SDO HMI 2014-08-09 11:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.88 | 26.99 | 2.11 | 14.84 | -19.10 | 160.77 | 2.06 | 184.52 | 0.4328 | 752.0 | 642.4 | |
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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 | 0.65 | -18.84 | 164.33 | 5.62 | 192.31 | 0.4365 | 711.0 | 571.9 | |
| 0.00 | 2.98 | 0.00 | 1.64 | -19.09 | 163.12 | 4.40 | 189.60 | 0.4368 | 516.0 | 590.5 | |
| 0.90 | 4.16 | 0.50 | 2.29 | -19.75 | 160.96 | 2.25 | 184.81 | 0.4428 | 782.4 | 725.9 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -19.31 | 160.70 | 1.99 | 184.33 | 0.4356 | 885.0 | 737.3 | |
| 0.00 | 0.72 | 0.00 | 0.40 | -20.19 | 160.52 | 1.80 | 183.78 | 0.4492 | 705.0 | 635.4 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -19.75 | 160.51 | 1.80 | 183.84 | 0.4423 | 768.0 | 620.7 | |
| 0.00 | 1.63 | 0.00 | 0.90 | -19.48 | 160.48 | 1.76 | 183.81 | 0.4380 | 837.0 | 702.6 | |
| 2.98 | 5.51 | 1.61 | 2.98 | -17.14 | 160.39 | 1.68 | 184.02 | 0.4007 | 1111.1 | 825.9 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -19.58 | 160.22 | 1.51 | 183.24 | 0.4393 | 737.0 | 566.9 | |
| 0.00 | 1.26 | 0.00 | 0.69 | -19.24 | 160.18 | 1.47 | 183.21 | 0.4340 | 788.0 | 602.1 | |
| 0.00 | 1.99 | 0.00 | 1.10 | -20.32 | 159.93 | 1.22 | 182.55 | 0.4508 | 681.0 | 548.0 | |
| 0.00 | 0.36 | 0.00 | 0.20 | -20.97 | 159.81 | 1.09 | 182.23 | 0.4608 | 434.0 | 567.0 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -21.38 | 159.62 | 0.90 | 181.80 | 0.4671 | 649.0 | 532.3 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -20.46 | 159.55 | 0.83 | 181.73 | 0.4526 | 648.0 | 517.2 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -20.08 | 159.35 | 0.64 | 181.34 | 0.4467 | 831.0 | 582.9 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -16.83 | 159.12 | 0.41 | 180.99 | 0.3949 | 715.0 | 579.2 | |
| 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. | |