SDO HMI 2014-07-03 14:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.08 | 34.07 | 13.66 | 30.54 | -16.14 | 232.92 | -53.64 | 111.76 | 0.8341 | -45.7 | -10.9 | |
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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 | 1.09 | 0.00 | 0.81 | -16.90 | 242.26 | -44.30 | 116.12 | 0.7465 | 502.0 | 413.0 | |
| 0.00 | 0.64 | 0.00 | 0.50 | -14.03 | 238.65 | -47.91 | 111.08 | 0.7738 | 343.0 | 399.7 | |
| 0.00 | 0.82 | 0.00 | 0.68 | -14.84 | 235.43 | -51.13 | 110.99 | 0.8083 | -218.0 | -178.0 | |
| 3.54 | 8.81 | 2.95 | 7.36 | -14.39 | 235.53 | -51.03 | 110.48 | 0.8061 | 761.6 | 514.6 | |
| 1.91 | -4.00 | 1.60 | -4.00 | -14.59 | 235.31 | -51.25 | 110.65 | 0.8088 | 496.1 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.23 | -14.51 | 234.88 | -51.68 | 110.43 | 0.8127 | 371.0 | 391.3 | |
| 0.00 | 1.91 | 0.00 | 1.66 | -16.27 | 234.15 | -52.42 | 112.28 | 0.8242 | 434.0 | 361.0 | |
| 0.00 | 0.91 | 0.00 | 0.79 | -15.18 | 234.08 | -52.48 | 110.98 | 0.8220 | -267.0 | -228.8 | |
| 0.00 | 0.27 | 0.00 | 0.25 | -15.89 | 232.54 | -54.03 | 111.35 | 0.8378 | 362.0 | 342.7 | |
| 0.00 | 1.82 | 0.00 | 1.67 | -16.43 | 232.04 | -54.52 | 111.82 | 0.8434 | -683.0 | -557.7 | |
| 9.63 | 17.53 | 9.11 | 16.59 | -16.99 | 230.96 | -55.60 | 112.15 | 0.8541 | -535.1 | -227.8 | |
| 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. | |