SDO HMI 2011-10-05 14:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.59 | 88.98 | 52.39 | 172.23 | -14.05 | 117.08 | -72.52 | 106.52 | 0.9655 | 165.9 | -228.5 | |
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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 |
| 0.44 | 59.81 | 0.75 | 106.67 | -14.17 | 119.00 | -70.60 | 107.00 | 0.9576 | -183.0 | -338.1 | |
| 10.28 | -1.00 | 17.21 | -1.00 | -13.87 | 119.12 | -70.48 | 106.72 | 0.9568 | 351.0 | 999999 | |
| 7.90 | -1.00 | 14.16 | -1.00 | -13.75 | 117.95 | -71.65 | 106.37 | 0.9621 | 315.5 | 999999 | |
| 0.00 | 0.97 | 0.00 | 1.90 | -15.11 | 116.73 | -72.87 | 107.52 | 0.9686 | -338.0 | -321.7 | |
| 2.11 | 3.34 | 3.74 | 5.89 | -13.15 | 117.99 | -71.61 | 105.76 | 0.9614 | 274.0 | 394.7 | |
| 0.00 | 0.70 | 0.00 | 1.42 | -15.00 | 116.29 | -73.31 | 107.32 | 0.9703 | -237.0 | -184.0 | |
| 0.97 | 2.99 | 2.08 | 6.46 | -15.36 | 115.39 | -74.22 | 107.51 | 0.9741 | -157.3 | -151.1 | |
| 0.79 | -7.00 | 1.73 | -7.00 | -15.42 | 115.09 | -74.52 | 107.53 | 0.9752 | 155.6 | 999999 | |
| 0.00 | 1.58 | 0.00 | 3.10 | -13.66 | 116.46 | -73.14 | 106.00 | 0.9685 | 57.0 | 14.1 | |
| 0.00 | 4.22 | 0.00 | 8.63 | -13.67 | 115.79 | -73.81 | 105.88 | 0.9713 | -71.0 | -73.8 | |
| 0.00 | 1.93 | 0.00 | 4.47 | -14.86 | 114.20 | -75.40 | 106.80 | 0.9780 | -485.0 | -390.6 | |
| 2.90 | 12.12 | 7.15 | 30.50 | -14.67 | 113.37 | -76.23 | 106.46 | 0.9807 | -262.6 | 82.1 | |
| 2.20 | -12.00 | 5.57 | -12.00 | -14.67 | 113.10 | -76.50 | 106.42 | 0.9815 | 288.3 | 999999 | |
| 0.00 | 1.32 | 0.00 | 3.19 | -14.08 | 113.60 | -76.00 | 105.91 | 0.9796 | -303.0 | -274.5 | |
| 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. | |