SDO HMI 2014-03-24 13:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.00 | 36.68 | 7.72 | 26.23 | 3.22 | 137.27 | -45.05 | 78.75 | 0.7227 | -43.7 | 67.2 | |
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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 |
| 2.97 | 9.08 | 2.06 | 6.30 | 3.43 | 139.06 | -43.27 | 77.91 | 0.7020 | -737.7 | -507.1 | |
| 1.66 | -1.00 | 1.15 | -1.00 | 3.13 | 139.03 | -43.29 | 78.34 | 0.7014 | -692.2 | 999999 | |
| 0.52 | 2.45 | 0.36 | 1.70 | 2.78 | 138.84 | -43.48 | 78.89 | 0.7028 | -483.2 | -375.6 | |
| 3.76 | 5.33 | 2.64 | 3.75 | 3.92 | 138.32 | -44.00 | 77.48 | 0.7123 | -667.5 | -551.3 | |
| 0.00 | 0.26 | 0.00 | 0.18 | 2.70 | 137.97 | -44.35 | 79.26 | 0.7131 | 470.0 | 472.7 | |
| 0.00 | 0.70 | 0.00 | 0.50 | 3.69 | 137.75 | -44.58 | 77.98 | 0.7184 | 641.0 | 501.4 | |
| 0.00 | 2.27 | 0.00 | 1.64 | 3.83 | 136.89 | -45.44 | 78.07 | 0.7289 | -644.0 | -471.3 | |
| 0.61 | 1.48 | 0.44 | 1.07 | 2.79 | 136.65 | -45.68 | 79.54 | 0.7290 | 484.3 | 444.5 | |
| 0.00 | 0.87 | 0.00 | 0.64 | 5.46 | 136.37 | -45.96 | 76.08 | 0.7396 | -405.0 | -370.3 | |
| 1.48 | 4.54 | 1.07 | 3.28 | 2.29 | 136.46 | -45.87 | 80.26 | 0.7300 | 749.6 | 582.0 | |
| 0.00 | 0.96 | 0.00 | 0.70 | 2.73 | 136.22 | -46.10 | 79.73 | 0.7338 | 217.0 | 146.3 | |
| 0.00 | 1.75 | 0.00 | 1.31 | 5.61 | 135.34 | -46.98 | 76.22 | 0.7515 | 211.0 | 152.4 | |
| 0.00 | 1.14 | 0.00 | 0.83 | 2.22 | 135.50 | -46.82 | 80.61 | 0.7409 | 703.0 | 534.8 | |
| 0.00 | 2.18 | 0.00 | 1.61 | 2.44 | 135.40 | -46.92 | 80.35 | 0.7426 | 676.0 | 621.2 | |
| 0.00 | 3.67 | 0.00 | 2.72 | 2.38 | 135.10 | -47.23 | 80.51 | 0.7459 | 548.0 | 470.6 | |
| 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. | |