SDO HMI 2014-01-07 23:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.38 | 0.00 | 9.40 | -16.75 | 71.50 | -26.33 | 119.82 | 0.4840 | -93.1 | -153.7 | |
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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 | 0.85 | 0.00 | 0.45 | -19.15 | 83.06 | -14.77 | 137.93 | 0.3610 | 746.0 | 622.4 | |
| 0.00 | 1.02 | 0.00 | 0.55 | -19.55 | 81.76 | -16.08 | 136.40 | 0.3800 | 738.0 | 491.9 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -13.67 | 79.86 | -17.98 | 120.22 | 0.3486 | -773.0 | -697.2 | |
| 0.00 | 1.27 | 0.00 | 0.67 | -13.57 | 79.32 | -18.51 | 119.29 | 0.3554 | -745.0 | -584.9 | |
| 0.00 | 1.53 | 0.00 | 0.81 | -13.33 | 79.12 | -18.72 | 118.43 | 0.3566 | -822.0 | -640.7 | |
| 0.00 | 0.51 | 0.00 | 0.27 | -13.24 | 77.97 | -19.86 | 116.92 | 0.3726 | -706.0 | -592.3 | |
| 0.00 | 1.19 | 0.00 | 0.65 | -15.27 | 76.28 | -21.56 | 119.85 | 0.4105 | 829.0 | 701.0 | |
| 0.00 | 0.42 | 0.00 | 0.24 | -19.79 | 73.48 | -24.36 | 125.92 | 0.4812 | 561.0 | 474.2 | |
| 0.00 | 1.10 | 0.00 | 0.63 | -20.80 | 73.10 | -24.74 | 127.31 | 0.4939 | 852.0 | 612.2 | |
| 0.00 | 1.53 | 0.00 | 0.88 | -21.90 | 72.82 | -25.01 | 128.91 | 0.5062 | 627.0 | 417.0 | |
| 0.00 | 1.53 | 0.00 | 0.87 | -12.47 | 68.73 | -29.10 | 108.52 | 0.5029 | -848.0 | -656.4 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -12.32 | 68.68 | -29.15 | 108.20 | 0.5030 | -623.0 | -561.2 | |
| 0.00 | 1.19 | 0.00 | 0.76 | -16.32 | 59.51 | -38.32 | 111.18 | 0.6405 | -574.0 | -449.2 | |
| 0.00 | 0.85 | 0.00 | 0.57 | -18.60 | 57.10 | -40.73 | 113.64 | 0.6774 | -263.0 | -326.8 | |
| 0.00 | 0.93 | 0.00 | 0.69 | -23.33 | 52.35 | -45.49 | 118.31 | 0.7460 | -395.0 | -410.0 | |
| 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. | |