SDO HMI 2014-01-11 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 | 20.87 | 0.00 | 11.32 | -20.90 | 62.19 | 12.61 | 214.29 | 0.3932 | -309.5 | -233.1 | |
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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 | 0.68 | 0.00 | 0.41 | -18.79 | 81.68 | 32.10 | 242.42 | 0.5699 | 736.0 | 637.1 | |
| 0.00 | 1.44 | 0.00 | 0.81 | -19.49 | 74.34 | 24.77 | 235.61 | 0.4806 | 644.0 | 580.6 | |
| 0.00 | 1.19 | 0.00 | 0.65 | -14.74 | 72.82 | 23.24 | 243.65 | 0.4277 | -876.0 | -682.6 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -21.58 | 73.17 | 23.60 | 230.69 | 0.4831 | 751.0 | 596.2 | |
| 0.00 | 1.44 | 0.00 | 0.82 | -21.65 | 72.94 | 23.37 | 230.32 | 0.4810 | 768.0 | 653.2 | |
| 0.00 | 1.44 | 0.00 | 0.81 | -21.36 | 72.17 | 22.60 | 229.97 | 0.4693 | 783.0 | 629.4 | |
| 0.00 | 1.27 | 0.00 | 0.67 | -16.27 | 64.73 | 15.15 | 229.81 | 0.3299 | -815.0 | -638.5 | |
| 0.00 | 1.44 | 0.00 | 0.74 | -16.29 | 59.66 | 10.08 | 218.56 | 0.2708 | -992.0 | -745.8 | |
| 0.00 | 3.14 | 0.00 | 1.62 | -16.08 | 59.59 | 10.01 | 218.87 | 0.2673 | -713.0 | -566.8 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -15.39 | 58.96 | 9.39 | 218.83 | 0.2519 | -830.0 | -668.3 | |
| 0.00 | 1.61 | 0.00 | 0.83 | -17.53 | 58.72 | 9.15 | 213.17 | 0.2783 | -750.0 | -648.9 | |
| 0.00 | 1.70 | 0.00 | 0.94 | -30.59 | 52.15 | 2.57 | 184.97 | 0.4484 | -846.0 | -566.2 | |
| 0.00 | 0.93 | 0.00 | 0.51 | -29.31 | 50.06 | 0.48 | 180.99 | 0.4266 | -736.0 | -569.4 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -29.47 | 42.52 | -7.05 | 165.96 | 0.4427 | -875.0 | -671.1 | |
| 0.00 | 1.02 | 0.00 | 0.56 | -28.36 | 42.43 | -7.15 | 165.06 | 0.4263 | -892.0 | -669.6 | |
| 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. | |