SDO HMI 2014-11-07 15:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.59 | 25.37 | 1.44 | 13.71 | 5.80 | 71.85 | 23.37 | 276.35 | 0.3980 | -62.9 | -131.3 | |
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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 |
| 1.73 | 7.42 | 0.96 | 4.13 | 5.64 | 75.62 | 27.14 | 275.13 | 0.4577 | -937.5 | -779.5 | |
| 0.86 | 2.33 | 0.48 | 1.29 | 5.36 | 74.90 | 26.42 | 274.60 | 0.4464 | -932.2 | -760.0 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 4.09 | 74.71 | 26.24 | 271.73 | 0.4430 | -734.0 | -616.8 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 5.44 | 73.38 | 24.90 | 274.93 | 0.4225 | -695.0 | -529.6 | |
| 0.00 | 0.69 | 0.00 | 0.38 | 5.45 | 73.02 | 24.54 | 275.00 | 0.4168 | -770.0 | -694.4 | |
| 0.00 | 2.42 | 0.00 | 1.31 | 5.40 | 72.62 | 24.15 | 274.93 | 0.4105 | -831.0 | -641.0 | |
| 0.00 | 1.21 | 0.00 | 0.65 | 6.27 | 72.17 | 23.70 | 277.16 | 0.4044 | 715.0 | 581.6 | |
| 0.00 | 0.26 | 0.00 | 0.14 | 4.01 | 68.90 | 20.42 | 271.53 | 0.3498 | 11.0 | 13.3 | |
| 0.00 | 0.95 | 0.00 | 0.50 | 5.88 | 68.77 | 20.29 | 276.93 | 0.3491 | -16.0 | -5.3 | |
| 0.00 | 1.47 | 0.00 | 0.77 | 6.95 | 68.69 | 20.21 | 280.02 | 0.3498 | -7.0 | -12.4 | |
| 0.00 | 1.04 | 0.00 | 0.54 | 6.03 | 67.57 | 19.09 | 277.71 | 0.3298 | 787.0 | 564.9 | |
| 0.00 | 1.64 | 0.00 | 0.85 | 6.23 | 66.57 | 18.09 | 278.69 | 0.3137 | 987.0 | 823.2 | |
| 0.00 | 2.93 | 0.00 | 1.53 | 6.53 | 66.33 | 17.85 | 279.75 | 0.3104 | 965.0 | 830.2 | |
| 0.00 | 1.29 | 0.00 | 0.67 | 6.42 | 66.11 | 17.63 | 279.49 | 0.3065 | 960.0 | 717.4 | |
| 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. | |