SDO HMI 2014-07-13 22:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.09 | 116.52 | 2.20 | 63.59 | -20.10 | 148.35 | -1.43 | 177.25 | 0.4193 | 184.9 | 215.5 | |
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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 | 1.18 | 0.00 | 0.63 | -10.71 | 164.47 | 14.69 | 224.36 | 0.3580 | 700.0 | 529.0 | |
| 0.00 | 1.09 | 0.00 | 0.56 | -7.77 | 158.94 | 9.16 | 217.41 | 0.2609 | 732.0 | 545.6 | |
| 0.00 | 1.18 | 0.00 | 0.65 | -21.30 | 157.83 | 8.05 | 196.89 | 0.4509 | 666.0 | 510.2 | |
| 0.00 | 1.45 | 0.00 | 0.81 | -22.68 | 156.87 | 7.09 | 194.16 | 0.4676 | 315.0 | 439.6 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -20.57 | 156.54 | 6.76 | 194.76 | 0.4346 | 845.0 | 689.0 | |
| 0.00 | 1.82 | 0.00 | 1.00 | -20.40 | 156.17 | 6.40 | 194.10 | 0.4305 | 886.0 | 763.3 | |
| 0.00 | 2.45 | 0.00 | 1.34 | -20.63 | 155.20 | 5.42 | 191.91 | 0.4306 | 897.0 | 734.9 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -20.79 | 154.85 | 5.07 | 191.07 | 0.4320 | 879.0 | 790.2 | |
| 0.00 | 1.54 | 0.00 | 0.85 | -21.43 | 154.18 | 4.40 | 189.38 | 0.4400 | 688.0 | 556.1 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -17.70 | 153.99 | 4.21 | 190.62 | 0.3808 | 863.0 | 750.4 | |
| 0.00 | 1.00 | 0.00 | 0.53 | -17.43 | 153.82 | 4.04 | 190.34 | 0.3761 | 896.0 | 670.5 | |
| 0.00 | 0.82 | 0.00 | 0.46 | -23.85 | 153.59 | 3.81 | 187.36 | 0.4759 | 617.0 | 583.0 | |
| 0.00 | 0.64 | 0.00 | 0.35 | -22.10 | 152.19 | 2.41 | 185.03 | 0.4465 | 714.0 | 570.1 | |
| 0.00 | 2.18 | 0.00 | 1.16 | -17.62 | 151.77 | 2.00 | 185.11 | 0.3747 | 886.0 | 686.3 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -18.31 | 151.75 | 1.97 | 184.88 | 0.3858 | 944.0 | 850.0 | |
| 0.00 | 2.63 | 0.00 | 1.41 | -17.85 | 151.71 | 1.94 | 184.90 | 0.3783 | 698.0 | 620.6 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -17.13 | 151.67 | 1.90 | 184.97 | 0.3665 | 918.0 | 643.7 | |
| 0.00 | 1.18 | 0.00 | 0.65 | -22.26 | 151.30 | 1.52 | 183.16 | 0.4481 | 714.0 | 509.3 | |
| 0.00 | 1.82 | 0.00 | 1.00 | -22.02 | 151.20 | 1.42 | 182.98 | 0.4442 | 705.0 | 637.8 | |
| 0.00 | 2.63 | 0.00 | 1.40 | -17.32 | 150.91 | 1.13 | 182.94 | 0.3688 | 1051.0 | 830.5 | |
| 1.27 | 3.45 | 0.67 | 1.83 | -16.73 | 150.84 | 1.07 | 182.85 | 0.3592 | 1092.5 | 933.3 | |
| 0.00 | 0.45 | 0.00 | 0.25 | -22.12 | 150.41 | 0.63 | 181.33 | 0.4453 | 761.0 | 655.6 | |
| 0.00 | 2.81 | 0.00 | 1.53 | -20.07 | 149.79 | 0.01 | 180.03 | 0.4126 | 790.0 | 620.1 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -20.90 | 149.30 | -0.48 | 178.95 | 0.4261 | 661.0 | 406.3 | |
| 0.00 | 1.72 | 0.00 | 0.94 | -20.10 | 149.24 | -0.54 | 178.77 | 0.4133 | 989.0 | 804.3 | |
| 0.00 | 1.27 | 0.00 | 0.67 | -16.50 | 149.19 | -0.59 | 178.41 | 0.3551 | 842.0 | 604.9 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -16.60 | 148.87 | -0.91 | 177.56 | 0.3569 | 801.0 | 635.3 | |
| 0.00 | 0.45 | 0.00 | 0.25 | -22.94 | 148.56 | -1.22 | 177.55 | 0.4584 | 182.0 | 273.0 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -21.11 | 148.06 | -1.72 | 176.25 | 0.4301 | 504.0 | 362.9 | |
| 0.73 | 1.63 | 0.40 | 0.89 | -20.87 | 147.93 | -1.85 | 175.93 | 0.4265 | 686.5 | 568.1 | |
| 0.00 | 3.18 | 0.00 | 1.73 | -20.50 | 147.87 | -1.91 | 175.73 | 0.4207 | 833.0 | 694.8 | |
| 0.00 | 1.72 | 0.00 | 0.96 | -23.22 | 147.73 | -2.05 | 175.92 | 0.4634 | 583.0 | 391.6 | |
| 0.00 | 1.00 | 0.00 | 0.54 | -19.57 | 147.36 | -2.41 | 174.38 | 0.4065 | 857.0 | 639.4 | |
| 0.00 | 1.72 | 0.00 | 0.94 | -20.10 | 147.03 | -2.75 | 173.76 | 0.4156 | 735.0 | 659.1 | |
| 2.09 | 9.17 | 1.13 | 4.98 | -19.87 | 146.97 | -2.81 | 173.55 | 0.4120 | 984.7 | 906.0 | |
| 0.00 | 18.79 | 0.00 | 10.26 | -20.47 | 146.73 | -3.05 | 173.19 | 0.4220 | 336.0 | 399.8 | |
| 0.00 | 1.63 | 0.00 | 0.89 | -19.67 | 146.49 | -3.29 | 172.39 | 0.4098 | 745.0 | 676.4 | |
| 0.00 | 2.90 | 0.00 | 1.60 | -21.58 | 146.21 | -3.56 | 172.43 | 0.4404 | -903.0 | -791.8 | |
| 0.00 | 4.08 | 0.00 | 2.24 | -20.84 | 145.74 | -4.03 | 171.17 | 0.4299 | -1094.0 | -892.2 | |
| 0.00 | 1.63 | 0.00 | 0.89 | -20.64 | 145.68 | -4.09 | 170.96 | 0.4269 | -773.0 | -615.4 | |
| 0.00 | 1.45 | 0.00 | 0.79 | -19.81 | 145.51 | -4.27 | 170.23 | 0.4143 | -744.0 | -617.1 | |
| 0.00 | 1.54 | 0.00 | 0.83 | -18.21 | 145.49 | -4.29 | 169.44 | 0.3892 | -1001.0 | -854.7 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -20.95 | 145.32 | -4.46 | 170.29 | 0.4326 | -886.0 | -705.4 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -20.74 | 145.16 | -4.62 | 169.87 | 0.4299 | -743.0 | -481.1 | |
| 0.00 | 1.54 | 0.00 | 0.83 | -18.25 | 145.20 | -4.58 | 168.76 | 0.3907 | -934.0 | -812.6 | |
| 0.00 | 2.45 | 0.00 | 1.32 | -18.41 | 145.13 | -4.65 | 168.69 | 0.3935 | -693.0 | -664.8 | |
| 0.00 | 1.72 | 0.00 | 0.95 | -21.25 | 145.01 | -4.77 | 169.78 | 0.4382 | -682.0 | -544.1 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -21.35 | 144.58 | -5.20 | 168.92 | 0.4410 | -856.0 | -677.9 | |
| 0.00 | 2.09 | 0.00 | 1.17 | -22.85 | 144.49 | -5.29 | 169.41 | 0.4642 | -833.0 | -597.4 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -22.68 | 144.30 | -5.48 | 168.96 | 0.4622 | -842.0 | -731.4 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -21.97 | 144.29 | -5.49 | 168.62 | 0.4513 | -783.0 | -624.5 | |
| 0.00 | 0.82 | 0.00 | 0.45 | -21.90 | 143.70 | -6.08 | 167.40 | 0.4522 | -1002.0 | -883.1 | |
| 0.00 | 1.18 | 0.00 | 0.66 | -21.94 | 143.50 | -6.28 | 167.02 | 0.4535 | -784.0 | -590.3 | |
| 0.00 | 1.18 | 0.00 | 0.66 | -23.38 | 143.27 | -6.51 | 167.31 | 0.4759 | -528.0 | -471.2 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -22.66 | 143.30 | -6.48 | 167.01 | 0.4650 | -386.0 | -526.4 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -21.91 | 142.74 | -7.04 | 165.50 | 0.4559 | -647.0 | -554.6 | |
| 0.00 | 0.82 | 0.00 | 0.45 | -21.48 | 141.57 | -8.20 | 162.94 | 0.4544 | -738.0 | -571.8 | |
| 0.00 | 1.91 | 0.00 | 1.06 | -21.82 | 141.12 | -8.65 | 162.31 | 0.4615 | -757.0 | -614.9 | |
| 0.00 | 0.91 | 0.00 | 0.53 | -24.43 | 136.24 | -13.54 | 155.93 | 0.5248 | -483.0 | -511.4 | |
| 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. | |