SDO HMI 2014-11-29 04:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.66 | 33.28 | 5.70 | 19.39 | 17.07 | 152.39 | 27.90 | 301.78 | 0.5282 | 132.9 | -21.6 | |
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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 |
| 7.18 | 10.01 | 4.27 | 5.95 | 17.50 | 154.36 | 29.87 | 300.90 | 0.5557 | 909.8 | 642.2 | |
| 0.00 | 1.37 | 0.00 | 0.82 | 17.81 | 154.38 | 29.89 | 301.39 | 0.5579 | 697.0 | 478.2 | |
| 1.71 | 2.74 | 0.99 | 1.58 | 15.43 | 152.56 | 28.08 | 298.77 | 0.5197 | 879.8 | 701.9 | |
| 0.00 | 1.28 | 0.00 | 0.74 | 15.19 | 152.35 | 27.87 | 298.51 | 0.5154 | 684.0 | 653.6 | |
| 0.00 | 1.71 | 0.00 | 0.99 | 16.54 | 152.35 | 27.86 | 300.86 | 0.5240 | 547.0 | 485.9 | |
| 0.00 | 1.63 | 0.00 | 0.94 | 16.78 | 152.25 | 27.76 | 301.37 | 0.5244 | 738.0 | 598.3 | |
| 0.00 | 1.97 | 0.00 | 1.14 | 16.51 | 151.93 | 27.44 | 301.17 | 0.5184 | 799.0 | 621.7 | |
| 0.00 | 2.65 | 0.00 | 1.53 | 17.35 | 151.19 | 26.70 | 303.25 | 0.5150 | -780.0 | -573.4 | |
| 0.00 | 1.20 | 0.00 | 0.69 | 17.29 | 150.77 | 26.28 | 303.53 | 0.5092 | -703.0 | -547.0 | |
| 0.00 | 1.97 | 0.00 | 1.13 | 17.45 | 150.51 | 26.03 | 304.04 | 0.5072 | -858.0 | -665.2 | |
| 0.00 | 1.11 | 0.00 | 0.64 | 16.89 | 150.43 | 25.94 | 303.16 | 0.5020 | -802.0 | -665.3 | |
| 0.00 | 0.77 | 0.00 | 0.44 | 17.20 | 150.41 | 25.92 | 303.71 | 0.5040 | -739.0 | -649.4 | |
| 0.77 | 2.39 | 0.44 | 1.38 | 17.94 | 150.45 | 25.97 | 304.94 | 0.5102 | -843.7 | -683.7 | |
| 0.00 | 2.48 | 0.00 | 1.42 | 17.08 | 150.29 | 25.80 | 303.62 | 0.5016 | -772.0 | -751.7 | |
| 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. | |