SDO HMI 2014-08-07 00:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.44 | 18.79 | 1.63 | 12.60 | -20.81 | 158.12 | -33.08 | 130.69 | 0.6741 | 437.0 | 281.4 | |
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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 | 0.81 | 0.00 | 0.49 | -17.53 | 164.64 | -26.55 | 132.55 | 0.5808 | 541.0 | 512.1 | |
| 0.00 | 0.81 | 0.00 | 0.51 | -20.05 | 162.96 | -28.24 | 134.06 | 0.6207 | 602.0 | 463.4 | |
| 0.00 | 1.45 | 0.00 | 0.96 | -22.64 | 160.12 | -31.08 | 134.48 | 0.6700 | 762.0 | 598.6 | |
| 0.00 | 0.45 | 0.00 | 0.30 | -22.54 | 159.49 | -31.71 | 133.81 | 0.6750 | 382.0 | 386.4 | |
| 0.00 | 1.27 | 0.00 | 0.83 | -20.48 | 159.57 | -31.63 | 131.45 | 0.6576 | 665.0 | 557.8 | |
| 0.00 | 2.08 | 0.00 | 1.36 | -19.31 | 158.80 | -32.39 | 129.36 | 0.6561 | 734.0 | 620.8 | |
| 2.44 | 4.16 | 1.63 | 2.78 | -20.86 | 158.32 | -32.87 | 130.85 | 0.6728 | 789.4 | 630.1 | |
| 0.00 | 0.90 | 0.00 | 0.60 | -19.54 | 158.37 | -32.83 | 129.28 | 0.6623 | 618.0 | 474.1 | |
| 0.00 | 0.81 | 0.00 | 0.55 | -21.06 | 157.88 | -33.31 | 130.72 | 0.6786 | 596.0 | 406.2 | |
| 0.00 | 0.54 | 0.00 | 0.37 | -21.26 | 157.44 | -33.76 | 130.60 | 0.6844 | 538.0 | 460.3 | |
| 0.00 | 0.99 | 0.00 | 0.68 | -21.51 | 157.25 | -33.94 | 130.75 | 0.6880 | 519.0 | 470.9 | |
| 0.00 | 0.99 | 0.00 | 0.67 | -20.72 | 157.38 | -33.81 | 129.91 | 0.6809 | 626.0 | 553.8 | |
| 0.00 | 1.45 | 0.00 | 1.03 | -22.17 | 154.40 | -36.79 | 129.37 | 0.7197 | -683.0 | -540.1 | |
| 0.00 | 2.08 | 0.00 | 1.47 | -21.19 | 154.33 | -36.86 | 128.17 | 0.7138 | -794.0 | -640.0 | |
| 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. | |