SDO HMI 2014-09-07 06:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.06 | 58.56 | 12.01 | 31.89 | -14.47 | 149.57 | 11.32 | 207.46 | 0.4160 | -44.4 | 60.9 | |
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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 | 2.68 | 0.00 | 1.48 | -15.98 | 150.24 | 11.99 | 207.01 | 0.4415 | -638.0 | -642.2 | |
| 6.61 | 30.36 | 3.56 | 16.36 | -12.78 | 149.94 | 11.69 | 210.16 | 0.3949 | 1064.3 | 741.8 | |
| 2.59 | -2.00 | 1.40 | -2.00 | -13.07 | 149.89 | 11.64 | 209.69 | 0.3985 | 963.8 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -13.55 | 149.66 | 11.41 | 208.61 | 0.4034 | 463.0 | 498.8 | |
| 3.30 | -2.00 | 1.78 | -2.00 | -12.61 | 149.59 | 11.34 | 209.62 | 0.3897 | 1083.4 | 999999 | |
| 2.59 | 19.55 | 1.43 | 10.80 | -16.39 | 149.65 | 11.40 | 205.45 | 0.4432 | -940.2 | -769.3 | |
| 0.27 | -6.00 | 0.15 | -6.00 | -16.38 | 149.46 | 11.21 | 205.07 | 0.4419 | -1099.0 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -13.86 | 149.33 | 11.08 | 207.52 | 0.4053 | 827.0 | 615.4 | |
| 3.57 | -6.00 | 1.97 | -6.00 | -16.58 | 149.41 | 11.15 | 204.78 | 0.4443 | -1018.0 | 999999 | |
| 3.13 | -6.00 | 1.72 | -6.00 | -16.54 | 149.24 | 10.99 | 204.49 | 0.4427 | -1028.0 | 999999 | |
| 0.00 | 2.05 | 0.00 | 1.13 | -16.60 | 148.99 | 10.74 | 203.94 | 0.4419 | -771.0 | -534.5 | |
| 0.00 | 1.25 | 0.00 | 0.68 | -16.04 | 147.68 | 9.43 | 201.80 | 0.4259 | -600.0 | -447.6 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -15.77 | 145.67 | 7.42 | 197.67 | 0.4111 | -810.0 | -743.8 | |
| 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. | |