SDO HMI 2014-10-30 00:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.30 | 35.20 | 7.16 | 17.71 | -3.96 | 158.79 | -3.39 | 161.59 | 0.1687 | 630.8 | 447.5 | |
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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 |
| 14.30 | 17.68 | 7.16 | 8.85 | -3.62 | 161.03 | -1.15 | 172.03 | 0.1452 | 1202.7 | 825.7 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -2.00 | 159.72 | -2.46 | 159.57 | 0.1233 | 875.0 | 670.7 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -4.22 | 159.51 | -2.67 | 163.13 | 0.1611 | 810.0 | 600.8 | |
| 0.00 | 1.56 | 0.00 | 0.79 | -5.16 | 159.38 | -2.80 | 164.00 | 0.1772 | 892.0 | 702.3 | |
| 0.00 | 5.29 | 0.00 | 2.66 | -4.77 | 159.36 | -2.83 | 163.21 | 0.1709 | 878.0 | 707.2 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -4.83 | 158.91 | -3.28 | 160.84 | 0.1743 | 952.0 | 776.4 | |
| 0.00 | 1.73 | 0.00 | 0.87 | -1.29 | 157.91 | -4.27 | 144.00 | 0.1274 | 789.0 | 501.4 | |
| 0.00 | 1.91 | 0.00 | 0.96 | -4.50 | 157.56 | -4.62 | 153.08 | 0.1782 | 976.0 | 762.7 | |
| 0.00 | 0.87 | 0.00 | 0.44 | -1.89 | 149.13 | -13.05 | 116.23 | 0.2528 | -786.0 | -625.8 | |
| 0.00 | 0.87 | 0.00 | 0.45 | -7.46 | 148.31 | -13.88 | 131.01 | 0.3165 | -907.0 | -695.6 | |
| 0.00 | 0.78 | 0.00 | 0.40 | -5.37 | 148.27 | -13.91 | 125.54 | 0.2954 | -786.0 | -620.2 | |
| 0.00 | 1.39 | 0.00 | 0.72 | -5.16 | 148.25 | -13.93 | 124.90 | 0.2937 | -849.0 | -703.1 | |
| 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. | |