SDO HMI 2014-09-08 14:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.34 | 0.00 | 10.97 | -18.02 | 159.86 | 39.21 | 236.31 | 0.7237 | 244.9 | 224.3 | |
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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 | 2.59 | 0.00 | 1.99 | -18.53 | 164.06 | 43.41 | 238.32 | 0.7679 | 237.0 | 217.2 | |
| 0.00 | 0.54 | 0.00 | 0.39 | -17.43 | 161.71 | 41.06 | 238.26 | 0.7392 | 580.0 | 530.7 | |
| 0.00 | 1.61 | 0.00 | 1.16 | -17.65 | 160.56 | 39.91 | 237.27 | 0.7291 | 681.0 | 518.3 | |
| 0.00 | 0.98 | 0.00 | 0.72 | -18.94 | 160.84 | 40.18 | 235.91 | 0.7392 | 515.0 | 404.7 | |
| 0.00 | 0.98 | 0.00 | 0.71 | -18.46 | 160.70 | 40.05 | 236.39 | 0.7351 | 552.0 | 476.5 | |
| 0.00 | 0.62 | 0.00 | 0.45 | -18.38 | 160.47 | 39.81 | 236.35 | 0.7323 | 733.0 | 645.4 | |
| 0.00 | 1.34 | 0.00 | 0.97 | -18.58 | 160.48 | 39.83 | 236.12 | 0.7336 | 568.0 | 424.1 | |
| 0.00 | 0.80 | 0.00 | 0.58 | -18.36 | 160.26 | 39.60 | 236.23 | 0.7301 | 591.0 | 539.3 | |
| 0.00 | 1.07 | 0.00 | 0.73 | -16.38 | 157.94 | 37.29 | 237.10 | 0.6945 | 343.0 | 343.1 | |
| 0.00 | 1.25 | 0.00 | 0.85 | -16.21 | 157.78 | 37.13 | 237.21 | 0.6918 | 662.0 | 527.4 | |
| 0.00 | 0.98 | 0.00 | 0.68 | -18.21 | 157.30 | 36.64 | 234.39 | 0.6997 | -618.0 | -533.3 | |
| 0.00 | 0.62 | 0.00 | 0.43 | -19.13 | 156.73 | 36.08 | 232.86 | 0.7002 | -471.0 | -465.7 | |
| 0.00 | 0.89 | 0.00 | 0.61 | -19.65 | 156.03 | 35.38 | 231.72 | 0.6969 | -587.0 | -488.2 | |
| 0.00 | 1.07 | 0.00 | 0.70 | -16.38 | 154.60 | 33.95 | 234.65 | 0.6592 | -358.0 | -373.6 | |
| 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. | |