SDO HMI 2014-05-14 01:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.96 | 238.90 | 31.39 | 167.83 | -23.86 | 194.07 | -41.31 | 121.55 | 0.7103 | 579.1 | 268.9 | |
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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 | 1.44 | 0.00 | 0.97 | -26.55 | 198.35 | -37.03 | 127.38 | 0.6803 | -406.0 | -296.4 | |
| 3.32 | 227.03 | 2.30 | 158.41 | -23.85 | 195.03 | -40.35 | 121.98 | 0.7004 | 1041.4 | 320.4 | |
| 40.29 | -2.00 | 28.11 | -2.00 | -23.73 | 194.42 | -40.96 | 121.52 | 0.7064 | 959.8 | 999999 | |
| 0.99 | -2.00 | 0.69 | -2.00 | -23.39 | 193.81 | -41.58 | 120.78 | 0.7113 | 454.7 | 999999 | |
| 0.00 | 1.35 | 0.00 | 1.02 | -23.36 | 189.22 | -46.17 | 118.86 | 0.7584 | -551.0 | -455.6 | |
| 0.00 | 0.99 | 0.00 | 0.78 | -25.84 | 187.50 | -47.89 | 121.29 | 0.7836 | -706.0 | -596.2 | |
| 0.00 | 0.90 | 0.00 | 0.72 | -25.93 | 187.15 | -48.24 | 121.27 | 0.7871 | -438.0 | -396.6 | |
| 0.36 | 1.62 | 0.29 | 1.31 | -26.34 | 186.71 | -48.68 | 121.61 | 0.7925 | -647.5 | -548.6 | |
| 0.00 | 0.81 | 0.00 | 0.65 | -26.05 | 186.87 | -48.51 | 121.32 | 0.7900 | -565.0 | -513.2 | |
| 0.00 | 0.63 | 0.00 | 0.51 | -26.00 | 186.39 | -49.00 | 121.09 | 0.7943 | -495.0 | -434.1 | |
| 0.00 | 1.08 | 0.00 | 0.92 | -27.85 | 184.57 | -50.81 | 122.65 | 0.8162 | -726.0 | -559.4 | |
| 0.00 | 0.90 | 0.00 | 0.74 | -25.84 | 185.75 | -49.64 | 120.68 | 0.7996 | -542.0 | -430.2 | |
| 0.00 | 2.15 | 0.00 | 1.80 | -26.32 | 185.10 | -50.29 | 121.03 | 0.8069 | -454.0 | -372.5 | |
| 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. | |