SDO HMI 2014-04-01 09:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.65 | 0.00 | 9.43 | -27.28 | 80.80 | 1.80 | 184.42 | 0.3750 | -423.5 | -390.0 | |
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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 | 0.79 | 0.00 | 0.43 | -21.71 | 99.71 | 20.71 | 230.70 | 0.4262 | 732.0 | 587.6 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -26.42 | 91.92 | 12.92 | 210.29 | 0.3988 | 796.0 | 592.2 | |
| 0.00 | 1.40 | 0.00 | 0.76 | -26.45 | 91.82 | 12.82 | 210.05 | 0.3985 | 929.0 | 665.1 | |
| 0.00 | 2.46 | 0.00 | 1.30 | -26.78 | 82.59 | 3.59 | 189.17 | 0.3524 | -744.0 | -656.3 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -26.21 | 81.57 | 2.57 | 186.81 | 0.3408 | -754.0 | -541.9 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -28.36 | 80.97 | 1.97 | 184.65 | 0.3748 | -834.0 | -649.8 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -33.79 | 76.86 | -2.14 | 176.13 | 0.4612 | -801.0 | -564.6 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -29.29 | 76.59 | -2.41 | 174.59 | 0.3904 | -732.0 | -594.5 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -28.87 | 76.43 | -2.57 | 174.10 | 0.3839 | -943.0 | -807.5 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -29.03 | 76.39 | -2.61 | 174.07 | 0.3866 | -869.0 | -725.9 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -27.03 | 76.01 | -3.00 | 172.43 | 0.3550 | -887.0 | -600.8 | |
| 0.00 | 3.51 | 0.00 | 1.84 | -25.28 | 75.72 | -3.28 | 170.86 | 0.3272 | -756.0 | -602.7 | |
| 0.00 | 0.44 | 0.00 | 0.24 | -29.78 | 64.87 | -14.13 | 151.96 | 0.4526 | -643.0 | -538.8 | |
| 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. | |