SDO HMI 2014-01-14 06:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.39 | 232.59 | 23.60 | 135.94 | 5.92 | 45.20 | 30.21 | 288.92 | 0.5306 | -824.3 | -374.5 | |
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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 | 1.70 | 0.00 | 1.26 | 11.56 | 60.32 | 45.32 | 289.99 | 0.7437 | -590.0 | -512.5 | |
| 0.00 | 0.77 | 0.00 | 0.54 | 10.90 | 58.46 | 43.46 | 289.87 | 0.7206 | -413.0 | -436.0 | |
| 0.00 | 1.02 | 0.00 | 0.66 | 8.98 | 52.93 | 37.93 | 289.61 | 0.6469 | -556.0 | -467.7 | |
| 0.00 | 0.68 | 0.00 | 0.42 | 10.40 | 48.88 | 33.89 | 293.96 | 0.6024 | -551.0 | -491.6 | |
| 40.39 | 217.69 | 23.60 | 127.27 | 5.73 | 45.42 | 30.43 | 288.28 | 0.5329 | -1200.4 | -395.6 | |
| 0.00 | 1.53 | 0.00 | 0.84 | 3.43 | 38.64 | 23.64 | 288.12 | 0.4230 | 698.0 | 522.5 | |
| 0.00 | 3.23 | 0.00 | 1.75 | 7.06 | 35.67 | 20.68 | 299.08 | 0.4027 | -877.0 | -747.2 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 12.43 | 35.32 | 20.33 | 310.13 | 0.4456 | 636.0 | 588.5 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 6.87 | 34.37 | 19.37 | 300.29 | 0.3831 | -426.0 | -408.6 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 6.94 | 33.49 | 18.50 | 301.62 | 0.3715 | 539.0 | 386.5 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 6.94 | 33.24 | 18.25 | 301.96 | 0.3679 | 555.0 | 500.4 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 11.58 | 28.98 | 13.99 | 319.19 | 0.3640 | 793.0 | 667.8 | |
| 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. | |