SDO HMI 2014-04-10 08:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.38 | 0.00 | 10.78 | -13.52 | 302.49 | -18.29 | 113.64 | 0.3469 | -233.6 | -250.3 | |
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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 | 1.06 | 0.00 | 0.54 | -18.49 | 313.44 | -7.35 | 150.87 | 0.2503 | -878.0 | -657.8 | |
| 0.00 | 1.41 | 0.00 | 0.73 | -18.05 | 309.61 | -11.17 | 138.92 | 0.2816 | 947.0 | 756.2 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 0.05 | 309.34 | -11.45 | 62.65 | 0.2245 | 734.0 | 580.9 | |
| 0.00 | 1.41 | 0.00 | 0.73 | -17.55 | 307.84 | -12.94 | 133.61 | 0.2962 | 833.0 | 615.1 | |
| 0.00 | 1.41 | 0.00 | 0.72 | -6.85 | 305.98 | -14.80 | 94.25 | 0.2555 | 971.0 | 833.2 | |
| 0.00 | 0.71 | 0.00 | 0.38 | -20.42 | 302.24 | -18.54 | 130.52 | 0.3937 | 815.0 | 695.2 | |
| 0.00 | 2.82 | 0.00 | 1.48 | -11.14 | 301.66 | -19.12 | 106.60 | 0.3369 | -855.0 | -729.8 | |
| 0.00 | 1.94 | 0.00 | 1.02 | -10.86 | 301.36 | -19.43 | 105.58 | 0.3406 | -620.0 | -507.5 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -16.53 | 300.42 | -20.36 | 119.62 | 0.3854 | -805.0 | -609.1 | |
| 0.00 | 1.59 | 0.00 | 0.85 | -15.65 | 300.42 | -20.37 | 117.50 | 0.3795 | -898.0 | -692.1 | |
| 0.00 | 1.24 | 0.00 | 0.65 | -9.91 | 300.22 | -20.57 | 102.29 | 0.3557 | -783.0 | -674.5 | |
| 0.00 | 0.53 | 0.00 | 0.29 | -14.36 | 297.88 | -22.91 | 112.21 | 0.4090 | -385.0 | -477.8 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -16.32 | 296.55 | -24.23 | 115.58 | 0.4386 | -838.0 | -713.7 | |
| 0.00 | 1.68 | 0.00 | 0.92 | -16.68 | 296.43 | -24.35 | 116.26 | 0.4423 | -825.0 | -681.4 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -14.35 | 296.18 | -24.60 | 111.02 | 0.4339 | -645.0 | -534.7 | |
| 0.00 | 0.44 | 0.00 | 0.25 | -16.96 | 295.63 | -25.15 | 116.20 | 0.4550 | -506.0 | -569.0 | |
| 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. | |