SDO HMI 2014-11-15 02:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.90 | 0.00 | 7.55 | -9.72 | 339.39 | 29.27 | 245.72 | 0.5295 | -231.2 | -193.4 | |
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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 | 0.95 | 0.00 | 0.62 | -8.53 | 349.18 | 39.06 | 253.34 | 0.6528 | -500.0 | -454.5 | |
| 0.00 | 1.12 | 0.00 | 0.68 | -4.29 | 345.36 | 35.25 | 258.65 | 0.5892 | 97.0 | 161.5 | |
| 0.00 | 1.20 | 0.00 | 0.72 | -9.38 | 342.45 | 32.33 | 248.82 | 0.5681 | 780.0 | 573.8 | |
| 0.00 | 0.77 | 0.00 | 0.47 | -10.44 | 342.50 | 32.38 | 247.09 | 0.5740 | 617.0 | 545.2 | |
| 0.00 | 1.46 | 0.00 | 0.88 | -10.53 | 342.33 | 32.21 | 246.84 | 0.5722 | 661.0 | 497.4 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -8.73 | 337.33 | 27.21 | 246.60 | 0.4945 | -610.0 | -475.8 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -9.36 | 335.73 | 25.62 | 244.13 | 0.4761 | -723.0 | -570.1 | |
| 0.00 | 1.20 | 0.00 | 0.69 | -12.32 | 335.94 | 25.82 | 238.86 | 0.4992 | -548.0 | -452.6 | |
| 0.00 | 1.38 | 0.00 | 0.78 | -11.33 | 335.60 | 25.49 | 240.31 | 0.4877 | -897.0 | -708.2 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -10.98 | 334.87 | 24.75 | 240.26 | 0.4753 | -637.0 | -510.0 | |
| 0.00 | 1.81 | 0.00 | 1.01 | -10.38 | 334.12 | 24.00 | 240.65 | 0.4610 | -783.0 | -648.5 | |
| 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. | |