SDO HMI 2014-10-02 11:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.97 | 58.47 | 8.55 | 33.65 | -10.26 | 140.09 | -25.41 | 123.48 | 0.5084 | 337.6 | 353.0 | |
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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 | 2.03 | 0.00 | 1.15 | -9.77 | 140.88 | -24.62 | 123.54 | 0.4947 | 404.0 | 362.5 | |
| 0.00 | 1.32 | 0.00 | 0.77 | -12.15 | 140.42 | -25.08 | 126.94 | 0.5205 | 759.0 | 630.2 | |
| 1.85 | 45.52 | 1.06 | 26.00 | -9.81 | 140.57 | -24.93 | 123.29 | 0.4989 | 1023.6 | 588.5 | |
| 3.35 | -3.00 | 1.91 | -3.00 | -9.57 | 140.56 | -24.94 | 122.85 | 0.4970 | 1117.8 | 999999 | |
| 5.90 | -3.00 | 3.36 | -3.00 | -9.19 | 140.59 | -24.91 | 122.24 | 0.4936 | 994.5 | 999999 | |
| 3.87 | -3.00 | 2.22 | -3.00 | -10.07 | 140.45 | -25.05 | 123.59 | 0.5025 | 800.4 | 999999 | |
| 0.00 | 1.32 | 0.00 | 0.77 | -11.54 | 139.91 | -25.59 | 125.42 | 0.5215 | 798.0 | 736.1 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -13.55 | 139.07 | -26.43 | 127.62 | 0.5485 | -615.0 | -467.5 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -15.14 | 137.64 | -27.86 | 128.44 | 0.5782 | -750.0 | -644.7 | |
| 0.00 | 2.03 | 0.00 | 1.21 | -12.76 | 137.78 | -27.72 | 125.14 | 0.5570 | -797.0 | -615.4 | |
| 0.00 | 1.67 | 0.00 | 1.01 | -14.63 | 137.46 | -28.04 | 127.56 | 0.5759 | -625.0 | -497.6 | |
| 0.00 | 1.50 | 0.00 | 0.90 | -12.31 | 136.82 | -28.68 | 123.55 | 0.5648 | -826.0 | -606.1 | |
| 0.00 | 1.06 | 0.00 | 0.63 | -12.48 | 136.66 | -28.84 | 123.66 | 0.5680 | -761.0 | -627.9 | |
| 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. | |