SDO HMI 2014-01-07 11:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.00 | 0.00 | 8.23 | -17.13 | 75.11 | -29.34 | 117.20 | 0.5242 | -3.1 | 80.7 | |
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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 | 1.10 | 0.00 | 0.61 | -19.03 | 82.98 | -21.47 | 127.74 | 0.4395 | 577.0 | 503.8 | |
| 0.00 | 0.93 | 0.00 | 0.51 | -13.51 | 82.76 | -21.69 | 115.87 | 0.4010 | -746.0 | -565.5 | |
| 0.00 | 2.21 | 0.00 | 1.23 | -13.81 | 79.32 | -25.13 | 113.68 | 0.4522 | -606.0 | -376.8 | |
| 0.00 | 0.93 | 0.00 | 0.52 | -13.31 | 78.64 | -25.81 | 112.17 | 0.4594 | -606.0 | -457.9 | |
| 0.00 | 1.19 | 0.00 | 0.67 | -13.07 | 77.59 | -26.86 | 111.00 | 0.4734 | -573.0 | -518.7 | |
| 0.00 | 1.02 | 0.00 | 0.57 | -13.24 | 77.26 | -27.19 | 111.15 | 0.4789 | -659.0 | -501.7 | |
| 0.00 | 0.34 | 0.00 | 0.19 | -15.17 | 76.38 | -28.07 | 114.35 | 0.5005 | 677.0 | 685.5 | |
| 0.00 | 1.78 | 0.00 | 1.05 | -17.21 | 73.97 | -30.48 | 116.49 | 0.5436 | 701.0 | 497.3 | |
| 0.00 | 1.53 | 0.00 | 0.92 | -20.25 | 73.23 | -31.21 | 121.07 | 0.5699 | 796.0 | 660.2 | |
| 0.00 | 2.29 | 0.00 | 1.39 | -21.11 | 72.89 | -31.56 | 122.19 | 0.5793 | 753.0 | 656.3 | |
| 0.00 | 0.68 | 0.00 | 0.57 | -23.45 | 52.62 | -51.83 | 116.53 | 0.8084 | -348.0 | -348.4 | |
| 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. | |