SDO HMI 2011-11-02 16:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 81.87 | 406.66 | 83.51 | 415.45 | -13.75 | 120.57 | -58.62 | 108.38 | 0.8750 | 302.6 | 134.7 | |
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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 | 0.78 | 0.00 | 0.69 | -15.74 | 126.14 | -53.05 | 112.17 | 0.8328 | 423.0 | 447.4 | |
| 9.16 | 234.80 | 8.62 | 224.96 | -14.71 | 123.61 | -55.58 | 110.21 | 0.8523 | 922.1 | 231.6 | |
| 10.20 | -2.00 | 9.81 | -2.00 | -15.19 | 122.92 | -56.27 | 110.56 | 0.8593 | 513.0 | 999999 | |
| 3.03 | -2.00 | 2.93 | -2.00 | -15.57 | 122.76 | -56.43 | 110.95 | 0.8615 | 346.3 | 999999 | |
| 21.53 | -2.00 | 20.58 | -2.00 | -14.62 | 122.98 | -56.21 | 109.94 | 0.8575 | 690.4 | 999999 | |
| 3.63 | -2.00 | 3.54 | -2.00 | -14.54 | 122.28 | -56.91 | 109.65 | 0.8632 | 337.2 | 999999 | |
| 0.00 | 1.56 | 0.00 | 1.55 | -15.33 | 121.66 | -57.52 | 110.37 | 0.8699 | -363.0 | -331.9 | |
| 0.00 | 0.69 | 0.00 | 0.69 | -14.64 | 121.67 | -57.52 | 109.60 | 0.8684 | -81.0 | -130.6 | |
| 0.00 | 0.78 | 0.00 | 0.77 | -13.44 | 121.57 | -57.62 | 108.22 | 0.8668 | 297.0 | 279.4 | |
| 1.82 | 4.67 | 1.83 | 4.70 | -13.97 | 121.01 | -58.17 | 108.68 | 0.8724 | 182.2 | -63.4 | |
| 1.73 | 4.67 | 1.75 | 4.73 | -13.62 | 120.68 | -58.50 | 108.20 | 0.8743 | 254.0 | 46.4 | |
| 0.00 | 1.12 | 0.00 | 1.15 | -13.55 | 120.30 | -58.89 | 108.03 | 0.8773 | -306.0 | -260.2 | |
| 0.00 | 1.47 | 0.00 | 1.53 | -13.70 | 119.87 | -59.31 | 108.09 | 0.8809 | -386.0 | -404.9 | |
| 1.30 | 2.33 | 1.39 | 2.50 | -14.56 | 119.13 | -60.06 | 108.86 | 0.8882 | -550.3 | -469.8 | |
| 0.00 | 1.64 | 0.00 | 1.75 | -13.48 | 119.05 | -60.14 | 107.65 | 0.8869 | -592.0 | -570.5 | |
| 0.00 | 1.30 | 0.00 | 1.37 | -13.23 | 119.09 | -60.10 | 107.38 | 0.8862 | -710.0 | -630.9 | |
| 0.00 | 1.38 | 0.00 | 1.48 | -13.43 | 118.82 | -60.37 | 107.55 | 0.8886 | -510.0 | -479.0 | |
| 0.00 | 1.30 | 0.00 | 1.45 | -15.02 | 117.83 | -61.35 | 109.06 | 0.8986 | -582.0 | -533.5 | |
| 3.37 | 4.32 | 3.82 | 4.90 | -15.42 | 117.50 | -61.68 | 109.41 | 0.9017 | -526.8 | -506.5 | |
| 1.38 | 28.10 | 1.57 | 32.58 | -15.08 | 117.34 | -61.84 | 109.01 | 0.9022 | -545.4 | -50.4 | |
| 0.69 | -20.00 | 0.79 | -20.00 | -15.44 | 117.16 | -62.03 | 109.36 | 0.9041 | -221.9 | 999999 | |
| 1.04 | -20.00 | 1.19 | -20.00 | -15.28 | 117.18 | -62.01 | 109.19 | 0.9037 | -370.8 | 999999 | |
| 3.72 | -20.00 | 4.35 | -20.00 | -15.94 | 116.76 | -62.43 | 109.80 | 0.9077 | -326.8 | 999999 | |
| 1.21 | -20.00 | 1.40 | -20.00 | -15.61 | 116.94 | -62.25 | 109.49 | 0.9060 | -241.9 | 999999 | |
| 0.26 | -20.00 | 0.30 | -20.00 | -15.43 | 116.83 | -62.36 | 109.27 | 0.9064 | 305.3 | 999999 | |
| 2.59 | 5.53 | 2.95 | 6.30 | -14.01 | 117.15 | -62.04 | 107.80 | 0.9019 | -617.6 | -548.2 | |
| 7.43 | 101.49 | 8.08 | 111.75 | -10.87 | 117.86 | -61.32 | 104.52 | 0.8919 | 803.0 | 131.9 | |
| 0.00 | 2.07 | 0.00 | 2.47 | -14.95 | 116.07 | -63.12 | 108.58 | 0.9109 | -382.0 | -354.0 | |
| 0.00 | 1.82 | 0.00 | 2.13 | -14.19 | 116.33 | -62.86 | 107.81 | 0.9080 | 230.0 | 206.9 | |
| 7.78 | -27.00 | 8.61 | -27.00 | -10.94 | 117.32 | -61.86 | 104.48 | 0.8961 | 401.1 | 999999 | |
| 0.00 | 2.77 | 0.00 | 3.56 | -15.65 | 114.10 | -65.09 | 108.91 | 0.9248 | -537.0 | -414.2 | |
| 0.00 | 0.86 | 0.00 | 0.96 | -9.44 | 116.93 | -62.26 | 102.75 | 0.8970 | 427.0 | 370.0 | |
| 0.00 | 1.21 | 0.00 | 1.48 | -10.19 | 114.41 | -64.78 | 103.12 | 0.9160 | 498.0 | 415.6 | |
| 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. | |