | -522.6 | |
| 0.00 | 0.59 | 0.00 | 0.41 | -22.31 | 48.34 | -40.74 | 118.77 | 0.6912 | -502.0 | -509.7 | |
| 0.00 | 1.44 | 0.00 | 1.03 | -23.42 | 45.80 | -43.28 | 119.20 | 0.7231 | -304.0 | -334.8 | |
| 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. | |