SDO HMI 2014-03-24 19:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.75 | 45.84 | 9.93 | 30.95 | 2.99 | 137.29 | -41.73 | 77.97 | 0.6818 | 55.5 | 58.6 | |
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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 |
| 1.48 | 3.58 | 0.97 | 2.34 | 3.12 | 139.39 | -39.63 | 77.06 | 0.6558 | -778.7 | -602.2 | |
| 2.88 | 5.41 | 1.89 | 3.55 | 3.49 | 139.34 | -39.68 | 76.53 | 0.6577 | -863.8 | -654.3 | |
| 1.05 | 3.14 | 0.69 | 2.06 | 2.95 | 139.24 | -39.78 | 77.36 | 0.6571 | -558.1 | -359.0 | |
| 0.00 | 2.10 | 0.00 | 1.38 | 3.42 | 139.07 | -39.95 | 76.74 | 0.6609 | -434.0 | -362.3 | |
| 3.75 | 7.95 | 2.49 | 5.27 | 3.88 | 138.65 | -40.37 | 76.23 | 0.6677 | -691.3 | -484.4 | |
| 0.00 | 1.05 | 0.00 | 0.70 | 2.52 | 137.80 | -41.22 | 78.50 | 0.6741 | 475.0 | 380.9 | |
| 0.00 | 1.48 | 0.00 | 1.01 | 2.97 | 136.78 | -42.24 | 78.21 | 0.6882 | 536.0 | 510.6 | |
| 0.00 | 2.88 | 0.00 | 1.98 | 3.65 | 136.25 | -42.77 | 77.43 | 0.6967 | -400.0 | -366.7 | |
| 0.79 | 2.27 | 0.54 | 1.56 | 2.21 | 136.15 | -42.87 | 79.49 | 0.6937 | 813.3 | 678.7 | |
| 0.00 | 0.79 | 0.00 | 0.54 | 2.65 | 135.89 | -43.13 | 78.95 | 0.6982 | 572.0 | 421.0 | |
| 0.00 | 0.87 | 0.00 | 0.60 | 2.25 | 135.66 | -43.36 | 79.58 | 0.6999 | 733.0 | 592.7 | |
| 0.00 | 2.44 | 0.00 | 1.70 | 2.09 | 135.42 | -43.60 | 79.88 | 0.7024 | 671.0 | 608.3 | |
| 2.97 | 10.83 | 2.07 | 7.53 | 2.49 | 135.32 | -43.70 | 79.35 | 0.7047 | 771.8 | 681.7 | |
| 1.83 | -13.00 | 1.28 | -13.00 | 2.23 | 135.16 | -43.86 | 79.76 | 0.7059 | 670.3 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.73 | 2.44 | 134.86 | -44.16 | 79.56 | 0.7101 | 441.0 | 358.1 | |
| 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. | |