SDO HMI 2014-11-08 09:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.35 | 22.53 | 0.19 | 12.53 | -14.99 | 19.25 | -19.33 | 135.07 | 0.4510 | -100.8 | -212.3 | |
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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 |
| 0.00 | 0.86 | 0.00 | 0.45 | -12.09 | 27.61 | -10.97 | 145.38 | 0.3289 | 849.0 | 696.4 | |
| 0.00 | 1.73 | 0.00 | 0.93 | -14.73 | 24.72 | -13.86 | 143.48 | 0.3911 | 706.0 | 542.4 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -13.63 | 23.62 | -14.96 | 139.55 | 0.3884 | 799.0 | 681.0 | |
| 0.00 | 1.04 | 0.00 | 0.56 | -12.92 | 23.25 | -15.32 | 137.62 | 0.3839 | 668.0 | 492.7 | |
| 0.00 | 1.55 | 0.00 | 0.84 | -13.47 | 21.92 | -16.66 | 136.23 | 0.4049 | 921.0 | 789.8 | |
| 0.00 | 2.07 | 0.00 | 1.12 | -13.28 | 21.74 | -16.84 | 135.61 | 0.4048 | 850.0 | 740.7 | |
| 0.35 | 5.00 | 0.19 | 2.75 | -14.00 | 20.01 | -18.57 | 134.10 | 0.4321 | -948.8 | -772.8 | |
| 0.00 | 1.64 | 0.00 | 0.93 | -16.31 | 16.32 | -22.26 | 132.77 | 0.4972 | -852.0 | -574.1 | |
| 0.00 | 2.76 | 0.00 | 1.58 | -16.22 | 15.83 | -22.75 | 132.03 | 0.5019 | -867.0 | -809.2 | |
| 0.00 | 1.47 | 0.00 | 0.84 | -16.57 | 15.75 | -22.83 | 132.47 | 0.5061 | -706.0 | -642.5 | |
| 0.00 | 1.04 | 0.00 | 0.60 | -17.76 | 15.29 | -23.29 | 133.68 | 0.5227 | -827.0 | -674.8 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -18.85 | 15.06 | -23.52 | 134.97 | 0.5359 | -588.0 | -471.3 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -16.55 | 15.32 | -23.26 | 131.91 | 0.5108 | -530.0 | -381.9 | |
| 0.00 | 0.78 | 0.00 | 0.45 | -15.39 | 14.08 | -24.50 | 128.68 | 0.5142 | -724.0 | -677.4 | |
| 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. | |