SDO HMI 2014-11-20 19:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.07 | 636.48 | 118.43 | 1026.18 | -13.33 | 164.74 | -70.15 | 104.88 | 0.9475 | 261.0 | -184.8 | |
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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 | 1.20 | 0.00 | 1.39 | -17.20 | 172.37 | -62.51 | 110.23 | 0.9050 | 524.0 | 434.2 | |
| 0.00 | 0.94 | 0.00 | 1.20 | -10.44 | 168.61 | -66.28 | 102.30 | 0.9232 | 179.0 | 181.9 | |
| 0.00 | 2.40 | 0.00 | 3.47 | -14.62 | 166.25 | -68.64 | 106.43 | 0.9410 | -25.0 | -63.6 | |
| 57.97 | 618.47 | 82.90 | 992.85 | -12.99 | 166.28 | -68.61 | 104.72 | 0.9396 | 510.0 | -188.8 | |
| 0.26 | -4.00 | 0.37 | -4.00 | -12.35 | 166.31 | -68.57 | 104.04 | 0.9389 | 734.3 | 999999 | |
| 5.23 | -4.00 | 9.70 | -4.00 | -14.00 | 161.47 | -73.42 | 105.18 | 0.9648 | -602.2 | 999999 | |
| 8.15 | -4.00 | 16.28 | -4.00 | -14.63 | 160.34 | -74.55 | 105.70 | 0.9699 | -208.3 | 999999 | |
| 0.00 | 2.49 | 0.00 | 4.85 | -13.97 | 160.60 | -74.29 | 105.06 | 0.9685 | -415.0 | -346.8 | |
| 0.00 | 1.80 | 0.00 | 3.64 | -13.83 | 160.14 | -74.74 | 104.87 | 0.9703 | -184.0 | -83.4 | |
| 0.00 | 1.29 | 0.00 | 2.34 | -12.13 | 161.55 | -73.34 | 103.26 | 0.9635 | -372.0 | -349.3 | |
| 1.54 | -4.00 | 3.08 | -4.00 | -13.46 | 160.25 | -74.64 | 104.50 | 0.9698 | -419.9 | 999999 | |
| 1.89 | 5.32 | 3.77 | 10.62 | -12.70 | 160.08 | -74.80 | 103.70 | 0.9701 | 120.9 | 113.8 | |
| 1.03 | 2.57 | 2.33 | 5.82 | -14.14 | 158.46 | -76.43 | 105.02 | 0.9769 | -77.2 | -23.8 | |
| 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. | |