SDO HMI 2014-11-14 20:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.15 | 28.71 | 8.34 | 23.02 | 8.60 | 5.30 | 51.87 | 278.68 | 0.7887 | -171.0 | -39.2 | |
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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 |
| 4.30 | 17.19 | 3.54 | 14.14 | 8.02 | 6.51 | 53.08 | 277.85 | 0.8014 | -630.7 | -465.5 | |
| 3.01 | -1.00 | 2.48 | -1.00 | 8.25 | 6.56 | 53.13 | 278.14 | 0.8020 | -483.4 | 999999 | |
| 2.84 | -1.00 | 2.32 | -1.00 | 8.27 | 6.26 | 52.83 | 278.17 | 0.7989 | -778.8 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.63 | 7.82 | 6.12 | 52.70 | 277.62 | 0.7973 | -499.0 | -451.8 | |
| 0.00 | 0.69 | 0.00 | 0.56 | 7.47 | 5.96 | 52.53 | 277.19 | 0.7955 | -535.0 | -457.6 | |
| 0.00 | 0.69 | 0.00 | 0.56 | 8.37 | 5.83 | 52.40 | 278.33 | 0.7945 | -511.0 | -440.6 | |
| 0.00 | 1.03 | 0.00 | 0.83 | 8.44 | 5.55 | 52.12 | 278.44 | 0.7916 | -598.0 | -511.2 | |
| 0.00 | 0.52 | 0.00 | 0.40 | 8.35 | 4.23 | 50.80 | 278.40 | 0.7773 | 470.0 | 411.5 | |
| 0.00 | 1.20 | 0.00 | 0.91 | 10.24 | 2.58 | 49.15 | 281.01 | 0.7607 | 608.0 | 607.6 | |
| 0.00 | 2.06 | 0.00 | 1.57 | 10.86 | 2.72 | 49.29 | 281.82 | 0.7629 | 565.0 | 444.0 | |
| 0.00 | 0.60 | 0.00 | 0.45 | 8.46 | 2.15 | 48.72 | 278.70 | 0.7543 | 407.0 | 439.6 | |
| 0.00 | 1.81 | 0.00 | 1.35 | 8.52 | 1.97 | 48.55 | 278.81 | 0.7524 | 720.0 | 597.1 | |
| 0.00 | 1.38 | 0.00 | 1.04 | 10.43 | 2.34 | 48.91 | 281.29 | 0.7582 | 742.0 | 601.1 | |
| 0.00 | 0.77 | 0.00 | 0.58 | 10.08 | 2.13 | 48.70 | 280.85 | 0.7555 | 563.0 | 484.6 | |
| 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. | |