SDO HMI 2014-02-25 15:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.44 | 17.38 | 2.93 | 15.13 | 6.13 | 123.48 | -53.55 | 77.26 | 0.8181 | -229.3 | -273.7 | |
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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 | 1.03 | 0.00 | 0.83 | 9.09 | 127.76 | -49.27 | 72.43 | 0.7872 | -651.0 | -558.1 | |
| 0.00 | 0.43 | 0.00 | 0.35 | 9.70 | 127.55 | -49.48 | 71.77 | 0.7912 | -345.0 | -344.4 | |
| 0.00 | 1.46 | 0.00 | 1.19 | 10.01 | 127.25 | -49.78 | 71.50 | 0.7952 | -481.0 | -365.8 | |
| 0.00 | 0.60 | 0.00 | 0.49 | 9.83 | 127.15 | -49.88 | 71.75 | 0.7957 | -434.0 | -404.1 | |
| 0.00 | 1.12 | 0.00 | 0.87 | 4.57 | 127.65 | -49.38 | 78.08 | 0.7756 | -623.0 | -520.3 | |
| 0.00 | 3.44 | 0.00 | 2.77 | 6.74 | 126.79 | -50.24 | 75.63 | 0.7903 | -656.0 | -526.8 | |
| 3.44 | 6.63 | 2.93 | 5.64 | 3.96 | 123.73 | -53.30 | 79.88 | 0.8148 | -633.0 | -426.4 | |
| 0.00 | 0.26 | 0.00 | 0.23 | 5.02 | 122.80 | -54.23 | 78.85 | 0.8260 | 405.0 | 453.3 | |
| 0.00 | 0.52 | 0.00 | 0.48 | 5.04 | 120.59 | -56.45 | 79.37 | 0.8468 | 525.0 | 478.5 | |
| 0.00 | 0.77 | 0.00 | 0.71 | 4.32 | 120.57 | -56.47 | 80.22 | 0.8456 | 404.0 | 351.9 | |
| 0.00 | 0.52 | 0.00 | 0.48 | 4.50 | 120.55 | -56.49 | 80.01 | 0.8461 | 338.0 | 301.0 | |
| 0.00 | 0.60 | 0.00 | 1.09 | 10.40 | 104.72 | -72.31 | 77.00 | 0.9629 | 179.0 | 203.7 | |
| 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. | |