SDO HMI 2011-11-02 22:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 89.84 | 428.37 | 83.64 | 399.96 | -13.67 | 120.36 | -55.51 | 109.10 | 0.8489 | 281.9 | 196.1 | |
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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 |
| 8.21 | 229.23 | 7.09 | 200.59 | -14.78 | 123.77 | -52.10 | 111.36 | 0.8214 | 971.6 | 319.8 | |
| 8.73 | -1.00 | 7.68 | -1.00 | -15.26 | 123.15 | -52.72 | 111.71 | 0.8285 | 609.7 | 999999 | |
| 2.08 | -1.00 | 1.84 | -1.00 | -15.56 | 122.89 | -52.99 | 111.97 | 0.8317 | 379.3 | 999999 | |
| 26.72 | -1.00 | 23.43 | -1.00 | -14.67 | 123.10 | -52.77 | 111.01 | 0.8273 | 697.4 | 999999 | |
| 0.35 | -1.00 | 0.31 | -1.00 | -14.77 | 122.40 | -53.48 | 110.91 | 0.8340 | 285.8 | 999999 | |
| 1.90 | -1.00 | 1.69 | -1.00 | -14.55 | 122.42 | -53.45 | 110.66 | 0.8332 | 421.8 | 999999 | |
| 0.00 | 1.38 | 0.00 | 1.26 | -14.31 | 121.35 | -54.52 | 110.05 | 0.8421 | 325.0 | 299.8 | |
| 1.47 | 4.58 | 1.35 | 4.21 | -14.13 | 121.20 | -54.67 | 109.80 | 0.8430 | 340.5 | -127.0 | |
| 3.03 | 6.23 | 2.78 | 5.73 | -13.65 | 120.89 | -54.98 | 109.16 | 0.8447 | 453.0 | 114.2 | |
| 4.24 | 5.88 | 4.14 | 5.75 | -14.59 | 118.82 | -57.05 | 109.66 | 0.8644 | -703.9 | -583.6 | |
| 0.86 | 1.47 | 0.83 | 1.41 | -13.32 | 119.26 | -56.62 | 108.34 | 0.8581 | -740.5 | -695.7 | |
| 0.00 | 3.11 | 0.00 | 2.99 | -13.48 | 119.14 | -56.73 | 108.49 | 0.8594 | -685.0 | -556.1 | |
| 1.04 | 1.47 | 1.01 | 1.42 | -13.34 | 118.85 | -57.02 | 108.26 | 0.8616 | -558.2 | -531.8 | |
| 3.55 | 19.37 | 3.63 | 19.91 | -15.37 | 117.44 | -58.43 | 110.16 | 0.8771 | -591.5 | -389.4 | |
| 1.21 | 1.73 | 1.23 | 1.75 | -14.86 | 117.61 | -58.26 | 109.64 | 0.8748 | -552.8 | -558.0 | |
| 3.63 | -14.00 | 3.73 | -14.00 | -15.00 | 117.31 | -58.56 | 109.72 | 0.8774 | -573.0 | 999999 | |
| 3.63 | -14.00 | 3.76 | -14.00 | -15.24 | 117.03 | -58.85 | 109.91 | 0.8801 | -310.4 | 999999 | |
| 0.00 | 16.08 | 0.00 | 16.90 | -15.61 | 116.61 | -59.26 | 110.21 | 0.8841 | -154.0 | -122.8 | |
| 0.00 | 1.56 | 0.00 | 1.75 | -18.11 | 115.16 | -60.71 | 112.56 | 0.8995 | -586.0 | -463.1 | |
| 3.11 | 5.88 | 3.19 | 6.03 | -13.93 | 117.06 | -58.82 | 108.46 | 0.8774 | -705.6 | -442.0 | |
| 0.00 | 0.86 | 0.00 | 0.90 | -14.41 | 116.85 | -59.02 | 108.94 | 0.8799 | -274.0 | -232.0 | |
| 6.83 | 112.58 | 6.68 | 111.25 | -10.93 | 117.96 | -57.91 | 105.31 | 0.8645 | 964.6 | 239.3 | |
| 0.00 | 2.16 | 0.00 | 2.30 | -15.14 | 116.16 | -59.71 | 109.58 | 0.8866 | -394.0 | -212.2 | |
| 0.00 | 2.25 | 0.00 | 2.36 | -14.35 | 116.33 | -59.54 | 108.75 | 0.8838 | -173.0 | -67.0 | |
| 0.00 | 2.33 | 0.00 | 2.50 | -14.94 | 115.88 | -59.99 | 109.29 | 0.8884 | -395.0 | -346.2 | |
| 8.56 | -22.00 | 8.52 | -22.00 | -10.94 | 117.38 | -58.49 | 105.19 | 0.8694 | 518.4 | 999999 | |
| 0.00 | 0.61 | 0.00 | 0.59 | -9.01 | 117.93 | -57.94 | 103.11 | 0.8615 | 374.0 | 318.4 | |
| 0.00 | 0.95 | 0.00 | 0.97 | -11.24 | 116.51 | -59.36 | 105.33 | 0.8770 | -216.0 | -181.8 | |
| 0.00 | 2.25 | 0.00 | 2.56 | -15.65 | 114.19 | -61.68 | 109.65 | 0.9020 | -655.0 | -403.5 | |
| 0.00 | 0.78 | 0.00 | 0.81 | -10.94 | 115.95 | -59.92 | 104.88 | 0.8811 | 277.0 | 254.3 | |
| 0.00 | 1.73 | 0.00 | 1.78 | -10.23 | 116.06 | -59.81 | 104.10 | 0.8791 | 563.0 | 462.6 | |
| 0.00 | 0.61 | 0.00 | 0.69 | -14.31 | 113.61 | -62.26 | 108.07 | 0.9039 | -391.0 | -389.6 | |
| 0.69 | 3.29 | 0.75 | 3.55 | -10.27 | 114.62 | -61.25 | 103.85 | 0.8904 | 515.4 | 379.9 | |
| 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. | |