SDO HMI 2014-11-03 19:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.74 | 35.69 | 6.24 | 19.05 | -17.11 | 98.70 | -0.32 | 179.68 | 0.3733 | -12.6 | -84.7 | |
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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 |
| 3.02 | 14.52 | 1.61 | 7.71 | -16.46 | 103.98 | 4.97 | 193.31 | 0.3626 | 1060.3 | 781.7 | |
| 2.33 | -1.00 | 1.24 | -1.00 | -16.36 | 103.83 | 4.82 | 192.97 | 0.3605 | 1189.7 | 999999 | |
| 3.54 | -1.00 | 1.88 | -1.00 | -16.52 | 103.80 | 4.79 | 192.80 | 0.3629 | 948.2 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -16.57 | 101.00 | 1.99 | 185.39 | 0.3564 | 742.0 | 530.5 | |
| 2.85 | 5.70 | 1.51 | 3.03 | -16.85 | 100.39 | 1.37 | 183.67 | 0.3603 | 1131.1 | 785.3 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -17.33 | 94.50 | -4.51 | 168.39 | 0.3749 | -882.0 | -711.5 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -17.69 | 94.11 | -4.90 | 167.64 | 0.3818 | -741.0 | -613.9 | |
| 0.00 | 3.63 | 0.00 | 1.95 | -18.20 | 93.78 | -5.23 | 167.16 | 0.3911 | -738.0 | -657.8 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -17.50 | 93.62 | -5.39 | 166.32 | 0.3806 | -851.0 | -722.9 | |
| 0.00 | 1.56 | 0.00 | 0.84 | -18.11 | 93.32 | -5.70 | 165.99 | 0.3914 | -812.0 | -640.2 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -14.02 | 93.28 | -5.73 | 162.71 | 0.3273 | -734.0 | -606.3 | |
| 0.00 | 0.69 | 0.00 | 0.37 | -16.36 | 91.66 | -7.35 | 160.64 | 0.3721 | -1052.0 | -758.1 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -19.71 | 91.32 | -7.69 | 162.66 | 0.4245 | -829.0 | -713.6 | |
| 0.00 | 1.73 | 0.00 | 0.95 | -20.76 | 90.98 | -8.04 | 162.72 | 0.4418 | -401.0 | -495.9 | |
| 0.00 | 1.73 | 0.00 | 0.92 | -16.24 | 90.82 | -8.19 | 158.50 | 0.3750 | -592.0 | -443.4 | |
| 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. | |