SDO HMI 2014-09-07 03:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.26 | 68.39 | 13.68 | 36.98 | -14.31 | 149.49 | 9.59 | 203.91 | 0.4019 | 124.9 | 117.6 | |
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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 | 3.48 | 0.00 | 1.87 | -13.22 | 150.12 | 10.23 | 206.42 | 0.3901 | -14.0 | 36.2 | |
| 0.00 | 1.70 | 0.00 | 0.93 | -15.99 | 150.12 | 10.23 | 203.49 | 0.4300 | -901.0 | -743.7 | |
| 5.62 | 35.71 | 3.02 | 19.14 | -12.92 | 149.83 | 9.93 | 206.10 | 0.3837 | 1120.0 | 624.9 | |
| 7.05 | -3.00 | 3.78 | -3.00 | -13.17 | 149.61 | 9.72 | 205.33 | 0.3859 | 940.8 | 999999 | |
| 2.59 | -3.00 | 1.38 | -3.00 | -12.66 | 149.53 | 9.64 | 205.73 | 0.3778 | 1083.8 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -13.56 | 149.54 | 9.64 | 204.72 | 0.3910 | 655.0 | 528.8 | |
| 2.14 | 20.80 | 1.18 | 11.43 | -16.50 | 149.60 | 9.71 | 201.95 | 0.4343 | -938.6 | -783.6 | |
| 0.45 | -7.00 | 0.25 | -7.00 | -16.66 | 149.55 | 9.65 | 201.69 | 0.4364 | -740.8 | 999999 | |
| 0.00 | 2.86 | 0.00 | 1.54 | -13.91 | 149.39 | 9.50 | 204.01 | 0.3952 | 559.0 | 471.5 | |
| 5.80 | -7.00 | 3.19 | -7.00 | -16.63 | 149.32 | 9.43 | 201.27 | 0.4345 | -1027.6 | 999999 | |
| 1.61 | -7.00 | 0.88 | -7.00 | -16.59 | 149.19 | 9.30 | 201.03 | 0.4333 | -1001.2 | 999999 | |
| 0.00 | 1.70 | 0.00 | 0.91 | -13.94 | 147.66 | 7.77 | 199.99 | 0.3852 | 822.0 | 680.1 | |
| 0.00 | 1.25 | 0.00 | 0.68 | -15.70 | 145.70 | 5.80 | 194.04 | 0.4031 | -780.0 | -640.4 | |
| 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. | |