SDO HMI 2014-09-07 04:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.25 | 34.82 | 13.64 | 88.12 | -16.56 | 63.54 | -75.80 | 108.60 | 0.9806 | 144.1 | -26.0 | |
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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 |
| 0.00 | 0.54 | 0.00 | 1.11 | -16.84 | 66.34 | -73.01 | 109.42 | 0.9716 | 433.0 | 460.8 | |
| 2.32 | 11.25 | 4.99 | 24.71 | -16.88 | 65.74 | -73.61 | 109.34 | 0.9739 | 467.5 | 50.5 | |
| 1.70 | 9.02 | 3.63 | 19.71 | -16.54 | 65.64 | -73.71 | 108.98 | 0.9740 | 543.8 | 254.0 | |
| 2.23 | -3.00 | 5.02 | -3.00 | -16.72 | 64.98 | -74.36 | 109.02 | 0.9765 | -58.6 | 999999 | |
| 0.00 | 1.87 | 0.00 | 4.61 | -17.02 | 63.90 | -75.45 | 109.11 | 0.9804 | -122.0 | -178.1 | |
| 0.00 | 2.50 | 0.00 | 6.62 | -16.68 | 63.00 | -76.35 | 108.60 | 0.9830 | -318.0 | -319.8 | |
| 0.00 | 0.71 | 0.00 | 1.78 | -15.75 | 63.44 | -75.91 | 107.76 | 0.9811 | -159.0 | -92.6 | |
| 0.00 | 1.79 | 0.00 | 5.54 | -16.62 | 61.18 | -78.17 | 108.21 | 0.9880 | -384.0 | -364.2 | |
| 0.00 | 1.34 | 0.00 | 4.02 | -16.03 | 61.55 | -77.80 | 107.68 | 0.9868 | -473.0 | -481.9 | |
| 0.00 | 2.14 | 0.00 | 7.27 | -16.27 | 60.40 | -78.95 | 107.72 | 0.9898 | -5.0 | 23.3 | |
| 0.00 | 3.66 | 0.00 | 12.75 | -15.96 | 60.02 | -79.33 | 107.36 | 0.9905 | 135.0 | 49.7 | |
| 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. | |