SDO HMI 2014-11-22 01:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.34 | 23.14 | 0.18 | 12.01 | -13.56 | 225.15 | 6.75 | 202.58 | 0.2954 | -364.7 | -353.9 | |
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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 | 1.71 | 0.00 | 0.91 | -15.22 | 231.37 | 12.98 | 216.22 | 0.3683 | -961.0 | -715.0 | |
| 0.00 | 1.71 | 0.00 | 0.89 | -12.92 | 228.67 | 10.27 | 214.02 | 0.3121 | 795.0 | 657.1 | |
| 0.00 | 1.37 | 0.00 | 0.71 | -13.37 | 227.51 | 9.12 | 210.17 | 0.3082 | 773.0 | 670.2 | |
| 0.00 | 0.60 | 0.00 | 0.32 | -19.24 | 227.53 | 9.14 | 202.48 | 0.3939 | -808.0 | -715.3 | |
| 0.00 | 1.37 | 0.00 | 0.74 | -19.24 | 227.37 | 8.98 | 202.13 | 0.3929 | -143.0 | -166.4 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -12.97 | 226.70 | 8.30 | 208.57 | 0.2957 | 871.0 | 703.3 | |
| 0.00 | 1.46 | 0.00 | 0.76 | -13.30 | 226.71 | 8.32 | 208.04 | 0.3007 | 767.0 | 602.4 | |
| 0.00 | 4.12 | 0.00 | 2.11 | -12.28 | 223.44 | 5.05 | 199.19 | 0.2628 | -736.0 | -679.7 | |
| 0.00 | 1.89 | 0.00 | 0.97 | -11.88 | 223.43 | 5.04 | 199.69 | 0.2564 | -791.0 | -584.6 | |
| 0.00 | 0.60 | 0.00 | 0.31 | -10.63 | 223.32 | 4.93 | 201.08 | 0.2359 | -1000.0 | -726.7 | |
| 0.34 | 3.00 | 0.18 | 1.54 | -12.12 | 223.29 | 4.89 | 198.84 | 0.2595 | -1087.2 | -920.1 | |
| 0.00 | 1.54 | 0.00 | 0.80 | -13.65 | 223.13 | 4.74 | 196.54 | 0.2833 | -947.0 | -787.5 | |
| 0.00 | 1.37 | 0.00 | 0.70 | -11.33 | 223.09 | 4.70 | 199.17 | 0.2457 | -945.0 | -632.6 | |
| 0.00 | 1.46 | 0.00 | 0.76 | -17.03 | 221.06 | 2.67 | 187.77 | 0.3311 | -763.0 | -654.7 | |
| 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. | |