SDO HMI 2014-06-07 14:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.90 | 0.00 | 12.81 | 4.63 | 259.62 | -11.09 | 167.26 | 0.2333 | 244.0 | 162.1 | |
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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 | 2.44 | 0.00 | 1.22 | 5.21 | 273.72 | 3.00 | 329.64 | 0.1037 | -941.0 | -682.0 | |
| 0.00 | 1.36 | 0.00 | 0.67 | 4.27 | 273.37 | 2.66 | 327.47 | 0.0865 | -1007.0 | -865.6 | |
| 0.00 | 2.53 | 0.00 | 1.26 | 3.96 | 271.82 | 1.11 | 344.06 | 0.0704 | -679.0 | -470.5 | |
| 0.00 | 1.00 | 0.00 | 0.49 | 2.84 | 271.78 | 1.07 | 338.61 | 0.0515 | -785.0 | -691.1 | |
| 0.00 | 1.54 | 0.00 | 0.76 | 2.02 | 269.32 | -1.39 | 36.04 | 0.0415 | -1092.0 | -835.4 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 0.96 | 260.84 | -9.87 | 84.98 | 0.1728 | 873.0 | 610.4 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 4.86 | 260.53 | -10.18 | 64.76 | 0.1955 | 908.0 | 646.9 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 4.92 | 257.70 | -13.02 | 69.45 | 0.2407 | 756.0 | 588.1 | |
| 0.00 | 1.81 | 0.00 | 0.93 | 5.90 | 256.45 | -14.26 | 67.58 | 0.2663 | 892.0 | 632.7 | |
| 0.00 | 2.08 | 0.00 | 1.07 | 3.22 | 256.28 | -14.43 | 77.66 | 0.2559 | 923.0 | 705.6 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 9.47 | 252.28 | -18.44 | 62.44 | 0.3534 | 870.0 | 660.3 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 5.48 | 250.41 | -20.31 | 74.80 | 0.3595 | 804.0 | 583.3 | |
| 0.00 | 1.18 | 0.00 | 0.62 | -0.34 | 249.78 | -20.93 | 91.21 | 0.3589 | 830.0 | 607.1 | |
| 0.00 | 2.35 | 0.00 | 1.27 | 6.28 | 247.61 | -23.11 | 74.57 | 0.4064 | 507.0 | 412.8 | |
| 0.00 | 1.36 | 0.00 | 0.78 | 6.89 | 241.52 | -29.19 | 76.25 | 0.5004 | 801.0 | 641.3 | |
| 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. | |