SDO HMI 2014-08-19 12:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.88 | 107.84 | 18.88 | 97.01 | -9.51 | 331.67 | -54.30 | 106.18 | 0.8360 | 526.3 | 251.6 | |
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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 | 0.90 | 0.00 | 0.72 | -10.45 | 337.24 | -48.73 | 109.18 | 0.7848 | 457.0 | 455.7 | |
| 0.00 | 0.81 | 0.00 | 0.64 | -8.92 | 337.45 | -48.52 | 107.38 | 0.7778 | 667.0 | 549.2 | |
| 0.00 | 1.35 | 0.00 | 1.06 | -9.34 | 337.33 | -48.65 | 107.85 | 0.7804 | 649.0 | 523.1 | |
| 14.85 | 86.24 | 13.30 | 77.40 | -9.52 | 331.78 | -54.19 | 106.22 | 0.8351 | 740.6 | 238.1 | |
| 0.00 | 1.62 | 0.00 | 1.42 | -6.64 | 331.83 | -54.14 | 102.87 | 0.8279 | 485.0 | 427.0 | |
| 0.00 | 1.35 | 0.00 | 1.27 | -11.27 | 330.34 | -55.63 | 107.79 | 0.8522 | 377.0 | 290.3 | |
| 5.67 | 10.53 | 5.24 | 9.72 | -9.36 | 330.53 | -55.44 | 105.67 | 0.8461 | 548.5 | 406.9 | |
| 0.00 | 1.62 | 0.00 | 1.51 | -9.08 | 330.21 | -55.76 | 105.25 | 0.8482 | 560.0 | 461.6 | |
| 0.36 | 1.53 | 0.34 | 1.43 | -9.44 | 330.01 | -55.96 | 105.62 | 0.8508 | 291.5 | 224.3 | |
| 0.00 | 0.81 | 0.00 | 0.78 | -11.25 | 329.28 | -56.69 | 107.45 | 0.8612 | -278.0 | -251.0 | |
| 0.00 | 0.27 | 0.00 | 0.26 | -11.11 | 329.04 | -56.93 | 107.23 | 0.8629 | -336.0 | -274.0 | |
| 0.00 | 0.81 | 0.00 | 0.80 | -11.04 | 328.55 | -57.42 | 107.00 | 0.8669 | -497.0 | -386.1 | |
| 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. | |