SDO HMI 2014-11-08 03:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.43 | 0.00 | 10.02 | -15.44 | 18.33 | -23.53 | 130.26 | 0.5030 | -80.8 | -271.6 | |
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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 | 0.60 | 0.00 | 0.32 | -12.12 | 27.53 | -14.33 | 138.12 | 0.3641 | 748.0 | 560.7 | |
| 0.00 | 0.86 | 0.00 | 0.47 | -13.60 | 24.48 | -17.38 | 135.34 | 0.4147 | 691.0 | 502.1 | |
| 0.00 | 1.29 | 0.00 | 0.71 | -14.46 | 23.12 | -18.74 | 134.69 | 0.4394 | 683.0 | 579.9 | |
| 0.00 | 1.73 | 0.00 | 0.96 | -13.66 | 21.50 | -20.36 | 130.99 | 0.4497 | 800.0 | 698.6 | |
| 0.00 | 0.69 | 0.00 | 0.39 | -13.83 | 20.60 | -21.26 | 130.08 | 0.4620 | 712.0 | 544.6 | |
| 0.00 | 3.80 | 0.00 | 2.13 | -13.94 | 20.10 | -21.76 | 129.61 | 0.4690 | -624.0 | -560.8 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -16.29 | 16.32 | -25.54 | 129.00 | 0.5347 | -724.0 | -604.2 | |
| 0.00 | 3.37 | 0.00 | 1.97 | -16.21 | 15.95 | -25.91 | 128.49 | 0.5381 | -758.0 | -808.4 | |
| 0.00 | 1.29 | 0.00 | 0.77 | -17.84 | 15.46 | -26.40 | 130.39 | 0.5579 | -710.0 | -505.5 | |
| 0.00 | 1.04 | 0.00 | 0.62 | -17.72 | 15.13 | -26.73 | 129.88 | 0.5605 | -754.0 | -669.0 | |
| 0.00 | 1.21 | 0.00 | 0.74 | -19.06 | 14.12 | -27.74 | 130.76 | 0.5830 | -531.0 | -446.6 | |
| 0.00 | 0.60 | 0.00 | 0.38 | -15.91 | 8.29 | -33.57 | 121.41 | 0.6253 | -503.0 | -440.0 | |
| 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. | |