SDO HMI 2014-01-14 05:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 85.37 | 462.07 | 43.28 | 234.26 | -16.50 | 13.02 | -2.52 | 168.59 | 0.2144 | 1183.1 | 435.3 | |
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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 | 2.04 | 0.00 | 1.04 | -18.47 | 17.78 | 2.24 | 188.71 | 0.2460 | 740.0 | 579.0 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -17.02 | 17.15 | 1.61 | 187.03 | 0.2200 | 728.0 | 571.6 | |
| 44.64 | 282.98 | 22.63 | 143.42 | -16.62 | 13.70 | -1.84 | 171.68 | 0.2138 | 1451.5 | 485.8 | |
| 4.08 | -3.00 | 2.07 | -3.00 | -16.68 | 13.05 | -2.49 | 168.88 | 0.2167 | 1127.5 | 999999 | |
| 0.00 | 1.87 | 0.00 | 0.95 | -16.77 | 12.68 | -2.86 | 167.37 | 0.2194 | 782.0 | 659.0 | |
| 0.00 | 2.89 | 0.00 | 1.46 | -15.93 | 12.66 | -2.88 | 166.35 | 0.2055 | 816.0 | 755.3 | |
| 0.00 | 1.62 | 0.00 | 0.82 | -15.63 | 12.54 | -3.00 | 165.43 | 0.2010 | 746.0 | 490.7 | |
| 5.44 | 162.92 | 2.76 | 82.62 | -16.56 | 12.22 | -3.32 | 165.17 | 0.2178 | 1140.6 | 352.5 | |
| 0.00 | 2.98 | 0.00 | 1.50 | -14.93 | 12.13 | -3.41 | 162.44 | 0.1915 | 923.0 | 710.7 | |
| 29.85 | -8.00 | 15.13 | -8.00 | -16.22 | 12.01 | -3.53 | 163.84 | 0.2132 | 1344.6 | 999999 | |
| 1.36 | -8.00 | 0.69 | -8.00 | -15.95 | 11.71 | -3.83 | 162.13 | 0.2103 | 1036.1 | 999999 | |
| 0.00 | 1.70 | 0.00 | 0.87 | -16.88 | 7.38 | -8.16 | 147.81 | 0.2560 | -1033.0 | -829.5 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -18.66 | 4.55 | -10.99 | 143.77 | 0.3069 | -635.0 | -558.4 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -18.40 | 3.52 | -12.02 | 140.81 | 0.3140 | -600.0 | -549.0 | |
| 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. | |