SDO HMI 2014-11-08 06:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.35 | 19.07 | 0.21 | 11.17 | 5.20 | 72.29 | 32.07 | 274.10 | 0.5313 | -90.8 | -274.9 | |
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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 | 4.49 | 0.00 | 2.73 | 5.49 | 75.84 | 35.63 | 274.37 | 0.5838 | -811.0 | -672.4 | |
| 0.00 | 0.86 | 0.00 | 0.52 | 4.12 | 75.03 | 34.81 | 272.00 | 0.5720 | -602.0 | -492.8 | |
| 0.35 | 1.55 | 0.21 | 0.94 | 5.29 | 74.95 | 34.74 | 274.05 | 0.5710 | -797.8 | -679.6 | |
| 0.00 | 1.04 | 0.00 | 0.61 | 4.11 | 73.77 | 33.55 | 271.96 | 0.5537 | -724.0 | -626.8 | |
| 0.00 | 1.90 | 0.00 | 1.13 | 4.95 | 73.63 | 33.42 | 273.49 | 0.5518 | -915.0 | -783.3 | |
| 0.00 | 1.55 | 0.00 | 0.92 | 4.87 | 73.34 | 33.13 | 273.35 | 0.5476 | -944.0 | -556.8 | |
| 0.00 | 0.78 | 0.00 | 0.45 | 5.83 | 71.46 | 31.24 | 275.26 | 0.5202 | 725.0 | 611.3 | |
| 0.00 | 1.98 | 0.00 | 1.14 | 4.39 | 70.96 | 30.74 | 272.48 | 0.5122 | -762.0 | -610.2 | |
| 0.00 | 0.78 | 0.00 | 0.43 | 5.57 | 67.47 | 27.25 | 275.11 | 0.4594 | 640.0 | 512.2 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 5.52 | 66.93 | 26.71 | 275.08 | 0.4511 | 650.0 | 573.3 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 5.65 | 66.67 | 26.45 | 275.39 | 0.4471 | 917.0 | 716.2 | |
| 0.00 | 1.29 | 0.00 | 0.72 | 6.19 | 66.60 | 26.38 | 276.61 | 0.4465 | 833.0 | 732.1 | |
| 0.00 | 0.78 | 0.00 | 0.43 | 5.90 | 66.11 | 25.90 | 276.04 | 0.4387 | 759.0 | 666.7 | |
| 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. | |