SDO HMI 2014-11-23 16:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.52 | 0.00 | 13.12 | -12.19 | 225.48 | 28.48 | 242.82 | 0.5254 | -164.5 | -72.2 | |
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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 | 0.94 | 0.00 | 0.57 | -13.08 | 228.61 | 31.61 | 243.65 | 0.5719 | 524.0 | 483.5 | |
| 0.00 | 1.03 | 0.00 | 0.62 | -12.41 | 228.48 | 31.48 | 244.66 | 0.5665 | 754.0 | 599.1 | |
| 0.00 | 3.94 | 0.00 | 2.36 | -12.74 | 228.28 | 31.28 | 243.98 | 0.5657 | 708.0 | 666.6 | |
| 0.00 | 2.40 | 0.00 | 1.43 | -12.77 | 227.93 | 30.92 | 243.70 | 0.5612 | 846.0 | 735.4 | |
| 0.00 | 1.28 | 0.00 | 0.76 | -12.99 | 226.58 | 29.58 | 242.37 | 0.5451 | 772.0 | 590.8 | |
| 0.00 | 1.97 | 0.00 | 1.13 | -11.87 | 223.90 | 26.90 | 242.18 | 0.5026 | -700.0 | -556.1 | |
| 0.00 | 2.23 | 0.00 | 1.27 | -11.75 | 223.69 | 26.68 | 242.23 | 0.4989 | -534.0 | -612.5 | |
| 0.00 | 0.86 | 0.00 | 0.49 | -10.23 | 223.54 | 26.54 | 244.93 | 0.4874 | -375.0 | -383.7 | |
| 0.00 | 1.97 | 0.00 | 1.12 | -11.56 | 223.50 | 26.49 | 242.41 | 0.4952 | -869.0 | -692.0 | |
| 0.00 | 1.37 | 0.00 | 0.78 | -12.02 | 223.54 | 26.54 | 241.61 | 0.4988 | -838.0 | -722.8 | |
| 0.00 | 1.71 | 0.00 | 0.98 | -12.47 | 223.36 | 26.35 | 240.63 | 0.4994 | -905.0 | -743.0 | |
| 0.00 | 1.71 | 0.00 | 0.98 | -12.66 | 223.34 | 26.34 | 240.29 | 0.5005 | -847.0 | -667.4 | |
| 0.00 | 1.11 | 0.00 | 0.63 | -10.07 | 222.85 | 25.85 | 244.68 | 0.4769 | -674.0 | -562.2 | |
| 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. | |