SDO HMI 2014-08-19 07:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.63 | 115.89 | 27.86 | 112.47 | -9.46 | 331.49 | -57.22 | 105.30 | 0.8616 | 598.6 | 208.6 | |
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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 | 0.54 | 0.00 | 0.43 | -10.14 | 339.47 | -49.24 | 108.62 | 0.7891 | 535.0 | 467.8 | |
| 0.00 | 0.99 | 0.00 | 0.84 | -10.14 | 337.14 | -51.58 | 107.79 | 0.8122 | 463.0 | 380.8 | |
| 0.00 | 1.80 | 0.00 | 1.51 | -9.31 | 337.27 | -51.45 | 106.85 | 0.8085 | 650.0 | 584.8 | |
| 23.23 | 103.83 | 22.46 | 100.93 | -9.48 | 331.66 | -57.05 | 105.36 | 0.8604 | 766.0 | 192.8 | |
| 0.00 | 0.90 | 0.00 | 0.85 | -6.74 | 331.94 | -56.78 | 102.30 | 0.8524 | 425.0 | 396.1 | |
| 0.00 | 0.81 | 0.00 | 0.76 | -6.55 | 331.97 | -56.74 | 102.09 | 0.8517 | 549.0 | 490.8 | |
| 0.00 | 1.35 | 0.00 | 1.37 | -11.32 | 330.36 | -58.35 | 107.05 | 0.8751 | 396.0 | 347.5 | |
| 4.05 | -4.00 | 4.03 | -4.00 | -9.37 | 330.59 | -58.12 | 104.95 | 0.8692 | 549.0 | 999999 | |
| 0.00 | 1.80 | 0.00 | 1.79 | -9.12 | 330.66 | -58.05 | 104.68 | 0.8681 | 383.0 | 426.5 | |
| 0.00 | 1.98 | 0.00 | 1.97 | -9.04 | 330.45 | -58.27 | 104.54 | 0.8697 | 522.0 | 409.5 | |
| 1.35 | -4.00 | 1.37 | -4.00 | -9.46 | 330.04 | -58.68 | 104.90 | 0.8739 | 213.6 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.29 | -11.08 | 328.99 | -59.73 | 106.41 | 0.8855 | -227.0 | -254.3 | |
| 0.00 | 1.35 | 0.00 | 1.45 | -10.93 | 328.60 | -60.11 | 106.15 | 0.8881 | -476.0 | -421.7 | |
| 0.00 | 0.27 | 0.00 | 0.28 | -8.73 | 329.21 | -59.51 | 103.88 | 0.8792 | 331.0 | 302.7 | |
| 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. | |