SDO HMI 2014-11-04 15:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.23 | 202.26 | 49.12 | 451.06 | 15.07 | 11.05 | -76.98 | 75.44 | 0.9712 | 25.5 | 160.9 | |
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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 | 0.26 | 0.00 | 0.43 | 17.90 | 14.92 | -73.12 | 72.49 | 0.9561 | -307.0 | -302.0 | |
| 0.00 | 0.78 | 0.00 | 1.49 | 18.72 | 12.53 | -75.50 | 71.69 | 0.9670 | -163.0 | -117.4 | |
| 15.29 | 90.02 | 24.88 | 146.93 | 14.78 | 15.35 | -72.68 | 75.76 | 0.9537 | -392.1 | -139.5 | |
| 0.00 | 0.26 | 0.00 | 0.53 | 14.89 | 11.46 | -76.57 | 75.65 | 0.9714 | 559.0 | 510.0 | |
| 0.00 | 1.64 | 0.00 | 3.35 | 14.71 | 11.53 | -76.50 | 75.83 | 0.9711 | 525.0 | 499.3 | |
| 1.90 | 90.89 | 4.05 | 229.23 | 14.66 | 10.89 | -77.14 | 75.87 | 0.9736 | 278.6 | 320.4 | |
| 4.67 | -6.00 | 10.69 | -6.00 | 14.94 | 9.97 | -78.07 | 75.58 | 0.9771 | 589.2 | 999999 | |
| 0.00 | 3.46 | 0.00 | 9.91 | 16.54 | 7.14 | -80.90 | 73.89 | 0.9860 | 191.0 | 190.4 | |
| 2.42 | -6.00 | 5.51 | -6.00 | 14.30 | 10.01 | -78.02 | 76.23 | 0.9769 | 207.7 | 999999 | |
| 0.00 | 1.90 | 0.00 | 8.49 | 17.70 | 3.50 | -84.53 | 72.62 | 0.9942 | -201.0 | -183.2 | |
| 0.95 | 4.15 | 3.99 | 17.67 | 17.17 | 3.93 | -84.10 | 73.17 | 0.9935 | 187.9 | 92.2 | |
| 0.00 | 2.25 | 0.00 | 7.61 | 16.56 | 5.55 | -82.48 | 73.83 | 0.9901 | 459.0 | 424.0 | |
| 0.00 | 3.11 | 0.00 | 12.73 | 16.87 | 4.20 | -83.84 | 73.47 | 0.9930 | 392.0 | 345.0 | |
| 0.00 | 0.95 | 0.00 | 2.60 | 14.82 | 7.78 | -80.25 | 75.65 | 0.9843 | 56.0 | 43.5 | |
| 0.00 | 2.59 | 0.00 | 10.09 | 16.07 | 4.35 | -83.68 | 74.28 | 0.9927 | 431.0 | 375.0 | |
| 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. | |