SDO HMI 2014-07-05 19:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 118.11 | 699.84 | 63.44 | 376.39 | -19.33 | 256.49 | -0.83 | 177.80 | 0.3894 | 698.7 | 331.4 | |
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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 | 1.27 | 0.00 | 0.70 | -19.75 | 270.29 | 12.97 | 208.38 | 0.4463 | 711.0 | 566.4 | |
| 0.00 | 2.00 | 0.00 | 1.10 | -20.88 | 267.95 | 10.63 | 202.82 | 0.4463 | 784.0 | 584.4 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -23.00 | 267.41 | 10.09 | 199.99 | 0.4735 | 672.0 | 580.2 | |
| 0.00 | 3.09 | 0.00 | 1.69 | -20.66 | 266.15 | 8.83 | 199.47 | 0.4328 | 689.0 | 700.6 | |
| 0.00 | 1.54 | 0.00 | 0.85 | -21.10 | 266.18 | 8.86 | 199.17 | 0.4394 | 706.0 | 584.1 | |
| 0.00 | 2.09 | 0.00 | 1.12 | -17.71 | 264.83 | 7.51 | 199.14 | 0.3816 | -893.0 | -811.7 | |
| 0.00 | 0.73 | 0.00 | 0.41 | -23.93 | 265.11 | 7.79 | 195.14 | 0.4764 | 710.0 | 536.6 | |
| 0.00 | 1.00 | 0.00 | 0.57 | -24.69 | 264.85 | 7.53 | 194.23 | 0.4865 | 646.0 | 465.6 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -21.85 | 264.20 | 6.88 | 194.65 | 0.4416 | 661.0 | 557.2 | |
| 0.00 | 1.54 | 0.00 | 0.86 | -23.13 | 263.56 | 6.24 | 192.65 | 0.4587 | 737.0 | 682.5 | |
| 0.00 | 1.91 | 0.00 | 1.06 | -22.52 | 263.54 | 6.22 | 192.92 | 0.4493 | 861.0 | 670.7 | |
| 0.00 | 0.82 | 0.00 | 0.45 | -21.54 | 263.23 | 5.91 | 192.83 | 0.4332 | 488.0 | 376.0 | |
| 0.00 | 0.73 | 0.00 | 0.40 | -21.20 | 263.22 | 5.90 | 192.99 | 0.4280 | 608.0 | 491.0 | |
| 0.00 | 1.09 | 0.00 | 0.59 | -18.75 | 263.06 | 5.74 | 194.15 | 0.3894 | 795.0 | 690.5 | |
| 9.62 | 29.78 | 5.26 | 16.28 | -21.03 | 262.72 | 5.40 | 192.01 | 0.4237 | 1028.5 | 366.4 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -23.57 | 262.82 | 5.50 | 190.97 | 0.4629 | -801.0 | -548.7 | |
| 0.00 | 1.91 | 0.00 | 1.05 | -22.55 | 262.77 | 5.45 | 191.37 | 0.4472 | 762.0 | 484.3 | |
| 1.63 | -15.00 | 0.89 | -15.00 | -20.93 | 262.39 | 5.07 | 191.35 | 0.4210 | 949.1 | 999999 | |
| 0.00 | 0.91 | 0.00 | 0.48 | -16.39 | 262.23 | 4.91 | 193.66 | 0.3490 | -734.0 | -570.4 | |
| 0.00 | 1.09 | 0.00 | 0.59 | -20.89 | 262.03 | 4.71 | 190.58 | 0.4194 | 792.0 | 670.6 | |
| 0.00 | 1.45 | 0.00 | 0.79 | -20.69 | 261.79 | 4.47 | 190.15 | 0.4156 | 896.0 | 721.1 | |
| 0.00 | 1.00 | 0.00 | 0.54 | -20.99 | 261.73 | 4.41 | 189.89 | 0.4201 | 685.0 | 482.5 | |
| 0.00 | 2.36 | 0.00 | 1.30 | -22.10 | 260.81 | 3.49 | 187.48 | 0.4352 | -766.0 | -754.8 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -22.61 | 260.82 | 3.50 | 187.34 | 0.4431 | -716.0 | -548.8 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -22.47 | 260.49 | 3.17 | 186.69 | 0.4403 | -637.0 | -534.0 | |
| 0.00 | 2.63 | 0.00 | 1.41 | -19.26 | 260.17 | 2.85 | 186.95 | 0.3889 | -520.0 | -313.6 | |
| 0.00 | 2.00 | 0.00 | 1.09 | -21.02 | 259.94 | 2.62 | 185.90 | 0.4166 | -942.0 | -679.8 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -20.68 | 259.60 | 2.28 | 185.23 | 0.4107 | -895.0 | -771.5 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -21.86 | 259.62 | 2.30 | 185.00 | 0.4293 | 585.0 | 457.5 | |
| 0.00 | 5.27 | 0.00 | 2.87 | -21.15 | 259.22 | 1.90 | 184.26 | 0.4176 | 952.0 | 785.4 | |
| 0.00 | 1.45 | 0.00 | 0.78 | -18.92 | 259.16 | 1.84 | 184.59 | 0.3819 | -605.0 | -436.9 | |
| 0.00 | 0.91 | 0.00 | 0.50 | -22.19 | 258.14 | 0.83 | 181.77 | 0.4332 | -820.0 | -640.8 | |
| 3.18 | 27.96 | 1.75 | 15.36 | -22.32 | 256.56 | -0.76 | 178.39 | 0.4353 | -1079.9 | -643.6 | |
| 0.00 | 0.27 | 0.00 | 0.15 | -21.68 | 256.04 | -1.28 | 177.20 | 0.4255 | -697.0 | -699.0 | |
| 0.00 | 0.82 | 0.00 | 0.45 | -22.90 | 256.00 | -1.32 | 177.25 | 0.4447 | -507.0 | -368.4 | |
| 97.51 | 556.55 | 52.19 | 297.99 | -18.82 | 255.85 | -1.47 | 176.31 | 0.3798 | 1525.6 | 445.9 | |
| 0.54 | 4.18 | 0.30 | 2.30 | -22.42 | 255.81 | -1.51 | 176.78 | 0.4374 | -829.3 | -760.5 | |
| 1.18 | -37.00 | 0.65 | -37.00 | -22.32 | 255.77 | -1.55 | 176.70 | 0.4358 | -930.1 | 999999 | |
| 0.00 | 1.91 | 0.00 | 1.06 | -23.10 | 255.60 | -1.72 | 176.45 | 0.4482 | -846.0 | -578.3 | |
| 0.00 | 1.63 | 0.00 | 0.91 | -23.24 | 255.53 | -1.79 | 176.33 | 0.4504 | -872.0 | -827.2 | |
| 0.00 | 1.63 | 0.00 | 0.90 | -21.82 | 254.93 | -2.39 | 174.79 | 0.4288 | 601.0 | 456.9 | |
| 0.00 | 0.91 | 0.00 | 0.50 | -22.73 | 254.88 | -2.44 | 174.89 | 0.4433 | -744.0 | -556.1 | |
| 0.00 | 0.36 | 0.00 | 0.20 | -23.48 | 254.59 | -2.72 | 174.48 | 0.4553 | -565.0 | -650.0 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -22.66 | 254.55 | -2.77 | 174.19 | 0.4427 | -898.0 | -739.9 | |
| 0.00 | 1.63 | 0.00 | 0.89 | -20.84 | 254.52 | -2.80 | 173.64 | 0.4141 | 852.0 | 639.7 | |
| 0.00 | 1.91 | 0.00 | 1.04 | -21.31 | 253.76 | -3.56 | 172.10 | 0.4231 | -978.0 | -864.1 | |
| 0.00 | 2.27 | 0.00 | 1.22 | -19.55 | 253.60 | -3.72 | 171.08 | 0.3955 | 738.0 | 701.0 | |
| 0.00 | 2.36 | 0.00 | 1.27 | -19.58 | 253.21 | -4.11 | 170.18 | 0.3971 | 720.0 | 538.9 | |
| 0.00 | 0.82 | 0.00 | 0.44 | -18.99 | 252.68 | -4.64 | 168.62 | 0.3893 | 619.0 | 491.1 | |
| 0.00 | 1.73 | 0.00 | 0.92 | -17.91 | 252.39 | -4.93 | 167.29 | 0.3731 | -968.0 | -829.4 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -23.39 | 252.10 | -5.22 | 169.48 | 0.4593 | -730.0 | -592.5 | |
| 0.00 | 2.27 | 0.00 | 1.23 | -19.95 | 251.61 | -5.71 | 166.69 | 0.4081 | -818.0 | -618.5 | |
| 4.09 | 9.17 | 2.20 | 4.95 | -19.29 | 251.60 | -5.72 | 166.27 | 0.3978 | -968.1 | -458.9 | |
| 0.36 | 1.18 | 0.20 | 0.63 | -18.80 | 251.30 | -6.02 | 165.23 | 0.3913 | -979.0 | -745.8 | |
| 0.00 | 1.36 | 0.00 | 0.78 | -25.26 | 246.09 | -11.23 | 159.77 | 0.5113 | -752.0 | -592.0 | |
| 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. | |