SDO HMI 2014-08-08 15:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.93 | 0.00 | 11.68 | -19.15 | 160.79 | -8.94 | 161.34 | 0.4560 | 621.2 | 518.5 | |
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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 | 1.35 | 0.00 | 0.74 | -18.05 | 168.63 | -1.10 | 177.47 | 0.4139 | 401.0 | 399.4 | |
| 0.00 | 2.17 | 0.00 | 1.18 | -17.23 | 164.82 | -4.92 | 168.39 | 0.4084 | 914.0 | 578.3 | |
| 0.00 | 1.72 | 0.00 | 0.95 | -20.04 | 163.17 | -6.56 | 166.36 | 0.4571 | 390.0 | 329.8 | |
| 0.00 | 1.81 | 0.00 | 0.99 | -17.52 | 160.57 | -9.16 | 159.31 | 0.4315 | 907.0 | 710.8 | |
| 0.00 | 1.17 | 0.00 | 0.67 | -21.24 | 160.12 | -9.61 | 161.32 | 0.4880 | 711.0 | 554.0 | |
| 0.00 | 3.07 | 0.00 | 1.72 | -19.78 | 160.11 | -9.62 | 160.24 | 0.4669 | 737.0 | 542.1 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -20.53 | 159.73 | -10.00 | 160.11 | 0.4797 | 576.0 | 526.0 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -17.44 | 159.80 | -9.93 | 157.65 | 0.4347 | 953.0 | 788.1 | |
| 0.00 | 1.26 | 0.00 | 0.72 | -20.84 | 159.58 | -10.15 | 160.06 | 0.4849 | 808.0 | 614.5 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -17.31 | 159.61 | -10.12 | 157.16 | 0.4340 | 892.0 | 708.3 | |
| 0.00 | 1.63 | 0.00 | 0.89 | -17.11 | 159.56 | -10.17 | 156.86 | 0.4315 | 884.0 | 734.6 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -21.26 | 159.02 | -10.71 | 159.39 | 0.4939 | 612.0 | 496.9 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -19.37 | 158.33 | -11.40 | 156.60 | 0.4712 | 489.0 | 437.2 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -20.65 | 157.51 | -12.22 | 156.25 | 0.4939 | 704.0 | 435.7 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -21.89 | 154.53 | -15.20 | 152.55 | 0.5298 | -660.0 | -468.3 | |
| 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. | |