SDO HMI 2014-08-06 10:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.90 | 19.80 | 1.44 | 14.57 | -20.26 | 158.64 | -40.29 | 124.80 | 0.7395 | 234.7 | 191.2 | |
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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 |
| 0.00 | 2.89 | 0.00 | 1.91 | -17.54 | 164.72 | -34.21 | 125.61 | 0.6617 | 192.0 | 356.4 | |
| 0.00 | 1.18 | 0.00 | 0.81 | -18.50 | 162.17 | -36.76 | 124.96 | 0.6947 | 598.0 | 473.2 | |
| 0.00 | 0.99 | 0.00 | 0.69 | -17.98 | 161.50 | -37.43 | 123.85 | 0.6984 | 637.0 | 442.9 | |
| 0.00 | 1.81 | 0.00 | 1.33 | -22.78 | 160.00 | -38.93 | 128.55 | 0.7431 | 598.0 | 434.1 | |
| 0.00 | 0.72 | 0.00 | 0.53 | -20.08 | 158.71 | -40.22 | 124.58 | 0.7388 | 286.0 | 282.2 | |
| 0.00 | 0.90 | 0.00 | 0.64 | -17.25 | 159.19 | -39.74 | 121.44 | 0.7180 | 631.0 | 510.4 | |
| 0.00 | 1.27 | 0.00 | 0.92 | -19.23 | 158.42 | -40.51 | 123.39 | 0.7368 | 607.0 | 539.7 | |
| 0.00 | 1.18 | 0.00 | 0.89 | -21.38 | 157.55 | -41.38 | 125.38 | 0.7573 | 603.0 | 531.8 | |
| 1.09 | 2.08 | 0.82 | 1.58 | -21.20 | 157.31 | -41.62 | 125.02 | 0.7585 | 521.1 | 459.8 | |
| 0.00 | 0.45 | 0.00 | 0.34 | -20.88 | 157.42 | -41.51 | 124.73 | 0.7557 | 600.0 | 507.4 | |
| 0.81 | 1.99 | 0.62 | 1.51 | -21.22 | 156.99 | -41.94 | 124.86 | 0.7615 | 372.1 | 318.2 | |
| 0.00 | 0.27 | 0.00 | 0.21 | -21.66 | 155.68 | -43.26 | 124.60 | 0.7760 | -280.0 | -376.7 | |
| 0.00 | 1.27 | 0.00 | 1.00 | -21.54 | 155.00 | -43.94 | 124.08 | 0.7815 | -579.0 | -456.5 | |
| 0.00 | 0.90 | 0.00 | 0.71 | -21.05 | 155.13 | -43.80 | 123.60 | 0.7778 | -539.0 | -487.6 | |
| 0.00 | 1.90 | 0.00 | 1.50 | -21.25 | 154.83 | -44.10 | 123.66 | 0.7815 | -623.0 | -535.3 | |
| 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. | |