SDO HMI 2014-01-09 11:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.03 | 0.00 | 9.66 | -15.15 | 111.11 | 33.00 | 248.44 | 0.5668 | -425.2 | -371.8 | |
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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 | 1.61 | 0.00 | 1.06 | -12.26 | 118.82 | 40.71 | 255.85 | 0.6596 | 680.0 | 574.5 | |
| 0.00 | 1.02 | 0.00 | 0.66 | -12.38 | 117.97 | 39.86 | 255.48 | 0.6490 | 691.0 | 606.8 | |
| 0.00 | 1.19 | 0.00 | 0.72 | -14.08 | 112.29 | 34.18 | 251.04 | 0.5785 | -745.0 | -638.1 | |
| 0.00 | 2.21 | 0.00 | 1.33 | -15.40 | 111.53 | 33.42 | 248.48 | 0.5730 | -717.0 | -567.9 | |
| 0.00 | 0.93 | 0.00 | 0.56 | -16.41 | 110.33 | 32.22 | 246.18 | 0.5613 | -640.0 | -485.2 | |
| 0.00 | 2.46 | 0.00 | 1.46 | -17.13 | 109.59 | 31.48 | 244.54 | 0.5549 | -800.0 | -693.3 | |
| 0.00 | 0.76 | 0.00 | 0.46 | -17.71 | 109.56 | 31.45 | 243.54 | 0.5574 | -118.0 | -139.2 | |
| 0.00 | 1.78 | 0.00 | 1.06 | -16.75 | 109.27 | 31.16 | 245.01 | 0.5488 | -753.0 | -630.9 | |
| 0.00 | 1.10 | 0.00 | 0.65 | -17.10 | 108.86 | 30.75 | 244.17 | 0.5452 | -809.0 | -688.6 | |
| 0.00 | 1.44 | 0.00 | 0.83 | -13.56 | 107.25 | 29.14 | 249.68 | 0.5068 | -811.0 | -664.5 | |
| 0.00 | 1.53 | 0.00 | 0.87 | -13.86 | 106.42 | 28.31 | 248.66 | 0.4964 | -655.0 | -426.6 | |
| 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. | |