SDO HMI 2014-03-29 04:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.16 | 0.00 | 11.06 | -26.54 | 86.14 | -35.17 | 126.09 | 0.6231 | -138.3 | 0.9 | |
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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 | 3.33 | 0.00 | 1.82 | -22.96 | 101.59 | -19.72 | 132.65 | 0.4242 | 926.0 | 713.0 | |
| 0.00 | 1.75 | 0.00 | 0.96 | -21.92 | 99.78 | -21.53 | 128.41 | 0.4364 | 672.0 | 508.6 | |
| 0.00 | 1.66 | 0.00 | 1.01 | -26.83 | 90.52 | -30.79 | 128.15 | 0.5830 | 799.0 | 679.9 | |
| 0.00 | 1.31 | 0.00 | 0.81 | -26.49 | 89.02 | -32.29 | 126.56 | 0.5976 | 338.0 | 348.5 | |
| 0.00 | 1.23 | 0.00 | 0.82 | -27.75 | 82.54 | -38.77 | 124.57 | 0.6753 | -753.0 | -568.4 | |
| 0.00 | 1.58 | 0.00 | 1.07 | -28.28 | 81.78 | -39.53 | 124.92 | 0.6859 | -505.0 | -396.4 | |
| 0.00 | 1.14 | 0.00 | 0.77 | -27.31 | 81.94 | -39.37 | 123.68 | 0.6796 | -485.0 | -456.5 | |
| 0.00 | 0.61 | 0.00 | 0.43 | -29.90 | 79.56 | -41.76 | 126.00 | 0.7160 | -440.0 | -320.6 | |
| 0.00 | 1.75 | 0.00 | 1.25 | -29.60 | 78.77 | -42.54 | 125.28 | 0.7224 | -587.0 | -396.4 | |
| 0.00 | 0.79 | 0.00 | 0.58 | -26.87 | 75.69 | -45.62 | 120.54 | 0.7425 | -585.0 | -562.8 | |
| 0.00 | 0.61 | 0.00 | 0.45 | -26.82 | 75.39 | -45.93 | 120.36 | 0.7454 | -423.0 | -429.1 | |
| 0.00 | 0.61 | 0.00 | 0.46 | -27.08 | 74.66 | -46.65 | 120.46 | 0.7535 | -410.0 | -343.4 | |
| 0.00 | 0.79 | 0.00 | 0.63 | -28.70 | 72.02 | -49.29 | 121.67 | 0.7835 | -345.0 | -308.6 | |
| 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. | |