SDO HMI 2014-04-15 05:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.48 | 397.21 | 32.12 | 217.94 | 11.88 | 274.95 | 18.53 | 313.60 | 0.4314 | -923.1 | -357.6 | |
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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 |
| 58.21 | 375.54 | 31.97 | 206.25 | 11.76 | 275.28 | 18.86 | 312.83 | 0.4334 | -1433.3 | -421.2 | |
| 0.27 | -1.00 | 0.15 | -1.00 | 12.19 | 274.89 | 18.47 | 314.16 | 0.4336 | -1111.7 | 999999 | |
| 0.00 | 1.15 | 0.00 | 0.63 | 13.92 | 272.04 | 15.63 | 321.67 | 0.4234 | -688.0 | -617.9 | |
| 0.00 | 1.06 | 0.00 | 0.58 | 14.24 | 272.07 | 15.65 | 322.11 | 0.4276 | -701.0 | -536.2 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 12.76 | 270.47 | 14.05 | 322.84 | 0.3937 | 723.0 | 631.2 | |
| 0.00 | 2.03 | 0.00 | 1.10 | 13.02 | 270.32 | 13.90 | 323.52 | 0.3955 | 891.0 | 724.4 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 12.79 | 270.21 | 13.80 | 323.38 | 0.3915 | 908.0 | 653.5 | |
| 0.00 | 3.10 | 0.00 | 1.67 | 13.10 | 269.91 | 13.50 | 324.46 | 0.3927 | 1010.0 | 844.3 | |
| 0.00 | 6.28 | 0.00 | 3.40 | 14.42 | 269.04 | 12.62 | 328.12 | 0.4024 | 859.0 | 690.2 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 14.77 | 268.83 | 12.42 | 329.00 | 0.4054 | 769.0 | 634.8 | |
| 0.00 | 1.24 | 0.00 | 0.67 | 14.63 | 268.16 | 11.74 | 330.21 | 0.3980 | 877.0 | 823.0 | |
| 0.00 | 1.86 | 0.00 | 0.99 | 13.81 | 267.32 | 10.91 | 330.95 | 0.3801 | 906.0 | 734.4 | |
| 0.00 | 1.50 | 0.00 | 0.79 | 11.89 | 266.33 | 9.91 | 330.63 | 0.3450 | 820.0 | 725.4 | |
| 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. | |