SDO HMI 2014-07-07 23:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.70 | 0.00 | 8.82 | -13.66 | 258.37 | 29.74 | 238.96 | 0.5646 | 445.5 | 456.4 | |
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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 | 1.09 | 0.00 | 0.66 | -12.97 | 260.12 | 31.49 | 241.52 | 0.5812 | 598.0 | 473.8 | |
| 0.00 | 2.36 | 0.00 | 1.44 | -13.96 | 260.15 | 31.52 | 240.03 | 0.5879 | 705.0 | 546.4 | |
| 0.00 | 1.27 | 0.00 | 0.78 | -13.73 | 260.08 | 31.45 | 240.32 | 0.5856 | 696.0 | 520.2 | |
| 0.00 | 1.00 | 0.00 | 0.61 | -13.38 | 259.92 | 31.29 | 240.74 | 0.5813 | 650.0 | 507.5 | |
| 0.00 | 1.63 | 0.00 | 0.98 | -13.10 | 259.22 | 30.59 | 240.65 | 0.5708 | 783.0 | 561.3 | |
| 0.00 | 1.36 | 0.00 | 0.82 | -12.52 | 259.03 | 30.40 | 241.42 | 0.5648 | 724.0 | 618.6 | |
| 0.00 | 1.36 | 0.00 | 0.81 | -12.45 | 258.84 | 30.21 | 241.38 | 0.5619 | 748.0 | 600.7 | |
| 0.00 | 1.00 | 0.00 | 0.60 | -13.17 | 258.58 | 29.95 | 240.03 | 0.5632 | 490.0 | 435.2 | |
| 0.00 | 1.09 | 0.00 | 0.65 | -14.94 | 256.91 | 28.28 | 235.84 | 0.5554 | 792.0 | 699.4 | |
| 0.00 | 0.36 | 0.00 | 0.21 | -14.68 | 255.91 | 27.28 | 235.32 | 0.5413 | 538.0 | 585.5 | |
| 0.00 | 0.91 | 0.00 | 0.52 | -14.81 | 253.79 | 25.15 | 232.97 | 0.5168 | 575.0 | 522.9 | |
| 0.00 | 0.27 | 0.00 | 0.16 | -15.30 | 253.01 | 24.38 | 231.34 | 0.5119 | -790.0 | -688.0 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -15.43 | 252.96 | 24.33 | 231.08 | 0.5124 | -718.0 | -590.8 | |
| 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. | |