SDO HMI 2014-09-06 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 |
| 57.36 | 225.13 | 45.22 | 177.53 | -19.58 | 107.24 | -44.22 | 122.44 | 0.7808 | 738.8 | 376.1 | |
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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 | 5.27 | 0.00 | 4.26 | -22.73 | 107.80 | -43.66 | 126.28 | 0.7922 | 531.0 | 474.9 | |
| 0.00 | 2.68 | 0.00 | 2.17 | -22.40 | 107.56 | -43.90 | 125.79 | 0.7925 | 642.0 | 572.9 | |
| 0.00 | 0.54 | 0.00 | 0.44 | -22.69 | 107.45 | -44.01 | 126.04 | 0.7950 | 359.0 | 354.2 | |
| 0.00 | 1.70 | 0.00 | 1.38 | -22.27 | 107.21 | -44.25 | 125.43 | 0.7948 | 335.0 | 372.2 | |
| 14.74 | 85.94 | 11.33 | 65.91 | -18.66 | 108.24 | -43.22 | 121.94 | 0.7668 | 1070.4 | 540.0 | |
| 0.00 | 0.80 | 0.00 | 0.63 | -20.11 | 107.75 | -43.71 | 123.33 | 0.7788 | 300.0 | 316.4 | |
| 4.65 | -5.00 | 3.60 | -5.00 | -18.85 | 107.91 | -43.55 | 121.98 | 0.7709 | 648.4 | 999999 | |
| 9.47 | 35.11 | 7.57 | 27.97 | -20.64 | 107.11 | -44.35 | 123.57 | 0.7874 | 784.4 | 462.9 | |
| 25.37 | 75.22 | 20.24 | 60.13 | -19.79 | 106.78 | -44.68 | 122.43 | 0.7861 | 850.4 | 202.2 | |
| 0.00 | 1.97 | 0.00 | 1.59 | -20.47 | 106.44 | -45.02 | 123.00 | 0.7924 | 411.0 | 306.8 | |
| 3.13 | 10.18 | 2.48 | 8.09 | -19.07 | 106.68 | -44.78 | 121.55 | 0.7835 | 738.9 | 318.4 | |
| 0.00 | 0.63 | 0.00 | 0.53 | -18.12 | 102.72 | -48.74 | 118.48 | 0.8150 | -276.0 | -424.9 | |
| 0.00 | 1.07 | 0.00 | 0.93 | -18.05 | 101.81 | -49.64 | 117.98 | 0.8226 | -249.0 | -317.7 | |
| 0.00 | 3.04 | 0.00 | 2.64 | -17.97 | 101.60 | -49.86 | 117.80 | 0.8242 | -531.0 | -383.7 | |
| 0.00 | 0.98 | 0.00 | 0.86 | -18.14 | 101.18 | -50.28 | 117.81 | 0.8285 | -170.0 | -169.1 | |
| 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. | |