SDO HMI 2014-11-16 17:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.27 | 29.39 | 7.94 | 34.85 | -12.42 | 224.73 | -63.99 | 104.99 | 0.9097 | -73.3 | -0.2 | |
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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 | 0.63 | -13.01 | 228.61 | -60.11 | 106.34 | 0.8822 | 366.0 | 322.1 | |
| 0.69 | 1.55 | 0.72 | 1.62 | -12.83 | 228.44 | -60.28 | 106.11 | 0.8833 | 523.2 | 455.8 | |
| 0.00 | 1.46 | 0.00 | 1.59 | -13.74 | 227.42 | -61.30 | 106.91 | 0.8925 | 296.0 | 203.0 | |
| 0.00 | 1.55 | 0.00 | 1.62 | -11.44 | 228.23 | -60.49 | 104.50 | 0.8830 | 297.0 | 274.8 | |
| 0.00 | 0.60 | 0.00 | 0.67 | -14.19 | 226.82 | -61.90 | 107.29 | 0.8976 | -440.0 | -372.3 | |
| 0.00 | 0.26 | 0.00 | 0.27 | -11.12 | 227.72 | -61.00 | 104.06 | 0.8866 | 219.0 | 249.3 | |
| 0.00 | 0.77 | 0.00 | 0.88 | -14.07 | 226.08 | -62.64 | 107.02 | 0.9028 | -350.0 | -257.8 | |
| 0.00 | 1.98 | 0.00 | 2.18 | -11.96 | 226.76 | -61.96 | 104.82 | 0.8950 | 313.0 | 238.0 | |
| 0.00 | 1.03 | 0.00 | 1.18 | -13.74 | 225.98 | -62.75 | 106.63 | 0.9031 | -445.0 | -380.6 | |
| 0.00 | 0.52 | 0.00 | 0.57 | -11.53 | 226.74 | -61.98 | 104.34 | 0.8947 | 265.0 | 219.0 | |
| 0.00 | 4.55 | 0.00 | 5.00 | -11.35 | 226.74 | -61.98 | 104.14 | 0.8944 | 455.0 | 313.3 | |
| 0.00 | 0.77 | 0.00 | 0.89 | -12.92 | 225.55 | -63.17 | 105.67 | 0.9052 | -302.0 | -322.4 | |
| 5.58 | 12.46 | 7.22 | 16.07 | -12.50 | 222.52 | -66.20 | 104.72 | 0.9253 | -384.0 | -322.5 | |
| 0.00 | 1.29 | 0.00 | 1.68 | -12.18 | 222.22 | -66.50 | 104.33 | 0.9268 | 261.0 | 240.5 | |
| 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. | |