SDO HMI 2014-07-05 16:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.17 | 28.24 | 2.71 | 14.71 | -13.87 | 253.96 | -5.02 | 164.19 | 0.3107 | 440.8 | 339.4 | |
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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 | 1.00 | 0.00 | 0.51 | -12.54 | 259.40 | 0.42 | 181.49 | 0.2750 | 748.0 | 567.9 | |
| 0.00 | 0.36 | 0.00 | 0.19 | -13.69 | 257.80 | -1.18 | 176.09 | 0.2948 | 651.0 | 608.2 | |
| 0.00 | 1.18 | 0.00 | 0.61 | -12.70 | 257.56 | -1.43 | 174.98 | 0.2786 | 1000.0 | 847.0 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -14.48 | 257.45 | -1.53 | 175.17 | 0.3086 | 820.0 | 709.4 | |
| 0.00 | 1.73 | 0.00 | 0.89 | -13.37 | 257.05 | -1.93 | 173.49 | 0.2906 | 857.0 | 727.6 | |
| 0.00 | 1.45 | 0.00 | 0.75 | -11.76 | 254.67 | -4.32 | 164.19 | 0.2718 | 807.0 | 640.3 | |
| 1.63 | 4.00 | 0.85 | 2.08 | -14.01 | 254.37 | -4.61 | 165.34 | 0.3095 | 1092.8 | 820.5 | |
| 0.00 | 3.63 | 0.00 | 1.89 | -14.24 | 254.05 | -4.93 | 164.57 | 0.3145 | 976.0 | 769.9 | |
| 0.00 | 1.00 | 0.00 | 0.51 | -7.13 | 253.87 | -5.12 | 154.02 | 0.2029 | 829.0 | 711.8 | |
| 1.09 | 2.09 | 0.57 | 1.09 | -14.59 | 253.22 | -5.76 | 162.47 | 0.3240 | 780.2 | 612.2 | |
| 0.00 | 1.09 | 0.00 | 0.57 | -14.69 | 252.97 | -6.02 | 161.84 | 0.3269 | 653.0 | 513.6 | |
| 0.00 | 0.91 | 0.00 | 0.48 | -14.37 | 252.47 | -6.52 | 160.12 | 0.3246 | -717.0 | -570.9 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -13.22 | 252.47 | -6.51 | 158.80 | 0.3068 | 791.0 | 617.0 | |
| 0.00 | 2.27 | 0.00 | 1.19 | -14.79 | 251.57 | -7.42 | 158.12 | 0.3364 | -1039.0 | -806.4 | |
| 2.45 | 4.90 | 1.29 | 2.58 | -15.15 | 251.52 | -7.46 | 158.40 | 0.3420 | -980.4 | -843.3 | |
| 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. | |