SDO HMI 2014-07-10 13:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.00 | 0.00 | 8.39 | -22.38 | 201.44 | 6.97 | 194.57 | 0.4645 | 346.6 | 402.8 | |
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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 | 1.18 | 0.00 | 0.66 | -21.68 | 206.01 | 11.54 | 203.39 | 0.4703 | 579.0 | 434.9 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -21.73 | 204.84 | 10.37 | 201.22 | 0.4641 | 668.0 | 550.6 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -21.72 | 204.21 | 9.74 | 200.04 | 0.4605 | 825.0 | 672.2 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -21.99 | 203.83 | 9.36 | 199.11 | 0.4624 | 529.0 | 519.8 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -20.91 | 203.63 | 9.16 | 199.57 | 0.4456 | 648.0 | 499.4 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -21.78 | 203.55 | 9.08 | 198.74 | 0.4580 | 867.0 | 643.7 | |
| 0.00 | 4.00 | 0.00 | 2.23 | -22.02 | 203.50 | 9.03 | 198.46 | 0.4612 | 394.0 | 612.7 | |
| 0.00 | 1.18 | 0.00 | 0.66 | -22.53 | 203.36 | 8.89 | 197.84 | 0.4680 | 502.0 | 501.8 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -21.97 | 198.30 | 3.83 | 188.09 | 0.4418 | 847.0 | 669.1 | |
| 0.00 | 0.82 | 0.00 | 0.45 | -20.64 | 194.39 | -0.08 | 179.81 | 0.4164 | -592.0 | -484.1 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -24.42 | 192.47 | -2.00 | 176.17 | 0.4768 | -512.0 | -551.0 | |
| 0.00 | 0.64 | 0.00 | 0.39 | -30.85 | 184.55 | -9.92 | 165.42 | 0.5896 | -596.0 | -467.6 | |
| 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. | |