SDO HMI 2011-10-06 06:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.85 | 16.16 | 1.20 | 10.28 | -16.12 | 149.24 | -31.56 | 126.38 | 0.6288 | -98.6 | -80.0 | |
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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 | 0.97 | 0.00 | 0.59 | -19.70 | 156.13 | -24.66 | 137.67 | 0.5856 | 582.0 | 484.6 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -17.85 | 155.45 | -25.35 | 134.57 | 0.5742 | 651.0 | 509.5 | |
| 0.00 | 1.67 | 0.00 | 1.02 | -16.36 | 152.80 | -28.00 | 129.80 | 0.5885 | 649.0 | 480.2 | |
| 0.00 | 0.88 | 0.00 | 0.57 | -20.97 | 151.36 | -29.44 | 134.25 | 0.6430 | -653.0 | -544.3 | |
| 0.00 | 1.05 | 0.00 | 0.67 | -19.42 | 151.46 | -29.33 | 132.48 | 0.6287 | -663.0 | -598.5 | |
| 0.00 | 1.14 | 0.00 | 0.74 | -20.40 | 150.67 | -30.13 | 132.93 | 0.6448 | -736.0 | -540.8 | |
| 0.00 | 1.32 | 0.00 | 0.85 | -20.27 | 150.66 | -30.14 | 132.77 | 0.6438 | -763.0 | -586.2 | |
| 0.00 | 1.05 | 0.00 | 0.67 | -15.62 | 148.37 | -32.43 | 124.81 | 0.6313 | 480.0 | 414.6 | |
| 0.00 | 0.88 | 0.00 | 0.55 | -12.93 | 148.00 | -32.80 | 120.79 | 0.6169 | 678.0 | 617.3 | |
| 0.00 | 1.05 | 0.00 | 0.67 | -14.02 | 147.38 | -33.41 | 121.85 | 0.6313 | 617.0 | 489.3 | |
| 0.00 | 1.41 | 0.00 | 0.91 | -12.73 | 145.23 | -35.56 | 118.53 | 0.6480 | -721.0 | -573.7 | |
| 1.85 | 2.46 | 1.20 | 1.60 | -12.18 | 144.98 | -35.82 | 117.59 | 0.6477 | -615.0 | -576.3 | |
| 0.00 | 1.14 | 0.00 | 0.75 | -12.95 | 143.94 | -36.86 | 117.97 | 0.6643 | -685.0 | -584.6 | |
| 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. | |