SDO HMI 2014-07-04 21:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 128.18 | 736.88 | 70.52 | 406.15 | -19.24 | 256.77 | -12.67 | 151.58 | 0.4377 | 663.7 | 303.9 | |
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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 | 2.81 | 0.00 | 1.53 | -20.94 | 268.05 | -1.40 | 176.82 | 0.4122 | 902.0 | 730.0 | |
| 0.00 | 1.00 | 0.00 | 0.54 | -20.67 | 266.13 | -3.32 | 172.40 | 0.4109 | 707.0 | 519.5 | |
| 0.00 | 1.09 | 0.00 | 0.59 | -21.24 | 265.95 | -3.49 | 172.20 | 0.4203 | 714.0 | 482.5 | |
| 0.00 | 2.18 | 0.00 | 1.18 | -20.47 | 265.87 | -3.57 | 171.74 | 0.4083 | 919.0 | 650.4 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -22.67 | 263.63 | -5.82 | 167.92 | 0.4487 | 848.0 | 778.3 | |
| 0.00 | 1.63 | 0.00 | 0.90 | -22.43 | 263.34 | -6.11 | 167.21 | 0.4461 | 914.0 | 728.6 | |
| 0.00 | 1.63 | 0.00 | 0.90 | -21.46 | 262.95 | -6.49 | 165.87 | 0.4326 | 462.0 | 396.8 | |
| 10.62 | 65.83 | 5.81 | 36.05 | -20.89 | 262.78 | -6.66 | 165.15 | 0.4246 | 1111.5 | 387.6 | |
| 3.81 | -8.00 | 2.09 | -8.00 | -20.96 | 262.42 | -7.03 | 164.42 | 0.4272 | 903.7 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -23.46 | 262.22 | -7.22 | 165.60 | 0.4657 | -867.0 | -669.5 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -20.89 | 262.19 | -7.25 | 163.90 | 0.4272 | 814.0 | 679.3 | |
| 1.00 | -8.00 | 0.55 | -8.00 | -20.72 | 262.07 | -7.38 | 163.53 | 0.4252 | 1056.5 | 999999 | |
| 0.00 | 1.63 | 0.00 | 0.88 | -17.70 | 261.05 | -8.40 | 158.71 | 0.3849 | 831.0 | 664.3 | |
| 0.00 | 4.36 | 0.00 | 2.39 | -20.34 | 260.25 | -9.20 | 159.44 | 0.4286 | -1008.0 | -866.1 | |
| 0.00 | 0.82 | 0.00 | 0.45 | -20.31 | 259.99 | -9.46 | 158.89 | 0.4296 | -850.0 | -727.0 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -20.91 | 259.85 | -9.60 | 159.14 | 0.4392 | -938.0 | -829.5 | |
| 0.00 | 1.82 | 0.00 | 1.00 | -21.01 | 259.61 | -9.84 | 158.76 | 0.4420 | -838.0 | -791.5 | |
| 0.45 | 2.63 | 0.25 | 1.44 | -20.18 | 259.63 | -9.81 | 158.05 | 0.4298 | -1027.8 | -876.0 | |
| 0.00 | 0.82 | 0.00 | 0.45 | -20.71 | 259.56 | -9.88 | 158.40 | 0.4379 | -851.0 | -631.3 | |
| 0.00 | 2.54 | 0.00 | 1.39 | -19.58 | 259.51 | -9.94 | 157.23 | 0.4219 | -1032.0 | -859.6 | |
| 0.00 | 4.72 | 0.00 | 2.58 | -19.82 | 259.26 | -10.18 | 156.96 | 0.4268 | -684.0 | -638.0 | |
| 0.54 | 3.09 | 0.30 | 1.72 | -22.16 | 259.06 | -10.38 | 158.71 | 0.4616 | 765.3 | 644.0 | |
| 0.00 | 2.36 | 0.00 | 1.29 | -19.39 | 259.12 | -10.32 | 156.26 | 0.4215 | -840.0 | -680.5 | |
| 0.00 | 1.18 | 0.00 | 0.66 | -22.64 | 258.35 | -11.09 | 157.83 | 0.4725 | -183.0 | -146.0 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -22.81 | 258.00 | -11.45 | 157.36 | 0.4770 | -605.0 | -424.8 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -22.55 | 257.62 | -11.83 | 156.45 | 0.4756 | -747.0 | -445.6 | |
| 0.00 | 2.81 | 0.00 | 1.57 | -21.60 | 257.63 | -11.81 | 155.59 | 0.4624 | -212.0 | -215.7 | |
| 0.00 | 1.63 | 0.00 | 0.92 | -22.08 | 257.15 | -12.29 | 155.19 | 0.4720 | -961.0 | -806.7 | |
| 0.00 | 1.45 | 0.00 | 0.82 | -22.39 | 256.15 | -13.30 | 153.76 | 0.4830 | -692.0 | -551.6 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -22.70 | 255.77 | -13.67 | 153.45 | 0.4897 | -642.0 | -533.3 | |
| 106.50 | 579.63 | 58.56 | 319.05 | -18.79 | 256.07 | -13.37 | 149.65 | 0.4352 | 1455.6 | 416.4 | |
| 0.00 | 0.82 | 0.00 | 0.46 | -20.85 | 255.65 | -13.79 | 151.31 | 0.4659 | 806.0 | 630.2 | |
| 0.00 | 1.45 | 0.00 | 0.82 | -22.23 | 255.38 | -14.06 | 152.32 | 0.4862 | -371.0 | -370.4 | |
| 0.00 | 1.45 | 0.00 | 0.82 | -22.27 | 255.17 | -14.27 | 152.02 | 0.4882 | -727.0 | -549.3 | |
| 1.27 | 2.72 | 0.72 | 1.55 | -22.81 | 255.05 | -14.40 | 152.37 | 0.4962 | -954.4 | -822.2 | |
| 1.45 | -31.00 | 0.80 | -31.00 | -18.51 | 255.40 | -14.05 | 148.07 | 0.4369 | 1009.4 | 999999 | |
| 0.36 | 8.53 | 0.21 | 4.85 | -22.31 | 254.83 | -14.62 | 151.50 | 0.4912 | -869.8 | -659.7 | |
| 0.00 | 0.64 | 0.00 | 0.36 | -21.94 | 254.87 | -14.58 | 151.17 | 0.4860 | -708.0 | -594.1 | |
| 0.00 | 0.82 | 0.00 | 0.46 | -20.60 | 254.37 | -15.08 | 148.84 | 0.4726 | 644.0 | 484.6 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -20.51 | 254.21 | -15.24 | 148.47 | 0.4726 | 686.0 | 518.5 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -20.25 | 253.93 | -15.51 | 147.70 | 0.4715 | 584.0 | 442.3 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -23.12 | 253.05 | -16.39 | 149.59 | 0.5147 | -883.0 | -667.8 | |
| 0.00 | 1.18 | 0.00 | 0.65 | -18.01 | 253.22 | -16.23 | 143.62 | 0.4499 | -732.0 | -593.5 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -17.92 | 253.06 | -16.39 | 143.22 | 0.4502 | -747.0 | -605.4 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -17.37 | 252.81 | -16.63 | 142.03 | 0.4459 | -845.0 | -614.6 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -18.42 | 252.30 | -17.14 | 142.70 | 0.4633 | -723.0 | -627.9 | |
| 0.00 | 2.45 | 0.00 | 1.38 | -19.45 | 252.09 | -17.35 | 143.75 | 0.4776 | -706.0 | -588.6 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -20.18 | 251.84 | -17.61 | 144.31 | 0.4886 | -805.0 | -740.4 | |
| 2.18 | 7.54 | 1.23 | 4.24 | -18.96 | 251.77 | -17.67 | 142.61 | 0.4747 | -967.5 | -756.3 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -19.32 | 251.70 | -17.75 | 142.98 | 0.4797 | -761.0 | -656.7 | |
| 0.00 | 0.36 | 0.00 | 0.21 | -19.83 | 251.06 | -18.38 | 142.70 | 0.4915 | -196.0 | -318.2 | |
| 0.00 | 1.73 | 0.00 | 0.98 | -18.72 | 250.20 | -19.24 | 139.95 | 0.4870 | -868.0 | -733.5 | |
| 0.00 | 0.64 | 0.00 | 0.39 | -26.07 | 246.50 | -22.94 | 144.22 | 0.6010 | -587.0 | -470.3 | |
| 0.00 | 1.00 | 0.00 | 0.61 | -24.52 | 246.05 | -23.39 | 141.97 | 0.5885 | -662.0 | -586.9 | |
| 0.00 | 1.09 | 0.00 | 0.67 | -24.42 | 245.78 | -23.67 | 141.54 | 0.5899 | -650.0 | -483.2 | |
| 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. | |