SDO HMI 2014-11-14 00:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.95 | 0.00 | 8.91 | -9.75 | 338.05 | 13.65 | 225.60 | 0.3258 | -172.3 | -232.8 | |
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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 | 1.63 | 0.00 | 0.88 | -5.55 | 345.86 | 21.45 | 248.27 | 0.3936 | 713.0 | 637.2 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -9.87 | 343.00 | 18.60 | 235.00 | 0.3853 | 668.0 | 508.2 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -10.40 | 342.18 | 17.78 | 232.63 | 0.3795 | 713.0 | 492.7 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -10.04 | 342.12 | 17.72 | 233.34 | 0.3753 | 846.0 | 734.8 | |
| 0.00 | 1.29 | 0.00 | 0.69 | -10.62 | 340.55 | 16.15 | 229.50 | 0.3610 | 942.0 | 730.7 | |
| 0.00 | 1.12 | 0.00 | 0.58 | -10.06 | 337.53 | 13.13 | 224.88 | 0.3184 | -802.0 | -675.5 | |
| 0.00 | 1.20 | 0.00 | 0.63 | -9.69 | 337.24 | 12.84 | 225.08 | 0.3106 | -810.0 | -614.8 | |
| 0.00 | 2.24 | 0.00 | 1.18 | -12.58 | 336.18 | 11.78 | 216.68 | 0.3351 | -859.0 | -716.0 | |
| 0.00 | 3.10 | 0.00 | 1.60 | -8.93 | 334.94 | 10.54 | 221.27 | 0.2752 | -901.0 | -775.9 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -8.35 | 334.16 | 9.76 | 220.56 | 0.2592 | -922.0 | -756.1 | |
| 0.00 | 1.46 | 0.00 | 0.76 | -10.53 | 333.89 | 9.49 | 214.78 | 0.2853 | -818.0 | -555.6 | |
| 0.00 | 1.03 | 0.00 | 0.53 | -10.65 | 333.58 | 9.18 | 213.68 | 0.2841 | -838.0 | -722.6 | |
| 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. | |