SDO HMI 2014-11-11 09:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.16 | 0.00 | 8.30 | -10.78 | 337.97 | -21.06 | 124.35 | 0.4287 | -45.6 | -99.4 | |
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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 |
| 0.00 | 0.86 | 0.00 | 0.45 | -9.10 | 343.11 | -15.91 | 128.10 | 0.3455 | 823.0 | 700.0 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -5.03 | 343.14 | -15.89 | 117.56 | 0.3090 | 809.0 | 686.5 | |
| 0.00 | 1.46 | 0.00 | 0.78 | -9.81 | 342.89 | -16.13 | 129.31 | 0.3555 | 875.0 | 727.5 | |
| 0.00 | 1.64 | 0.00 | 0.89 | -13.23 | 340.25 | -18.78 | 131.90 | 0.4228 | 922.0 | 700.3 | |
| 0.00 | 1.55 | 0.00 | 0.84 | -11.08 | 339.93 | -19.09 | 127.34 | 0.4055 | 712.0 | 545.2 | |
| 0.00 | 2.76 | 0.00 | 1.53 | -12.27 | 336.92 | -22.11 | 125.68 | 0.4546 | -620.0 | -638.3 | |
| 0.00 | 1.29 | 0.00 | 0.71 | -10.11 | 336.31 | -22.71 | 120.87 | 0.4447 | -973.0 | -821.3 | |
| 0.00 | 1.55 | 0.00 | 0.87 | -10.85 | 334.54 | -24.49 | 120.43 | 0.4741 | -752.0 | -625.3 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -10.22 | 334.33 | -24.70 | 119.03 | 0.4723 | -770.0 | -601.8 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -11.17 | 334.24 | -24.78 | 120.71 | 0.4803 | -740.0 | -562.2 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -10.96 | 333.93 | -25.10 | 120.02 | 0.4829 | -788.0 | -596.4 | |
| 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. | |