SDO HMI 2014-11-03 10:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.38 | 33.65 | 5.49 | 18.03 | -17.26 | 98.70 | -5.26 | 167.63 | 0.3835 | 14.3 | 6.4 | |
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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 |
| 5.62 | 12.20 | 2.97 | 6.45 | -16.33 | 103.77 | -0.19 | 179.49 | 0.3513 | 1103.4 | 767.8 | |
| 3.29 | -1.00 | 1.74 | -1.00 | -16.39 | 103.62 | -0.34 | 179.07 | 0.3524 | 977.8 | 999999 | |
| 0.00 | 1.56 | 0.00 | 0.82 | -16.24 | 101.54 | -2.42 | 173.37 | 0.3521 | 806.0 | 534.7 | |
| 1.47 | 6.75 | 0.78 | 3.58 | -16.78 | 100.29 | -3.67 | 170.26 | 0.3638 | 1107.3 | 809.2 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -16.94 | 100.16 | -3.80 | 170.01 | 0.3667 | 700.0 | 539.4 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -16.91 | 95.79 | -8.17 | 159.22 | 0.3851 | -993.0 | -872.5 | |
| 0.00 | 1.04 | 0.00 | 0.56 | -18.24 | 94.08 | -9.88 | 156.76 | 0.4150 | -823.0 | -614.2 | |
| 0.00 | 1.47 | 0.00 | 0.80 | -18.08 | 93.74 | -10.22 | 155.89 | 0.4149 | -858.0 | -612.4 | |
| 0.00 | 2.77 | 0.00 | 1.51 | -18.12 | 93.48 | -10.48 | 155.40 | 0.4171 | -801.0 | -665.8 | |
| 0.00 | 1.90 | 0.00 | 1.05 | -19.18 | 91.42 | -12.54 | 152.51 | 0.4463 | -715.0 | -512.5 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -16.20 | 91.47 | -12.49 | 149.03 | 0.4052 | -686.0 | -501.1 | |
| 0.00 | 1.30 | 0.00 | 0.72 | -19.96 | 91.13 | -12.83 | 152.83 | 0.4591 | -849.0 | -750.7 | |
| 0.00 | 1.04 | 0.00 | 0.58 | -20.82 | 90.92 | -13.04 | 153.35 | 0.4721 | -736.0 | -596.5 | |
| 0.00 | 0.69 | 0.00 | 0.38 | -19.70 | 90.92 | -13.04 | 152.18 | 0.4570 | -652.0 | -541.5 | |
| 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. | |