SDO HMI 2014-07-22 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.21 | 155.24 | 21.62 | 98.20 | -21.00 | 68.87 | 28.80 | 226.36 | 0.6234 | 352.4 | 211.2 | |
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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 |
| 26.59 | 118.23 | 16.93 | 75.34 | -20.91 | 69.70 | 29.63 | 227.31 | 0.6306 | 1023.7 | 295.5 | |
| 0.00 | 1.00 | 0.00 | 0.62 | -20.18 | 68.54 | 28.47 | 227.13 | 0.6128 | 773.0 | 539.5 | |
| 1.36 | 10.16 | 0.86 | 6.39 | -21.08 | 68.32 | 28.25 | 225.78 | 0.6184 | 775.7 | 689.6 | |
| 0.00 | 1.36 | 0.00 | 0.85 | -20.47 | 68.16 | 28.09 | 226.39 | 0.6114 | 825.0 | 648.0 | |
| 0.00 | 1.36 | 0.00 | 0.84 | -19.97 | 67.62 | 27.55 | 226.49 | 0.6016 | 612.0 | 535.3 | |
| 0.00 | 1.54 | 0.00 | 0.95 | -21.86 | 65.79 | 25.72 | 222.24 | 0.6013 | -564.0 | -537.6 | |
| 0.00 | 1.18 | 0.00 | 0.73 | -22.33 | 65.70 | 25.63 | 221.58 | 0.6050 | -602.0 | -550.0 | |
| 0.00 | 2.18 | 0.00 | 1.34 | -21.26 | 65.42 | 25.35 | 222.56 | 0.5921 | -879.0 | -717.5 | |
| 0.00 | 1.09 | 0.00 | 0.67 | -21.54 | 65.47 | 25.40 | 222.28 | 0.5952 | -652.0 | -510.5 | |
| 0.00 | 1.27 | 0.00 | 0.78 | -21.83 | 65.20 | 25.13 | 221.63 | 0.5956 | -469.0 | -483.7 | |
| 0.82 | 1.81 | 0.50 | 1.11 | -21.62 | 65.09 | 25.02 | 221.76 | 0.5925 | -777.3 | -649.6 | |
| 5.08 | 7.62 | 3.11 | 4.67 | -21.64 | 64.77 | 24.70 | 221.38 | 0.5897 | -871.8 | -663.8 | |
| 0.00 | 1.54 | 0.00 | 0.94 | -20.79 | 64.58 | 24.51 | 222.21 | 0.5794 | -734.0 | -613.5 | |
| 0.00 | 2.63 | 0.00 | 1.59 | -21.01 | 64.12 | 24.04 | 221.41 | 0.5772 | -725.0 | -492.0 | |
| 0.36 | 2.27 | 0.22 | 1.38 | -22.05 | 63.79 | 23.72 | 219.79 | 0.5848 | -809.2 | -732.7 | |
| 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. | |