SDO HMI 2014-10-01 02:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.23 | 0.00 | 13.00 | -4.69 | 139.10 | -44.53 | 103.24 | 0.7203 | -598.3 | -515.9 | |
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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 | 1.32 | 0.00 | 0.91 | -4.01 | 141.07 | -42.56 | 102.99 | 0.6947 | -666.0 | -479.1 | |
| 0.00 | 1.32 | 0.00 | 0.93 | -4.59 | 139.61 | -44.01 | 103.29 | 0.7140 | -316.0 | -385.9 | |
| 0.00 | 1.76 | 0.00 | 1.25 | -4.85 | 139.38 | -44.24 | 103.57 | 0.7175 | -836.0 | -781.0 | |
| 0.00 | 1.23 | 0.00 | 0.87 | -3.41 | 139.44 | -44.18 | 101.62 | 0.7126 | -555.0 | -540.9 | |
| 0.00 | 2.47 | 0.00 | 1.76 | -4.99 | 139.16 | -44.47 | 103.68 | 0.7206 | -790.0 | -633.5 | |
| 0.00 | 0.88 | 0.00 | 0.62 | -4.04 | 139.23 | -44.39 | 102.41 | 0.7169 | -736.0 | -578.7 | |
| 0.00 | 1.67 | 0.00 | 1.20 | -5.04 | 138.94 | -44.69 | 103.67 | 0.7232 | -459.0 | -478.7 | |
| 0.00 | 4.32 | 0.00 | 3.09 | -4.75 | 138.84 | -44.79 | 103.24 | 0.7235 | -527.0 | -440.9 | |
| 0.00 | 0.97 | 0.00 | 0.70 | -5.49 | 138.77 | -44.86 | 104.20 | 0.7266 | -629.0 | -466.0 | |
| 0.00 | 1.23 | 0.00 | 0.89 | -5.68 | 138.67 | -44.96 | 104.42 | 0.7284 | -558.0 | -462.7 | |
| 0.00 | 1.06 | 0.00 | 0.78 | -3.94 | 137.17 | -46.45 | 101.63 | 0.7406 | -509.0 | -405.8 | |
| 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. | |