SDO HMI 2014-01-09 13:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.96 | 0.00 | 12.90 | -15.04 | 111.73 | 34.72 | 249.53 | 0.5894 | -250.9 | -301.2 | |
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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 |
| 0.00 | 1.10 | 0.00 | 0.77 | -15.70 | 120.97 | 43.95 | 251.62 | 0.7065 | 439.0 | 432.5 | |
| 0.00 | 0.68 | 0.00 | 0.46 | -12.01 | 119.32 | 42.31 | 256.54 | 0.6794 | 645.0 | 600.5 | |
| 0.00 | 1.53 | 0.00 | 1.02 | -12.27 | 118.85 | 41.83 | 256.07 | 0.6738 | 778.0 | 635.3 | |
| 0.00 | 0.85 | 0.00 | 0.56 | -12.36 | 118.10 | 41.08 | 255.78 | 0.6645 | 698.0 | 594.0 | |
| 0.00 | 1.61 | 0.00 | 0.99 | -14.10 | 112.34 | 35.33 | 251.44 | 0.5939 | -793.0 | -660.9 | |
| 0.00 | 1.19 | 0.00 | 0.74 | -16.05 | 112.45 | 35.44 | 248.30 | 0.6020 | -586.0 | -438.4 | |
| 0.00 | 1.10 | 0.00 | 0.67 | -16.63 | 110.04 | 33.02 | 246.24 | 0.5728 | -672.0 | -587.9 | |
| 0.00 | 2.89 | 0.00 | 1.74 | -16.67 | 109.68 | 32.66 | 245.98 | 0.5683 | -699.0 | -611.9 | |
| 0.00 | 3.65 | 0.00 | 2.20 | -17.34 | 109.73 | 32.72 | 244.90 | 0.5720 | -709.0 | -618.0 | |
| 0.00 | 1.27 | 0.00 | 0.77 | -17.13 | 109.66 | 32.64 | 245.20 | 0.5700 | -852.0 | -767.9 | |
| 0.00 | 1.19 | 0.00 | 0.71 | -16.77 | 109.33 | 32.32 | 245.62 | 0.5642 | -772.0 | -704.9 | |
| 0.00 | 1.27 | 0.00 | 0.76 | -17.09 | 108.88 | 31.87 | 244.84 | 0.5598 | -800.0 | -675.1 | |
| 0.00 | 1.44 | 0.00 | 0.84 | -13.59 | 107.27 | 30.26 | 250.20 | 0.5226 | -714.0 | -567.8 | |
| 0.00 | 1.19 | 0.00 | 0.67 | -4.92 | 105.42 | 28.40 | 266.98 | 0.4766 | 525.0 | 596.2 | |
| 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. | |