SDO HMI 2011-10-06 04:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.84 | 198.32 | 60.33 | 261.67 | -14.60 | 116.81 | -65.08 | 108.69 | 0.9270 | -19.8 | 9.2 | |
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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 |
| 6.77 | 95.69 | 7.90 | 113.33 | -14.52 | 119.93 | -61.97 | 109.38 | 0.9075 | 749.4 | 198.2 | |
| 0.00 | 1.76 | 0.00 | 2.14 | -15.13 | 118.94 | -62.96 | 109.76 | 0.9153 | -384.0 | -351.4 | |
| 13.88 | -1.00 | 16.53 | -1.00 | -14.17 | 119.36 | -62.53 | 108.85 | 0.9108 | 573.0 | 999999 | |
| 2.90 | -1.00 | 3.51 | -1.00 | -14.53 | 118.91 | -62.99 | 109.12 | 0.9145 | -472.4 | 999999 | |
| 1.93 | 9.75 | 2.39 | 12.18 | -13.76 | 118.19 | -63.70 | 108.11 | 0.9179 | 339.0 | 295.1 | |
| 1.32 | -5.00 | 1.67 | -5.00 | -13.57 | 117.57 | -64.32 | 107.76 | 0.9216 | 307.8 | 999999 | |
| 0.00 | 1.58 | 0.00 | 2.02 | -13.84 | 117.36 | -64.53 | 108.00 | 0.9234 | 236.0 | 191.4 | |
| 11.25 | 24.69 | 15.00 | 32.74 | -15.10 | 116.58 | -65.31 | 109.13 | 0.9301 | -631.0 | -435.9 | |
| 0.00 | 0.97 | 0.00 | 1.31 | -14.59 | 115.97 | -65.92 | 108.45 | 0.9330 | -413.0 | -373.6 | |
| 0.00 | 4.13 | 0.00 | 5.85 | -15.49 | 115.26 | -66.63 | 109.22 | 0.9384 | -494.0 | -246.1 | |
| 1.58 | 3.25 | 2.33 | 4.82 | -15.18 | 114.33 | -67.56 | 108.69 | 0.9431 | -378.8 | -274.6 | |
| 1.85 | 56.50 | 2.78 | 87.28 | -15.14 | 113.77 | -68.12 | 108.52 | 0.9461 | -370.3 | -88.5 | |
| 5.36 | -12.00 | 8.22 | -12.00 | -14.71 | 113.38 | -68.51 | 107.99 | 0.9477 | -474.3 | 999999 | |
| 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. | |