SDO HMI 2014-07-18 10:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.62 | 72.10 | 8.33 | 38.54 | 6.80 | 112.35 | 22.09 | 276.67 | 0.3775 | -44.7 | 102.5 | |
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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 |
| 3.18 | 11.53 | 1.72 | 6.24 | 7.21 | 114.04 | 23.78 | 277.38 | 0.4051 | -1050.5 | -751.9 | |
| 0.00 | 2.91 | 0.00 | 1.57 | 6.85 | 113.82 | 23.56 | 276.53 | 0.4012 | -934.0 | -747.5 | |
| 0.00 | 1.82 | 0.00 | 0.98 | 6.92 | 113.62 | 23.37 | 276.74 | 0.3981 | -903.0 | -678.9 | |
| 0.00 | 3.18 | 0.00 | 1.72 | 7.17 | 113.63 | 23.38 | 277.35 | 0.3986 | -886.0 | -688.7 | |
| 0.00 | 0.64 | 0.00 | 0.34 | 7.02 | 113.52 | 23.27 | 276.99 | 0.3967 | -751.0 | -630.9 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 6.93 | 113.35 | 23.10 | 276.81 | 0.3939 | -825.0 | -644.8 | |
| 0.00 | 2.91 | 0.00 | 1.56 | 6.75 | 113.14 | 22.89 | 276.40 | 0.3903 | -721.0 | -592.4 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 6.52 | 112.80 | 22.54 | 275.86 | 0.3845 | -897.0 | -749.6 | |
| 0.00 | 3.09 | 0.00 | 1.66 | 7.59 | 112.69 | 22.43 | 278.67 | 0.3843 | -947.0 | -822.2 | |
| 7.17 | 40.67 | 3.82 | 21.61 | 6.55 | 111.74 | 21.49 | 276.13 | 0.3675 | 954.0 | 775.9 | |
| 3.00 | -10.00 | 1.59 | -10.00 | 6.75 | 111.29 | 21.03 | 276.77 | 0.3605 | 1126.8 | 999999 | |
| 2.27 | -10.00 | 1.20 | -10.00 | 6.60 | 111.25 | 20.99 | 276.35 | 0.3596 | 1173.7 | 999999 | |
| 0.00 | 2.81 | 0.00 | 1.49 | 6.61 | 110.89 | 20.63 | 276.46 | 0.3538 | 1051.0 | 902.1 | |
| 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. | |