SDO HMI 2014-10-06 01:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.73 | 27.49 | 4.39 | 15.22 | 12.03 | 92.60 | -25.60 | 76.02 | 0.4365 | -45.5 | -101.2 | |
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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 | 0.97 | 0.00 | 0.49 | 4.17 | 105.01 | -13.19 | 99.30 | 0.2317 | -891.0 | -611.7 | |
| 0.00 | 3.07 | 0.00 | 1.59 | 9.89 | 102.14 | -16.06 | 76.84 | 0.2811 | -583.0 | -564.4 | |
| 0.00 | 1.58 | 0.00 | 0.82 | 10.94 | 100.36 | -17.84 | 74.55 | 0.3134 | -930.0 | -691.2 | |
| 0.00 | 0.61 | 0.00 | 0.32 | 12.92 | 99.19 | -19.01 | 69.58 | 0.3402 | -817.0 | -578.7 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 9.27 | 98.05 | -20.15 | 80.74 | 0.3460 | -722.0 | -509.2 | |
| 0.00 | 1.41 | 0.00 | 0.75 | 10.21 | 96.78 | -21.42 | 78.56 | 0.3682 | -711.0 | -560.4 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 10.94 | 95.35 | -22.85 | 77.24 | 0.3927 | -642.0 | -519.3 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 14.53 | 93.99 | -24.21 | 69.34 | 0.4260 | -675.0 | -452.8 | |
| 7.73 | 12.83 | 4.39 | 7.29 | 13.34 | 89.30 | -28.90 | 74.20 | 0.4907 | 1029.5 | 649.7 | |
| 0.00 | 0.70 | 0.00 | 0.41 | 16.02 | 88.33 | -29.87 | 69.37 | 0.5135 | 537.0 | 449.1 | |
| 0.00 | 1.05 | 0.00 | 0.61 | 13.39 | 88.05 | -30.15 | 74.54 | 0.5090 | 714.0 | 570.8 | |
| 0.00 | 0.61 | 0.00 | 0.36 | 13.24 | 86.92 | -31.28 | 75.19 | 0.5248 | 558.0 | 536.9 | |
| 0.00 | 0.53 | 0.00 | 0.31 | 8.72 | 84.94 | -33.26 | 83.97 | 0.5473 | -543.0 | -591.0 | |
| 0.00 | 0.97 | 0.00 | 0.58 | 10.27 | 83.22 | -34.98 | 81.32 | 0.5729 | -605.0 | -509.2 | |
| 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. | |