SDO HMI 2014-08-09 01:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.11 | 0.00 | 11.59 | -18.59 | 160.19 | -4.01 | 171.05 | 0.4282 | 784.6 | 658.5 | |
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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 | 1.17 | 0.00 | 0.64 | -17.60 | 165.02 | 0.82 | 181.94 | 0.4073 | 837.0 | 710.2 | |
| 0.00 | 0.81 | 0.00 | 0.44 | -17.34 | 160.79 | -3.41 | 171.93 | 0.4067 | 707.0 | 553.8 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -20.09 | 160.69 | -3.51 | 172.64 | 0.4501 | 710.0 | 646.6 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -19.96 | 160.67 | -3.53 | 172.54 | 0.4481 | 774.0 | 599.0 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -20.16 | 160.40 | -3.80 | 172.06 | 0.4518 | 837.0 | 692.8 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -19.59 | 160.38 | -3.82 | 171.83 | 0.4429 | 781.0 | 658.2 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -21.16 | 160.21 | -3.99 | 171.99 | 0.4675 | 706.0 | 513.8 | |
| 0.00 | 1.90 | 0.00 | 1.03 | -17.35 | 159.89 | -4.31 | 169.87 | 0.4091 | 968.0 | 768.3 | |
| 0.00 | 1.26 | 0.00 | 0.70 | -20.34 | 159.71 | -4.49 | 170.71 | 0.4561 | 796.0 | 652.2 | |
| 0.00 | 1.90 | 0.00 | 1.03 | -16.98 | 159.74 | -4.46 | 169.35 | 0.4038 | 876.0 | 715.6 | |
| 0.00 | 1.35 | 0.00 | 0.76 | -21.23 | 159.55 | -4.64 | 170.72 | 0.4701 | 800.0 | 652.3 | |
| 0.00 | 5.24 | 0.00 | 2.84 | -17.28 | 159.64 | -4.56 | 169.25 | 0.4088 | 772.0 | 705.9 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -18.79 | 159.31 | -4.89 | 169.22 | 0.4332 | 683.0 | 465.3 | |
| 0.00 | 0.63 | 0.00 | 0.35 | -18.05 | 159.10 | -5.09 | 168.42 | 0.4225 | 737.0 | 528.1 | |
| 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. | |