SDO HMI 2014-08-07 19:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.52 | 0.00 | 9.22 | -19.23 | 158.71 | -22.03 | 140.03 | 0.5528 | 596.1 | 521.3 | |
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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 | 0.63 | 0.00 | 0.36 | -17.21 | 162.24 | -18.49 | 142.32 | 0.4977 | 635.0 | 557.7 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -17.43 | 160.02 | -20.72 | 139.45 | 0.5212 | 684.0 | 480.4 | |
| 0.00 | 2.26 | 0.00 | 1.31 | -17.47 | 159.71 | -21.03 | 139.09 | 0.5247 | 812.0 | 568.9 | |
| 0.00 | 3.97 | 0.00 | 2.37 | -20.27 | 159.30 | -21.44 | 142.01 | 0.5592 | 1091.0 | 699.2 | |
| 0.00 | 0.63 | 0.00 | 0.37 | -19.33 | 159.33 | -21.41 | 140.92 | 0.5485 | 764.0 | 645.0 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -17.35 | 159.48 | -21.25 | 138.63 | 0.5255 | 725.0 | 631.6 | |
| 0.00 | 1.99 | 0.00 | 1.15 | -16.84 | 159.07 | -21.67 | 137.40 | 0.5242 | 729.0 | 540.4 | |
| 0.00 | 1.54 | 0.00 | 0.93 | -20.20 | 157.80 | -22.94 | 140.07 | 0.5719 | 751.0 | 540.4 | |
| 0.00 | 1.08 | 0.00 | 0.66 | -20.82 | 157.67 | -23.07 | 140.63 | 0.5797 | 570.0 | 465.5 | |
| 0.00 | 0.81 | 0.00 | 0.51 | -21.83 | 154.39 | -26.35 | 138.14 | 0.6196 | -541.0 | -465.4 | |
| 0.00 | 0.63 | 0.00 | 0.41 | -24.50 | 153.73 | -27.00 | 140.44 | 0.6510 | 337.0 | 302.9 | |
| 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. | |