SDO HMI 2014-04-20 06:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.63 | 60.76 | 22.79 | 47.09 | -20.01 | 140.47 | -49.37 | 111.82 | 0.7694 | 311.0 | 110.2 | |
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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 |
| 2.75 | 6.83 | 1.94 | 4.83 | -18.51 | 145.31 | -44.53 | 110.98 | 0.7145 | 871.6 | 619.0 | |
| 4.08 | 6.30 | 2.91 | 4.49 | -18.69 | 144.75 | -45.08 | 111.09 | 0.7213 | 702.1 | 470.3 | |
| 3.02 | 4.79 | 2.19 | 3.47 | -18.03 | 143.66 | -46.18 | 109.92 | 0.7321 | 717.6 | 499.1 | |
| 0.00 | 1.24 | 0.00 | 0.91 | -17.54 | 142.86 | -46.98 | 109.09 | 0.7400 | -197.0 | -160.9 | |
| 4.44 | 7.36 | 3.40 | 5.64 | -20.15 | 141.05 | -48.79 | 112.12 | 0.7647 | 704.4 | 426.1 | |
| 1.86 | 3.28 | 1.45 | 2.55 | -20.84 | 140.45 | -49.39 | 112.87 | 0.7722 | 516.1 | 431.8 | |
| 1.06 | 3.11 | 0.84 | 2.44 | -20.48 | 139.81 | -50.02 | 112.27 | 0.7780 | 475.0 | 342.7 | |
| 4.35 | 9.76 | 3.56 | 8.01 | -21.91 | 137.94 | -51.90 | 113.65 | 0.7993 | -687.9 | -561.8 | |
| 2.66 | 4.52 | 2.13 | 3.62 | -19.55 | 138.76 | -51.08 | 110.88 | 0.7870 | 638.9 | 432.3 | |
| 2.48 | 4.08 | 1.98 | 3.26 | -19.27 | 138.73 | -51.11 | 110.52 | 0.7868 | 722.0 | 533.1 | |
| 2.93 | 5.23 | 2.39 | 4.27 | -20.09 | 137.84 | -52.00 | 111.38 | 0.7970 | 426.5 | 275.5 | |
| 0.00 | 2.84 | 0.00 | 2.40 | -22.06 | 136.51 | -53.33 | 113.55 | 0.8131 | -614.0 | -449.6 | |
| 0.00 | 1.15 | 0.00 | 0.97 | -21.75 | 136.57 | -53.27 | 113.18 | 0.8120 | -598.0 | -499.9 | |
| 0.00 | 0.27 | 0.00 | 0.23 | -21.41 | 136.32 | -53.52 | 112.72 | 0.8138 | -468.0 | -454.7 | |
| 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. | |