SDO HMI 2014-08-08 12:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.35 | 0.00 | 10.33 | -19.13 | 159.11 | -12.28 | 154.83 | 0.4733 | 649.8 | 517.5 | |
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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 | 1.72 | 0.00 | 0.95 | -17.49 | 160.57 | -10.82 | 155.95 | 0.4410 | 764.0 | 663.9 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -21.25 | 160.08 | -11.31 | 158.33 | 0.4969 | 632.0 | 507.5 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -17.54 | 160.21 | -11.18 | 155.28 | 0.4439 | 639.0 | 475.1 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -19.82 | 159.99 | -11.40 | 156.98 | 0.4774 | 884.0 | 738.4 | |
| 0.00 | 1.90 | 0.00 | 1.05 | -17.48 | 159.82 | -11.56 | 154.48 | 0.4456 | 896.0 | 744.1 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -20.89 | 159.51 | -11.88 | 157.04 | 0.4951 | 781.0 | 614.0 | |
| 0.00 | 1.99 | 0.00 | 1.10 | -17.35 | 159.64 | -11.75 | 153.99 | 0.4451 | 962.0 | 836.5 | |
| 0.00 | 1.99 | 0.00 | 1.13 | -20.79 | 159.28 | -12.11 | 156.57 | 0.4951 | 644.0 | 516.8 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -17.05 | 159.46 | -11.93 | 153.34 | 0.4422 | 953.0 | 755.9 | |
| 0.00 | 2.08 | 0.00 | 1.16 | -18.09 | 159.23 | -12.16 | 153.97 | 0.4582 | 727.0 | 552.9 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -21.27 | 158.97 | -12.41 | 156.47 | 0.5037 | 683.0 | 514.4 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -20.55 | 157.77 | -13.62 | 153.81 | 0.5015 | 623.0 | 463.3 | |
| 0.00 | 1.63 | 0.00 | 0.96 | -21.85 | 154.59 | -16.80 | 150.11 | 0.5405 | -740.0 | -634.3 | |
| 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. | |