SDO HMI 2014-07-02 22:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.17 | 0.00 | 9.67 | -12.95 | 254.64 | -40.72 | 112.53 | 0.6892 | 409.0 | 219.6 | |
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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 | 1.36 | 0.00 | 0.87 | -11.81 | 259.35 | -36.01 | 113.19 | 0.6284 | 86.0 | 87.7 | |
| 0.00 | 0.73 | 0.00 | 0.47 | -12.62 | 257.81 | -37.55 | 113.56 | 0.6511 | 697.0 | 460.6 | |
| 0.00 | 0.91 | 0.00 | 0.59 | -12.91 | 257.60 | -37.76 | 113.87 | 0.6550 | 718.0 | 590.0 | |
| 0.00 | 1.00 | 0.00 | 0.65 | -12.60 | 257.62 | -37.74 | 113.42 | 0.6533 | 825.0 | 628.1 | |
| 0.00 | 0.91 | 0.00 | 0.59 | -12.72 | 257.52 | -37.85 | 113.56 | 0.6552 | 728.0 | 625.2 | |
| 0.00 | 0.73 | 0.00 | 0.49 | -13.20 | 255.49 | -39.87 | 113.23 | 0.6814 | 619.0 | 573.8 | |
| 0.00 | 1.45 | 0.00 | 0.98 | -11.85 | 255.26 | -40.11 | 111.23 | 0.6787 | 729.0 | 556.1 | |
| 0.00 | 0.45 | 0.00 | 0.31 | -12.49 | 255.06 | -40.31 | 112.04 | 0.6836 | 654.0 | 548.6 | |
| 0.00 | 0.73 | 0.00 | 0.49 | -13.00 | 254.92 | -40.45 | 112.68 | 0.6874 | 533.0 | 421.4 | |
| 0.00 | 1.54 | 0.00 | 1.05 | -12.98 | 254.59 | -40.77 | 112.50 | 0.6911 | 384.0 | 316.4 | |
| 0.00 | 1.27 | 0.00 | 0.86 | -11.41 | 254.35 | -41.01 | 110.22 | 0.6878 | 365.0 | 329.5 | |
| 0.00 | 1.18 | 0.00 | 0.89 | -14.85 | 249.55 | -45.81 | 112.84 | 0.7543 | -385.0 | -352.2 | |
| 0.00 | 1.91 | 0.00 | 1.43 | -14.51 | 249.47 | -45.89 | 112.36 | 0.7540 | -636.0 | -561.8 | |
| 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. | |