SDO HMI 2014-11-07 01:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.24 | 18.14 | 1.56 | 12.37 | -15.94 | 17.02 | -39.12 | 118.08 | 0.6888 | -202.5 | -374.9 | |
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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 | 0.78 | 0.00 | 0.46 | -11.46 | 27.14 | -29.00 | 118.19 | 0.5412 | 701.0 | 491.4 | |
| 0.00 | 0.69 | 0.00 | 0.42 | -13.54 | 23.92 | -32.22 | 119.05 | 0.5952 | 790.0 | 630.5 | |
| 0.00 | 0.60 | 0.00 | 0.37 | -13.80 | 23.77 | -32.37 | 119.32 | 0.5986 | 555.0 | 558.3 | |
| 0.00 | 1.04 | 0.00 | 0.69 | -14.74 | 17.91 | -38.23 | 116.93 | 0.6735 | 814.0 | 641.7 | |
| 0.00 | 1.12 | 0.00 | 0.77 | -16.11 | 16.57 | -39.57 | 118.02 | 0.6957 | -463.0 | -403.5 | |
| 0.00 | 1.21 | 0.00 | 0.84 | -16.25 | 16.25 | -39.89 | 118.03 | 0.6999 | -677.0 | -587.1 | |
| 0.00 | 4.32 | 0.00 | 3.00 | -16.51 | 16.11 | -40.03 | 118.29 | 0.7027 | -766.0 | -667.0 | |
| 0.00 | 1.04 | 0.00 | 0.72 | -16.71 | 15.89 | -40.25 | 118.44 | 0.7061 | -552.0 | -465.0 | |
| 2.24 | 4.92 | 1.56 | 3.41 | -16.11 | 16.01 | -40.14 | 117.71 | 0.7019 | -954.4 | -715.1 | |
| 0.00 | 1.90 | 0.00 | 1.32 | -16.18 | 15.66 | -40.48 | 117.62 | 0.7060 | -731.0 | -437.8 | |
| 0.00 | 0.52 | 0.00 | 0.37 | -18.87 | 14.58 | -41.56 | 120.47 | 0.7307 | -523.0 | -430.8 | |
| 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. | |