SDO HMI 2011-11-18 19:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 91.96 | 339.93 | 97.26 | 357.46 | -15.80 | 266.76 | -59.82 | 109.44 | 0.8832 | 89.9 | -23.8 | |
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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 | 4.12 | 0.00 | 3.88 | -16.20 | 270.66 | -55.92 | 110.78 | 0.8528 | 543.0 | 511.8 | |
| 22.14 | 115.40 | 21.25 | 111.22 | -16.69 | 270.11 | -56.47 | 111.20 | 0.8585 | 791.2 | 222.8 | |
| 4.63 | -2.00 | 4.55 | -2.00 | -17.06 | 269.36 | -57.22 | 111.42 | 0.8654 | 281.9 | 999999 | |
| 0.00 | 2.75 | 0.00 | 2.77 | -17.75 | 268.55 | -58.03 | 111.99 | 0.8733 | 446.0 | 382.0 | |
| 0.00 | 0.77 | 0.00 | 0.80 | -17.90 | 267.87 | -58.71 | 111.99 | 0.8789 | 161.0 | 135.9 | |
| 5.83 | 8.41 | 5.96 | 8.60 | -17.33 | 267.99 | -58.59 | 111.38 | 0.8769 | 448.0 | 115.1 | |
| 2.49 | 49.08 | 2.63 | 52.52 | -16.79 | 266.75 | -59.83 | 110.48 | 0.8855 | -757.0 | -462.4 | |
| 12.61 | -7.00 | 13.55 | -7.00 | -16.65 | 266.20 | -60.38 | 110.21 | 0.8895 | -640.4 | 999999 | |
| 0.00 | 2.14 | 0.00 | 2.38 | -16.84 | 265.33 | -61.26 | 110.23 | 0.8962 | -305.0 | -246.1 | |
| 0.00 | 0.69 | 0.00 | 0.69 | -12.56 | 267.31 | -59.27 | 105.88 | 0.8743 | 123.0 | 156.0 | |
| 15.44 | 53.02 | 15.95 | 54.57 | -13.56 | 266.85 | -59.73 | 106.91 | 0.8795 | 655.9 | 317.4 | |
| 0.86 | 8.92 | 0.90 | 9.45 | -14.50 | 266.38 | -60.20 | 107.87 | 0.8847 | 193.2 | -114.8 | |
| 0.00 | 1.97 | 0.00 | 2.16 | -16.15 | 265.57 | -61.01 | 109.52 | 0.8933 | -592.0 | -550.8 | |
| 0.43 | -11.00 | 0.44 | -11.00 | -13.10 | 266.80 | -59.78 | 106.39 | 0.8793 | 393.4 | 999999 | |
| 1.37 | -11.00 | 1.43 | -11.00 | -13.76 | 266.52 | -60.06 | 107.07 | 0.8824 | -128.7 | 999999 | |
| 0.94 | -12.00 | 1.00 | -12.00 | -14.36 | 266.20 | -60.38 | 107.67 | 0.8858 | 194.5 | 999999 | |
| 2.14 | 11.07 | 2.43 | 12.63 | -16.99 | 264.65 | -61.93 | 110.25 | 0.9013 | 444.9 | 140.2 | |
| 1.72 | 21.96 | 1.93 | 24.47 | -16.30 | 264.77 | -61.81 | 109.52 | 0.8994 | -411.1 | -407.6 | |
| 1.63 | -17.00 | 1.87 | -17.00 | -16.85 | 264.26 | -62.32 | 110.02 | 0.9038 | 417.3 | 999999 | |
| 0.00 | 1.54 | 0.00 | 1.86 | -17.75 | 263.09 | -63.49 | 110.74 | 0.9131 | 288.0 | 250.4 | |
| 3.35 | 4.38 | 3.60 | 4.71 | -13.19 | 265.46 | -61.13 | 106.22 | 0.8899 | 352.6 | 247.8 | |
| 1.29 | 2.14 | 1.49 | 2.48 | -16.09 | 263.96 | -62.62 | 109.12 | 0.9049 | -338.9 | -433.1 | |
| 0.00 | 1.03 | 0.00 | 1.15 | -14.48 | 264.60 | -61.98 | 107.49 | 0.8980 | 292.0 | 321.0 | |
| 0.00 | 1.97 | 0.00 | 2.38 | -16.72 | 262.89 | -63.69 | 109.60 | 0.9130 | -545.0 | -432.4 | |
| 0.00 | 1.37 | 0.00 | 1.62 | -15.96 | 263.21 | -63.37 | 108.84 | 0.9099 | -639.0 | -548.9 | |
| 4.63 | 5.58 | 5.77 | 6.95 | -17.57 | 262.06 | -64.52 | 110.35 | 0.9196 | -483.3 | -458.6 | |
| 0.00 | 1.03 | 0.00 | 1.23 | -16.10 | 262.92 | -63.66 | 108.93 | 0.9121 | -334.0 | -306.8 | |
| 0.00 | 1.03 | 0.00 | 1.17 | -13.77 | 263.88 | -62.70 | 106.58 | 0.9023 | -515.0 | -537.3 | |
| 8.49 | 27.03 | 10.02 | 31.95 | -13.96 | 262.97 | -63.61 | 106.62 | 0.9090 | -657.5 | -281.4 | |
| 0.00 | 1.89 | 0.00 | 2.34 | -15.39 | 261.91 | -64.68 | 107.98 | 0.9180 | -536.0 | -516.9 | |
| 0.00 | 0.77 | 0.00 | 0.96 | -15.15 | 261.83 | -64.75 | 107.71 | 0.9182 | -555.0 | -522.9 | |
| 1.97 | 8.75 | 2.49 | 11.12 | -15.23 | 261.42 | -65.16 | 107.72 | 0.9210 | -393.7 | -203.9 | |
| 0.00 | 1.12 | 0.00 | 1.40 | -14.85 | 261.49 | -65.09 | 107.33 | 0.9201 | -437.0 | -387.9 | |
| 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. | |