SDO HMI 2014-04-07 17:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.94 | 0.00 | 9.75 | -20.15 | 321.64 | -33.80 | 116.33 | 0.5815 | -192.5 | -137.7 | |
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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 |
| 0.00 | 1.06 | 0.00 | 0.56 | -13.51 | 334.23 | -21.21 | 111.01 | 0.3784 | 829.0 | 602.8 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -18.09 | 329.39 | -26.05 | 117.50 | 0.4725 | 863.0 | 812.5 | |
| 0.00 | 2.82 | 0.00 | 1.60 | -17.21 | 327.67 | -27.78 | 114.58 | 0.4915 | 690.0 | 542.0 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -18.87 | 327.05 | -28.39 | 117.32 | 0.5084 | 724.0 | 644.4 | |
| 0.00 | 1.41 | 0.00 | 0.88 | -20.94 | 320.02 | -35.42 | 116.83 | 0.6088 | -605.0 | -561.4 | |
| 0.00 | 1.41 | 0.00 | 0.88 | -21.14 | 319.65 | -35.79 | 116.96 | 0.6142 | -621.0 | -470.1 | |
| 0.00 | 1.23 | 0.00 | 0.77 | -21.09 | 319.46 | -35.98 | 116.80 | 0.6163 | -593.0 | -496.9 | |
| 0.00 | 1.67 | 0.00 | 1.04 | -18.65 | 319.24 | -36.20 | 112.87 | 0.6095 | -785.0 | -610.9 | |
| 0.00 | 1.41 | 0.00 | 0.92 | -22.28 | 316.44 | -39.00 | 117.26 | 0.6573 | -703.0 | -571.4 | |
| 0.00 | 0.53 | 0.00 | 0.35 | -23.02 | 316.15 | -39.29 | 118.20 | 0.6636 | -737.0 | -623.5 | |
| 0.00 | 1.06 | 0.00 | 0.70 | -23.63 | 315.76 | -39.68 | 118.91 | 0.6705 | -629.0 | -533.7 | |
| 0.00 | 0.62 | 0.00 | 0.41 | -23.08 | 315.54 | -39.90 | 118.02 | 0.6709 | -400.0 | -341.1 | |
| 0.00 | 0.70 | 0.00 | 0.49 | -26.44 | 314.02 | -41.42 | 122.04 | 0.7012 | -536.0 | -431.5 | |
| 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. | |