SDO HMI 2014-01-14 13:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.14 | 231.79 | 22.00 | 141.38 | 5.90 | 45.26 | 34.09 | 286.67 | 0.5839 | -836.8 | -358.2 | |
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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 | 0.77 | 0.00 | 0.58 | 10.84 | 58.51 | 47.34 | 288.35 | 0.7632 | -418.0 | -381.3 | |
| 0.00 | 1.53 | 0.00 | 1.17 | 11.02 | 58.46 | 47.29 | 288.59 | 0.7632 | -629.0 | -502.4 | |
| 0.00 | 0.34 | 0.00 | 0.23 | 14.54 | 50.14 | 38.97 | 296.92 | 0.6851 | -561.0 | -567.0 | |
| 0.00 | 0.94 | 0.00 | 0.61 | 10.74 | 49.22 | 38.04 | 292.13 | 0.6560 | -634.0 | -511.9 | |
| 34.18 | 216.53 | 20.85 | 132.19 | 5.82 | 45.42 | 34.25 | 286.46 | 0.5861 | -1185.7 | -371.2 | |
| 1.11 | -5.00 | 0.67 | -5.00 | 6.12 | 44.80 | 33.63 | 287.26 | 0.5788 | -978.9 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 6.74 | 44.38 | 33.21 | 288.49 | 0.5758 | -674.0 | -554.1 | |
| 0.00 | 0.60 | 0.00 | 0.35 | 8.41 | 42.00 | 30.82 | 292.72 | 0.5517 | -741.0 | -621.4 | |
| 0.00 | 1.28 | 0.00 | 0.75 | 7.59 | 41.72 | 30.55 | 291.49 | 0.5436 | -714.0 | -518.6 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 1.37 | 40.67 | 29.50 | 280.57 | 0.5028 | 542.0 | 372.9 | |
| 0.00 | 1.02 | 0.00 | 0.57 | 4.39 | 37.84 | 26.67 | 288.06 | 0.4727 | 637.0 | 461.8 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 0.50 | 36.99 | 25.82 | 280.28 | 0.4446 | 621.0 | 539.3 | |
| 0.00 | 2.38 | 0.00 | 1.31 | 2.90 | 36.25 | 25.08 | 285.98 | 0.4422 | 739.0 | 519.8 | |
| 0.85 | 1.79 | 0.48 | 1.00 | 7.21 | 36.20 | 25.03 | 294.96 | 0.4650 | -867.1 | -745.2 | |
| 0.00 | 1.62 | 0.00 | 0.90 | 7.44 | 36.09 | 24.92 | 295.53 | 0.4649 | -794.0 | -640.7 | |
| 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. | |