SDO HMI 2011-11-23 09:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.07 | 122.24 | 12.59 | 63.98 | -16.80 | 266.12 | -0.05 | 179.85 | 0.3235 | 74.8 | -22.9 | |
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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 | 0.94 | 0.00 | 0.49 | -17.27 | 269.17 | 2.99 | 188.63 | 0.3333 | 837.0 | 650.7 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -18.69 | 269.10 | 2.92 | 187.82 | 0.3561 | 694.0 | 539.2 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -19.45 | 269.05 | 2.87 | 187.40 | 0.3684 | 765.0 | 610.2 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -16.24 | 268.53 | 2.36 | 187.23 | 0.3149 | 872.0 | 679.7 | |
| 0.00 | 1.71 | 0.00 | 0.91 | -18.63 | 268.50 | 2.32 | 186.26 | 0.3539 | 749.0 | 620.9 | |
| 0.00 | 1.20 | 0.00 | 0.62 | -16.02 | 268.25 | 2.08 | 186.46 | 0.3107 | 701.0 | 558.5 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -18.53 | 268.16 | 1.98 | 185.37 | 0.3518 | 710.0 | 568.9 | |
| 16.37 | 53.56 | 8.57 | 28.04 | -16.96 | 267.64 | 1.47 | 184.34 | 0.3252 | 1158.8 | 424.5 | |
| 0.00 | 4.11 | 0.00 | 2.11 | -13.24 | 267.25 | 1.08 | 184.01 | 0.2627 | 866.0 | 727.6 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -15.40 | 267.11 | 0.93 | 183.03 | 0.2988 | 873.0 | 684.6 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -18.69 | 266.50 | 0.33 | 180.88 | 0.3529 | 840.0 | 700.8 | |
| 0.00 | 1.46 | 0.00 | 0.77 | -18.28 | 265.88 | -0.30 | 179.18 | 0.3461 | 726.0 | 623.9 | |
| 0.00 | 1.37 | 0.00 | 0.72 | -16.49 | 265.79 | -0.39 | 178.82 | 0.3166 | -807.0 | -596.9 | |
| 1.71 | 16.37 | 0.89 | 8.53 | -16.39 | 265.48 | -0.70 | 177.87 | 0.3152 | -991.8 | -539.8 | |
| 3.51 | -14.00 | 1.83 | -14.00 | -16.21 | 265.33 | -0.85 | 177.37 | 0.3122 | -1024.8 | 999999 | |
| 0.34 | 1.11 | 0.18 | 0.57 | -14.32 | 265.21 | -0.97 | 176.65 | 0.2807 | 854.8 | 731.1 | |
| 1.11 | 10.28 | 0.58 | 5.37 | -16.61 | 264.89 | -1.28 | 176.12 | 0.3193 | -1084.4 | -798.4 | |
| 1.03 | -17.00 | 0.54 | -17.00 | -16.49 | 264.55 | -1.62 | 175.07 | 0.3177 | -886.4 | 999999 | |
| 0.00 | 1.97 | 0.00 | 1.03 | -16.99 | 263.40 | -2.77 | 171.86 | 0.3281 | -903.0 | -797.9 | |
| 0.00 | 1.37 | 0.00 | 0.73 | -19.04 | 263.34 | -2.84 | 172.53 | 0.3616 | -683.0 | -598.4 | |
| 0.00 | 3.43 | 0.00 | 1.79 | -16.49 | 263.22 | -2.95 | 171.09 | 0.3204 | -1103.0 | -956.1 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -18.85 | 263.09 | -3.09 | 171.81 | 0.3591 | -723.0 | -543.1 | |
| 0.00 | 2.14 | 0.00 | 1.12 | -17.02 | 263.06 | -3.12 | 170.89 | 0.3295 | -910.0 | -726.1 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -16.43 | 263.01 | -3.17 | 170.42 | 0.3199 | -787.0 | -627.1 | |
| 0.00 | 4.28 | 0.00 | 2.24 | -16.21 | 262.89 | -3.29 | 169.94 | 0.3167 | -648.0 | -647.0 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -17.81 | 262.86 | -3.32 | 170.72 | 0.3428 | -917.0 | -699.7 | |
| 0.00 | 0.60 | 0.00 | 0.31 | -17.12 | 262.78 | -3.40 | 170.13 | 0.3318 | -778.0 | -581.4 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -18.88 | 262.53 | -3.65 | 170.35 | 0.3611 | -723.0 | -577.3 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -19.17 | 261.99 | -4.19 | 169.12 | 0.3672 | -655.0 | -609.6 | |
| 0.00 | 0.94 | 0.00 | 0.50 | -19.17 | 261.74 | -4.44 | 168.48 | 0.3680 | -752.0 | -606.1 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -11.90 | 261.83 | -4.35 | 162.70 | 0.2505 | -705.0 | -543.0 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -21.02 | 260.50 | -5.67 | 166.66 | 0.4015 | -731.0 | -484.9 | |
| 0.00 | 1.54 | 0.00 | 0.80 | -15.16 | 260.63 | -5.55 | 162.33 | 0.3088 | -844.0 | -610.1 | |
| 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. | |