SDO HMI 2014-11-01 07:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.05 | 25.73 | 4.93 | 16.20 | -16.69 | 99.96 | -32.01 | 124.62 | 0.6168 | 77.0 | 164.8 | |
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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 | 1.04 | 0.00 | 0.63 | -16.99 | 104.10 | -27.87 | 128.51 | 0.5735 | -685.0 | -538.8 | |
| 0.00 | 0.87 | 0.00 | 0.53 | -16.45 | 102.38 | -29.59 | 126.14 | 0.5886 | 491.0 | 472.8 | |
| 2.77 | 8.23 | 1.69 | 5.02 | -16.17 | 102.40 | -29.57 | 125.74 | 0.5863 | 992.5 | 799.8 | |
| 5.28 | 8.05 | 3.24 | 4.93 | -16.15 | 102.01 | -29.96 | 125.38 | 0.5906 | 811.1 | 568.5 | |
| 0.00 | 1.56 | 0.00 | 0.98 | -15.70 | 99.73 | -32.24 | 122.87 | 0.6137 | 654.0 | 494.2 | |
| 0.00 | 1.21 | 0.00 | 0.78 | -15.79 | 96.96 | -35.01 | 120.97 | 0.6462 | -699.0 | -487.6 | |
| 0.00 | 1.21 | 0.00 | 0.84 | -18.74 | 93.90 | -38.07 | 122.85 | 0.6975 | -525.0 | -390.9 | |
| 0.00 | 1.04 | 0.00 | 0.70 | -17.02 | 94.29 | -37.68 | 120.88 | 0.6833 | -631.0 | -519.4 | |
| 0.00 | 1.13 | 0.00 | 0.80 | -19.84 | 92.04 | -39.93 | 123.07 | 0.7229 | -670.0 | -592.5 | |
| 0.00 | 1.13 | 0.00 | 0.81 | -19.60 | 91.57 | -40.40 | 122.50 | 0.7263 | -730.0 | -640.3 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -16.73 | 91.76 | -40.21 | 119.00 | 0.7093 | -438.0 | -512.7 | |
| 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. | |