SDO HMI 2014-11-06 19:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.15 | 0.00 | 12.43 | -22.68 | 76.26 | 16.80 | 211.27 | 0.5402 | 457.7 | 365.1 | |
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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 | 1.21 | 0.00 | 0.77 | -27.05 | 84.38 | 24.92 | 216.49 | 0.6334 | -711.0 | -635.8 | |
| 0.00 | 1.38 | 0.00 | 0.81 | -19.75 | 82.65 | 23.19 | 223.20 | 0.5436 | 701.0 | 612.4 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -20.17 | 82.58 | 23.12 | 222.56 | 0.5471 | 816.0 | 696.6 | |
| 0.00 | 1.38 | 0.00 | 0.82 | -20.43 | 82.51 | 23.06 | 222.14 | 0.5491 | 738.0 | 614.9 | |
| 0.00 | 1.73 | 0.00 | 1.01 | -19.78 | 82.34 | 22.89 | 222.80 | 0.5408 | 834.0 | 651.1 | |
| 0.00 | 1.29 | 0.00 | 0.77 | -21.53 | 82.24 | 22.79 | 220.41 | 0.5580 | 632.0 | 537.0 | |
| 0.00 | 2.33 | 0.00 | 1.36 | -21.02 | 80.24 | 20.78 | 218.53 | 0.5338 | 879.0 | 766.3 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -21.38 | 80.29 | 20.84 | 218.15 | 0.5383 | 649.0 | 552.0 | |
| 0.00 | 0.86 | 0.00 | 0.50 | -21.30 | 79.80 | 20.35 | 217.61 | 0.5330 | 667.0 | 557.5 | |
| 0.00 | 0.78 | 0.00 | 0.45 | -21.51 | 78.95 | 19.49 | 216.20 | 0.5277 | 679.0 | 579.8 | |
| 0.00 | 1.47 | 0.00 | 0.84 | -20.64 | 78.02 | 18.57 | 215.97 | 0.5094 | 764.0 | 664.9 | |
| 0.00 | 1.38 | 0.00 | 0.79 | -21.29 | 76.26 | 16.81 | 212.59 | 0.5023 | 752.0 | 611.9 | |
| 0.00 | 1.90 | 0.00 | 1.05 | -18.12 | 75.05 | 15.59 | 214.55 | 0.4525 | 752.0 | 613.1 | |
| 0.00 | 2.42 | 0.00 | 1.41 | -27.96 | 58.76 | -0.69 | 178.84 | 0.5287 | -600.0 | -408.0 | |
| 0.00 | 1.21 | 0.00 | 0.78 | -36.01 | 54.64 | -4.81 | 173.95 | 0.6461 | -686.0 | -527.9 | |
| 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. | |