SDO HMI 2014-09-24 08:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.12 | 25.73 | 1.28 | 15.48 | -15.46 | 246.33 | -26.39 | 130.79 | 0.5679 | -757.6 | -679.5 | |
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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 | 2.39 | 0.00 | 1.42 | -15.54 | 247.43 | -25.29 | 132.10 | 0.5568 | -749.0 | -580.1 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -15.42 | 247.20 | -25.51 | 131.69 | 0.5581 | -770.0 | -661.3 | |
| 0.00 | 1.59 | 0.00 | 0.95 | -15.59 | 247.04 | -25.67 | 131.74 | 0.5615 | -859.0 | -718.9 | |
| 0.00 | 1.50 | 0.00 | 0.90 | -15.40 | 247.00 | -25.72 | 131.43 | 0.5601 | -709.0 | -603.2 | |
| 0.00 | 1.15 | 0.00 | 0.69 | -15.72 | 246.54 | -26.18 | 131.37 | 0.5680 | -616.0 | -526.8 | |
| 0.00 | 4.51 | 0.00 | 2.71 | -15.24 | 246.40 | -26.32 | 130.55 | 0.5652 | -821.0 | -753.2 | |
| 0.00 | 1.06 | 0.00 | 0.64 | -15.38 | 246.13 | -26.59 | 130.47 | 0.5694 | -811.0 | -767.8 | |
| 0.00 | 3.98 | 0.00 | 2.41 | -15.95 | 245.87 | -26.84 | 130.98 | 0.5772 | -729.0 | -631.0 | |
| 2.12 | 5.04 | 1.28 | 3.04 | -15.36 | 245.89 | -26.83 | 130.19 | 0.5719 | -906.5 | -693.4 | |
| 0.00 | 2.39 | 0.00 | 1.44 | -15.10 | 245.93 | -26.79 | 129.87 | 0.5691 | -911.0 | -795.3 | |
| 0.00 | 1.24 | 0.00 | 0.75 | -15.38 | 245.68 | -27.04 | 129.99 | 0.5743 | -410.0 | -622.8 | |
| 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. | |