SDO HMI 2014-07-13 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 |
| 6.71 | 111.16 | 3.66 | 60.98 | -20.19 | 147.41 | -4.03 | 171.78 | 0.4260 | 80.6 | 181.1 | |
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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 | 1.45 | 0.00 | 0.81 | -22.71 | 156.81 | 5.37 | 190.81 | 0.4620 | 734.0 | 591.1 | |
| 0.00 | 3.81 | 0.00 | 2.08 | -20.41 | 156.11 | 4.67 | 190.39 | 0.4245 | 788.0 | 709.0 | |
| 0.00 | 0.45 | 0.00 | 0.25 | -20.50 | 155.82 | 4.38 | 189.72 | 0.4252 | 477.0 | 512.8 | |
| 0.00 | 0.82 | 0.00 | 0.45 | -20.33 | 155.36 | 3.91 | 188.78 | 0.4214 | 815.0 | 636.1 | |
| 0.00 | 2.72 | 0.00 | 1.49 | -20.60 | 155.20 | 3.76 | 188.33 | 0.4252 | 829.0 | 707.5 | |
| 0.00 | 0.36 | 0.00 | 0.20 | -21.51 | 155.22 | 3.78 | 188.06 | 0.4395 | 277.0 | 438.2 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -20.87 | 154.85 | 3.41 | 187.47 | 0.4286 | 878.0 | 752.5 | |
| 0.00 | 2.09 | 0.00 | 1.12 | -17.74 | 154.02 | 2.58 | 186.54 | 0.3772 | 900.0 | 746.9 | |
| 0.00 | 1.27 | 0.00 | 0.68 | -17.02 | 153.98 | 2.53 | 186.67 | 0.3655 | 913.0 | 805.6 | |
| 0.00 | 2.72 | 0.00 | 1.45 | -17.41 | 153.85 | 2.41 | 186.23 | 0.3716 | 815.0 | 734.0 | |
| 0.00 | 0.91 | 0.00 | 0.48 | -17.08 | 153.56 | 2.12 | 185.57 | 0.3658 | 790.0 | 671.7 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -23.90 | 153.58 | 2.14 | 184.15 | 0.4737 | 592.0 | 446.5 | |
| 0.00 | 1.09 | 0.00 | 0.56 | -12.50 | 153.34 | 1.89 | 186.41 | 0.2901 | 734.0 | 581.2 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -22.07 | 152.14 | 0.70 | 181.47 | 0.4443 | 740.0 | 623.6 | |
| 0.00 | 1.54 | 0.00 | 0.83 | -18.32 | 151.78 | 0.34 | 180.83 | 0.3844 | 881.0 | 813.0 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -17.70 | 151.75 | 0.30 | 180.78 | 0.3742 | 862.0 | 740.9 | |
| 0.00 | 1.00 | 0.00 | 0.53 | -17.04 | 151.71 | 0.27 | 180.72 | 0.3635 | 892.0 | 762.0 | |
| 0.00 | 1.54 | 0.00 | 0.85 | -21.90 | 151.09 | -0.35 | 179.26 | 0.4415 | 654.0 | 564.5 | |
| 0.00 | 1.45 | 0.00 | 0.77 | -17.30 | 150.88 | -0.56 | 178.54 | 0.3679 | 949.0 | 856.5 | |
| 1.36 | 3.27 | 0.72 | 1.73 | -16.71 | 150.82 | -0.62 | 178.34 | 0.3583 | 1127.5 | 840.3 | |
| 0.00 | 1.72 | 0.00 | 0.92 | -16.88 | 149.55 | -1.89 | 174.97 | 0.3622 | 741.0 | 509.5 | |
| 0.00 | 2.00 | 0.00 | 1.09 | -20.12 | 149.18 | -2.26 | 174.86 | 0.4148 | 1005.0 | 832.3 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -21.03 | 148.02 | -3.42 | 172.55 | 0.4311 | 618.0 | 491.8 | |
| 0.91 | 2.90 | 0.50 | 1.59 | -20.83 | 147.96 | -3.48 | 172.36 | 0.4281 | 709.0 | 593.0 | |
| 1.00 | 2.36 | 0.55 | 1.29 | -20.49 | 147.87 | -3.57 | 172.05 | 0.4230 | 869.2 | 743.7 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -19.49 | 147.41 | -4.03 | 170.63 | 0.4084 | 878.0 | 668.0 | |
| 1.45 | 21.15 | 0.79 | 11.53 | -19.86 | 146.98 | -4.46 | 169.81 | 0.4153 | 944.5 | 624.6 | |
| 0.00 | 0.27 | 0.00 | 0.15 | -20.56 | 146.93 | -4.52 | 170.01 | 0.4265 | 726.0 | 755.3 | |
| 0.00 | 6.53 | 0.00 | 3.58 | -20.60 | 146.53 | -4.91 | 169.17 | 0.4282 | 193.0 | 153.6 | |
| 0.00 | 1.54 | 0.00 | 0.84 | -19.63 | 146.53 | -4.91 | 168.70 | 0.4131 | 908.0 | 732.1 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -21.61 | 146.33 | -5.11 | 169.22 | 0.4444 | -611.0 | -511.2 | |
| 0.00 | 2.18 | 0.00 | 1.20 | -21.47 | 146.24 | -5.20 | 168.97 | 0.4426 | -924.0 | -723.9 | |
| 0.00 | 1.63 | 0.00 | 0.90 | -21.24 | 146.25 | -5.19 | 168.87 | 0.4389 | -679.0 | -546.8 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -21.11 | 145.83 | -5.61 | 167.93 | 0.4382 | -594.0 | -494.6 | |
| 0.00 | 1.45 | 0.00 | 0.79 | -20.40 | 145.79 | -5.65 | 167.48 | 0.4275 | -651.0 | -439.3 | |
| 1.54 | 3.09 | 0.85 | 1.70 | -20.84 | 145.71 | -5.73 | 167.54 | 0.4345 | -1012.2 | -869.6 | |
| 0.00 | 1.54 | 0.00 | 0.85 | -20.64 | 145.65 | -5.79 | 167.31 | 0.4316 | -819.0 | -632.6 | |
| 0.00 | 1.27 | 0.00 | 0.69 | -19.73 | 145.49 | -5.95 | 166.45 | 0.4183 | -843.0 | -694.9 | |
| 0.00 | 2.81 | 0.00 | 1.52 | -18.27 | 145.48 | -5.96 | 165.50 | 0.3957 | -926.0 | -791.7 | |
| 0.00 | 2.27 | 0.00 | 1.22 | -18.28 | 145.12 | -6.32 | 164.68 | 0.3972 | -982.0 | -810.7 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -21.35 | 144.60 | -6.84 | 165.55 | 0.4464 | -803.0 | -643.0 | |
| 0.00 | 1.91 | 0.00 | 1.03 | -18.38 | 144.67 | -6.77 | 163.71 | 0.4008 | -851.0 | -649.0 | |
| 0.00 | 0.82 | 0.00 | 0.46 | -22.58 | 144.37 | -7.07 | 165.82 | 0.4657 | -489.0 | -473.2 | |
| 0.00 | 0.91 | 0.00 | 0.49 | -18.74 | 144.52 | -6.92 | 163.65 | 0.4070 | -698.0 | -493.3 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -22.30 | 144.12 | -7.32 | 165.17 | 0.4626 | -810.0 | -657.0 | |
| 0.00 | 1.45 | 0.00 | 0.81 | -22.34 | 143.89 | -7.56 | 164.74 | 0.4641 | -803.0 | -668.7 | |
| 0.45 | 1.63 | 0.25 | 0.91 | -21.87 | 143.68 | -7.76 | 164.05 | 0.4579 | -1000.4 | -864.7 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -22.86 | 143.29 | -8.15 | 163.94 | 0.4742 | -673.0 | -565.8 | |
| 0.00 | 1.45 | 0.00 | 0.83 | -23.87 | 142.11 | -9.33 | 162.47 | 0.4941 | -200.0 | -222.3 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -21.35 | 141.59 | -9.85 | 159.66 | 0.4604 | -681.0 | -603.5 | |
| 0.00 | 1.45 | 0.00 | 0.81 | -21.82 | 141.42 | -10.02 | 159.73 | 0.4681 | -756.0 | -518.3 | |
| 0.00 | 1.82 | 0.00 | 1.02 | -21.69 | 141.07 | -10.37 | 158.97 | 0.4682 | -725.0 | -583.2 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -22.46 | 134.00 | -17.44 | 148.12 | 0.5264 | -592.0 | -439.2 | |
| 0.00 | 1.00 | 0.00 | 0.66 | -28.34 | 125.26 | -26.19 | 143.82 | 0.6601 | -532.0 | -438.9 | |
| 0.00 | 1.82 | 0.00 | 1.13 | -23.50 | 125.92 | -25.52 | 139.21 | 0.6071 | -531.0 | -394.5 | |
| 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. | |