SDO HMI 2014-07-08 08:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.34 | 161.99 | 16.45 | 85.22 | 6.56 | 204.24 | -19.45 | 80.66 | 0.3368 | -899.6 | -405.2 | |
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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 | 1.54 | 0.00 | 0.81 | 9.01 | 206.30 | -17.39 | 71.93 | 0.3118 | -853.0 | -680.2 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 10.87 | 205.71 | -17.98 | 66.98 | 0.3307 | -829.0 | -643.1 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 10.95 | 205.51 | -18.18 | 66.94 | 0.3343 | -742.0 | -594.0 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 4.29 | 205.66 | -18.02 | 87.33 | 0.3102 | -775.0 | -581.5 | |
| 4.63 | 7.72 | 2.42 | 4.04 | 7.15 | 205.41 | -18.27 | 78.31 | 0.3191 | -1094.7 | -814.9 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 7.63 | 204.61 | -19.07 | 77.31 | 0.3334 | -793.0 | -554.1 | |
| 26.71 | 139.10 | 14.03 | 73.05 | 6.34 | 204.44 | -19.25 | 81.22 | 0.3330 | -1395.4 | -444.9 | |
| 0.00 | 0.82 | 0.00 | 0.43 | 8.43 | 203.27 | -20.42 | 75.80 | 0.3576 | -713.0 | -513.8 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 8.57 | 202.96 | -20.73 | 75.58 | 0.3629 | -849.0 | -639.9 | |
| 0.00 | 3.00 | 0.00 | 1.62 | 7.90 | 200.20 | -23.48 | 78.62 | 0.4043 | 793.0 | 595.4 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 5.67 | 197.89 | -25.80 | 84.50 | 0.4369 | 786.0 | 634.2 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 8.02 | 197.65 | -26.03 | 79.23 | 0.4442 | 689.0 | 549.2 | |
| 0.00 | 1.73 | 0.00 | 0.96 | 8.86 | 197.01 | -26.68 | 77.60 | 0.4561 | 820.0 | 585.7 | |
| 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. | |