SDO HMI 2011-11-18 20:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 99.88 | 329.90 | 104.65 | 341.91 | -15.80 | 266.72 | -59.31 | 109.55 | 0.8791 | 96.4 | -25.0 | |
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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 | 1.29 | 0.00 | 1.20 | -16.28 | 270.57 | -55.46 | 111.00 | 0.8491 | 639.0 | 616.7 | |
| 25.31 | 114.20 | 23.94 | 108.32 | -16.71 | 270.11 | -55.92 | 111.36 | 0.8539 | 801.4 | 230.6 | |
| 2.66 | -2.00 | 2.57 | -2.00 | -17.05 | 269.39 | -56.64 | 111.55 | 0.8606 | 318.0 | 999999 | |
| 1.12 | 2.15 | 1.11 | 2.13 | -17.71 | 268.49 | -57.54 | 112.06 | 0.8693 | 420.4 | 335.8 | |
| 6.01 | 9.35 | 6.04 | 9.43 | -17.32 | 268.04 | -57.99 | 111.51 | 0.8721 | 442.7 | -84.0 | |
| 3.26 | 45.90 | 3.40 | 48.44 | -16.80 | 266.68 | -59.35 | 110.61 | 0.8818 | -731.9 | -460.9 | |
| 9.78 | -6.00 | 10.36 | -6.00 | -16.64 | 266.15 | -59.88 | 110.31 | 0.8856 | -656.4 | 999999 | |
| 16.56 | 48.22 | 16.79 | 48.77 | -13.54 | 266.91 | -59.12 | 107.02 | 0.8746 | 677.1 | 313.8 | |
| 0.00 | 0.94 | 0.00 | 1.02 | -16.70 | 265.43 | -60.60 | 110.21 | 0.8912 | -319.0 | -310.9 | |
| 0.00 | 1.29 | 0.00 | 1.40 | -16.89 | 265.26 | -60.77 | 110.39 | 0.8927 | -305.0 | -193.9 | |
| 0.00 | 0.69 | 0.00 | 0.75 | -17.02 | 265.19 | -60.84 | 110.51 | 0.8935 | -139.0 | -155.6 | |
| 0.00 | 3.52 | 0.00 | 3.65 | -14.46 | 266.34 | -59.69 | 107.92 | 0.8806 | 382.0 | 272.1 | |
| 0.00 | 2.49 | 0.00 | 2.60 | -14.80 | 266.18 | -59.85 | 108.28 | 0.8824 | -308.0 | -262.1 | |
| 1.97 | 23.42 | 2.14 | 25.59 | -16.18 | 265.19 | -60.84 | 109.59 | 0.8921 | -581.0 | -463.9 | |
| 2.83 | 11.50 | 3.15 | 12.87 | -16.98 | 264.69 | -61.34 | 110.36 | 0.8970 | 453.8 | 130.4 | |
| 1.46 | -14.00 | 1.61 | -14.00 | -16.28 | 264.81 | -61.21 | 109.62 | 0.8950 | -388.0 | 999999 | |
| 1.89 | -14.00 | 2.06 | -14.00 | -16.00 | 264.97 | -61.06 | 109.34 | 0.8935 | -459.4 | 999999 | |
| 1.03 | -14.00 | 1.13 | -14.00 | -15.88 | 264.90 | -61.13 | 109.19 | 0.8938 | 166.8 | 999999 | |
| 1.54 | -15.00 | 1.74 | -15.00 | -16.90 | 264.28 | -61.75 | 110.18 | 0.8999 | 432.3 | 999999 | |
| 0.00 | 0.51 | 0.00 | 0.54 | -13.56 | 265.68 | -60.35 | 106.79 | 0.8844 | 457.0 | 427.8 | |
| 0.00 | 0.34 | 0.00 | 0.40 | -17.76 | 263.16 | -62.87 | 110.88 | 0.9090 | 260.0 | 253.8 | |
| 3.60 | 4.89 | 3.81 | 5.17 | -13.17 | 265.47 | -60.55 | 106.31 | 0.8854 | 360.4 | 219.7 | |
| 0.00 | 2.23 | 0.00 | 2.37 | -13.45 | 265.35 | -60.67 | 106.60 | 0.8868 | 277.0 | 208.5 | |
| 1.12 | 2.23 | 1.26 | 2.53 | -16.13 | 263.91 | -62.12 | 109.27 | 0.9013 | -393.2 | -435.8 | |
| 0.00 | 1.89 | 0.00 | 2.06 | -14.43 | 264.72 | -61.31 | 107.56 | 0.8930 | 443.0 | 354.7 | |
| 0.94 | 1.80 | 1.09 | 2.08 | -15.94 | 263.35 | -62.68 | 108.95 | 0.9051 | -589.6 | -577.7 | |
| 0.00 | 3.09 | 0.00 | 3.66 | -16.77 | 262.80 | -63.23 | 109.74 | 0.9100 | -575.0 | -456.0 | |
| 5.15 | 5.83 | 6.29 | 7.12 | -17.55 | 262.10 | -63.93 | 110.44 | 0.9158 | -488.3 | -455.2 | |
| 0.00 | 1.12 | 0.00 | 1.31 | -16.08 | 262.93 | -63.10 | 109.02 | 0.9082 | -306.0 | -284.7 | |
| 0.00 | 1.80 | 0.00 | 2.02 | -13.75 | 263.87 | -62.16 | 106.66 | 0.8984 | -564.0 | -548.8 | |
| 0.00 | 1.03 | 0.00 | 1.31 | -17.59 | 261.05 | -64.98 | 110.28 | 0.9226 | -428.0 | -365.8 | |
| 9.10 | 26.17 | 10.52 | 30.32 | -13.97 | 262.96 | -63.07 | 106.73 | 0.9053 | -625.9 | -292.9 | |
| 0.00 | 2.83 | 0.00 | 3.44 | -15.35 | 261.81 | -64.22 | 108.01 | 0.9149 | -508.0 | -487.4 | |
| 0.00 | 0.43 | 0.00 | 0.53 | -14.90 | 261.49 | -64.54 | 107.47 | 0.9165 | -522.0 | -463.6 | |
| 4.55 | 8.75 | 5.64 | 10.88 | -15.25 | 261.21 | -64.81 | 107.80 | 0.9187 | -392.0 | -124.7 | |
| 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. | |