SDO HMI 2014-11-06 23:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.43 | 138.35 | 24.28 | 136.83 | 13.39 | 117.19 | 59.95 | 283.26 | 0.8667 | -488.7 | -197.3 | |
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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 |
| 21.58 | 119.10 | 21.82 | 120.52 | 13.96 | 117.95 | 60.71 | 283.89 | 0.8739 | -721.8 | -213.3 | |
| 0.00 | 1.99 | 0.00 | 1.72 | 7.71 | 112.49 | 55.25 | 276.76 | 0.8221 | -476.0 | -392.7 | |
| 0.43 | 8.89 | 0.37 | 7.67 | 7.89 | 112.48 | 55.23 | 276.98 | 0.8220 | -619.8 | -506.7 | |
| 0.00 | 0.69 | 0.00 | 0.62 | 13.24 | 113.87 | 56.62 | 283.37 | 0.8377 | -550.0 | -510.2 | |
| 1.64 | -3.00 | 1.42 | -3.00 | 8.08 | 112.36 | 55.11 | 277.21 | 0.8208 | -680.1 | 999999 | |
| 0.78 | -3.00 | 0.67 | -3.00 | 7.91 | 112.17 | 54.92 | 277.01 | 0.8189 | -727.6 | 999999 | |
| 0.00 | 2.33 | 0.00 | 1.92 | 8.33 | 110.55 | 53.30 | 277.57 | 0.8026 | 529.0 | 426.2 | |
| 0.00 | 0.86 | 0.00 | 0.71 | 10.92 | 110.43 | 53.19 | 280.81 | 0.8026 | 356.0 | 307.1 | |
| 0.00 | 0.78 | 0.00 | 0.65 | 12.17 | 110.68 | 53.44 | 282.35 | 0.8060 | 382.0 | 311.0 | |
| 0.00 | 0.86 | 0.00 | 0.70 | 7.96 | 109.63 | 52.38 | 277.13 | 0.7929 | 566.0 | 522.1 | |
| 0.00 | 1.21 | 0.00 | 1.00 | 13.12 | 110.46 | 53.22 | 283.55 | 0.8046 | 472.0 | 363.8 | |
| 0.00 | 1.64 | 0.00 | 1.32 | 12.28 | 109.15 | 51.91 | 282.64 | 0.7904 | 508.0 | 387.8 | |
| 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. | |