SDO HMI 2014-07-05 10:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.45 | 19.89 | 1.30 | 10.40 | -13.81 | 256.00 | -6.30 | 160.85 | 0.3174 | 613.7 | 483.3 | |
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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 | 1.91 | 0.00 | 0.98 | -12.65 | 259.75 | -2.55 | 171.04 | 0.2799 | 905.0 | 747.5 | |
| 0.00 | 2.27 | 0.00 | 1.17 | -12.71 | 259.31 | -2.99 | 169.57 | 0.2822 | 868.0 | 678.2 | |
| 0.00 | 1.82 | 0.00 | 0.94 | -13.76 | 259.26 | -3.03 | 170.08 | 0.2997 | 738.0 | 608.2 | |
| 0.00 | 1.54 | 0.00 | 0.81 | -14.25 | 257.52 | -4.77 | 165.04 | 0.3138 | 878.0 | 807.2 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -12.75 | 257.43 | -4.87 | 163.35 | 0.2902 | 916.0 | 682.5 | |
| 0.00 | 1.18 | 0.00 | 0.62 | -14.15 | 257.37 | -4.93 | 164.49 | 0.3130 | 639.0 | 614.1 | |
| 0.00 | 2.09 | 0.00 | 1.09 | -13.33 | 256.88 | -5.41 | 162.22 | 0.3021 | 867.0 | 616.6 | |
| 0.00 | 1.00 | 0.00 | 0.52 | -13.59 | 254.48 | -7.82 | 155.53 | 0.3207 | 687.0 | 562.8 | |
| 0.00 | 1.09 | 0.00 | 0.57 | -13.70 | 253.33 | -8.97 | 152.61 | 0.3305 | 928.0 | 697.8 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -14.76 | 252.97 | -9.33 | 153.16 | 0.3487 | 743.0 | 555.2 | |
| 2.45 | 4.63 | 1.30 | 2.46 | -14.93 | 251.71 | -10.59 | 150.39 | 0.3609 | -949.6 | -751.8 | |
| 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. | |