SDO HMI 2014-01-09 08:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.73 | 0.00 | 13.56 | -13.37 | 112.14 | 32.39 | 251.41 | 0.5528 | -97.9 | -98.6 | |
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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 | 1.28 | 0.00 | 0.90 | -10.87 | 125.33 | 45.58 | 258.66 | 0.7177 | 500.0 | 447.9 | |
| 0.00 | 1.19 | 0.00 | 0.80 | -14.28 | 121.40 | 41.65 | 253.06 | 0.6756 | 656.0 | 553.6 | |
| 0.00 | 1.02 | 0.00 | 0.66 | -11.41 | 119.83 | 40.08 | 257.00 | 0.6501 | 577.0 | 473.8 | |
| 0.00 | 0.94 | 0.00 | 0.60 | -12.30 | 118.77 | 39.02 | 255.41 | 0.6380 | 771.0 | 624.2 | |
| 0.00 | 0.68 | 0.00 | 0.44 | -12.54 | 118.66 | 38.91 | 255.01 | 0.6370 | 640.0 | 549.4 | |
| 0.00 | 1.11 | 0.00 | 0.70 | -12.24 | 117.98 | 38.24 | 255.31 | 0.6276 | 612.0 | 405.8 | |
| 0.00 | 0.51 | 0.00 | 0.31 | -12.36 | 115.76 | 36.02 | 254.53 | 0.5983 | -546.0 | -452.8 | |
| 0.00 | 0.68 | 0.00 | 0.40 | -13.76 | 111.77 | 32.03 | 250.69 | 0.5480 | -669.0 | -564.8 | |
| 0.00 | 0.77 | 0.00 | 0.45 | -17.27 | 109.89 | 30.14 | 243.49 | 0.5379 | -479.0 | -475.6 | |
| 0.00 | 3.40 | 0.00 | 1.99 | -17.21 | 109.66 | 29.92 | 243.44 | 0.5347 | -646.0 | -587.8 | |
| 0.00 | 1.28 | 0.00 | 0.74 | -16.60 | 108.99 | 29.24 | 244.11 | 0.5225 | -815.0 | -621.5 | |
| 0.00 | 2.13 | 0.00 | 1.23 | -17.15 | 108.76 | 29.02 | 242.96 | 0.5225 | -836.0 | -669.7 | |
| 0.00 | 1.79 | 0.00 | 1.03 | -16.88 | 108.65 | 28.90 | 243.37 | 0.5195 | -891.0 | -781.0 | |
| 0.00 | 1.36 | 0.00 | 0.78 | -17.56 | 107.15 | 27.40 | 241.06 | 0.5035 | -661.0 | -488.3 | |
| 0.00 | 4.59 | 0.00 | 2.53 | -6.05 | 105.68 | 25.93 | 264.29 | 0.4389 | 318.0 | 327.9 | |
| 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. | |