SDO HMI 2014-08-14 13:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.85 | 33.98 | 7.98 | 44.75 | 16.06 | 22.65 | -68.86 | 75.29 | 0.9276 | 57.1 | 77.2 | |
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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 |
| 0.63 | 4.42 | 0.74 | 5.16 | 16.43 | 25.80 | -65.71 | 74.91 | 0.9072 | -442.3 | -398.3 | |
| 0.00 | 0.99 | 0.00 | 1.17 | 16.50 | 25.53 | -65.98 | 74.84 | 0.9091 | -301.0 | -322.7 | |
| 0.00 | 1.98 | 0.00 | 2.36 | 16.73 | 25.29 | -66.22 | 74.59 | 0.9108 | -483.0 | -392.9 | |
| 0.00 | 0.81 | 0.00 | 0.97 | 16.64 | 25.03 | -66.48 | 74.69 | 0.9125 | -210.0 | -231.6 | |
| 0.00 | 2.25 | 0.00 | 2.78 | 17.01 | 24.36 | -67.15 | 74.29 | 0.9171 | -258.0 | -206.1 | |
| 0.00 | 0.99 | 0.00 | 1.20 | 16.12 | 24.90 | -66.61 | 75.26 | 0.9134 | -166.0 | -123.8 | |
| 0.00 | 0.54 | 0.00 | 0.65 | 15.94 | 25.02 | -66.49 | 75.45 | 0.9126 | -168.0 | -203.5 | |
| 0.00 | 0.63 | 0.00 | 0.77 | 15.44 | 24.46 | -67.05 | 76.00 | 0.9165 | -243.0 | -220.0 | |
| 0.63 | 1.44 | 0.81 | 1.86 | 16.51 | 23.21 | -68.30 | 74.83 | 0.9246 | -138.9 | -87.4 | |
| 2.52 | 9.38 | 3.33 | 12.31 | 15.44 | 22.59 | -68.92 | 75.98 | 0.9286 | 413.9 | 358.6 | |
| 0.00 | 4.06 | 0.00 | 5.93 | 16.26 | 20.25 | -71.26 | 75.05 | 0.9424 | 534.0 | 385.9 | |
| 0.00 | 1.17 | 0.00 | 1.71 | 15.89 | 20.36 | -71.14 | 75.44 | 0.9418 | 469.0 | 475.9 | |
| 2.07 | 3.25 | 3.10 | 4.85 | 16.25 | 19.86 | -71.65 | 75.05 | 0.9446 | 161.8 | 163.0 | |
| 0.00 | 0.99 | 0.00 | 1.43 | 15.27 | 20.68 | -70.83 | 76.12 | 0.9401 | 375.0 | 363.9 | |
| 0.00 | 1.08 | 0.00 | 1.60 | 15.70 | 20.03 | -71.48 | 75.64 | 0.9437 | 95.0 | 72.5 | |
| 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. | |