SDO HMI 2014-07-06 06:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 112.39 | 668.21 | 60.60 | 360.29 | -19.23 | 255.94 | 4.69 | 191.21 | 0.3958 | 642.1 | 358.6 | |
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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 | 1.73 | 0.00 | 1.01 | -22.85 | 270.30 | 19.05 | 214.37 | 0.5348 | -715.0 | -534.5 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -20.92 | 268.29 | 17.03 | 213.73 | 0.4948 | 668.0 | 471.8 | |
| 0.00 | 0.73 | 0.00 | 0.41 | -21.38 | 267.62 | 16.37 | 212.16 | 0.4949 | 627.0 | 528.9 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -21.14 | 267.15 | 15.90 | 211.71 | 0.4881 | 676.0 | 676.7 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -20.78 | 266.17 | 14.91 | 210.52 | 0.4758 | 852.0 | 673.5 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -20.15 | 266.07 | 14.82 | 211.09 | 0.4668 | 802.0 | 579.2 | |
| 0.00 | 3.27 | 0.00 | 1.83 | -20.31 | 265.82 | 14.56 | 210.48 | 0.4669 | 737.0 | 603.8 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -18.05 | 264.99 | 13.74 | 211.77 | 0.4306 | -905.0 | -687.5 | |
| 0.00 | 1.54 | 0.00 | 0.87 | -20.87 | 265.23 | 13.98 | 208.85 | 0.4697 | 773.0 | 694.6 | |
| 0.00 | 2.27 | 0.00 | 1.26 | -20.47 | 263.02 | 11.77 | 205.32 | 0.4487 | 919.0 | 762.0 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -21.71 | 263.06 | 11.80 | 204.16 | 0.4662 | 613.0 | 492.2 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -21.98 | 262.94 | 11.69 | 203.71 | 0.4692 | 782.0 | 580.2 | |
| 7.36 | 15.99 | 4.09 | 8.88 | -21.10 | 262.57 | 11.32 | 203.86 | 0.4545 | 920.5 | 723.8 | |
| 0.00 | 1.73 | 0.00 | 0.97 | -22.75 | 262.60 | 11.35 | 202.41 | 0.4780 | 742.0 | 586.8 | |
| 2.09 | -13.00 | 1.16 | -13.00 | -21.03 | 262.33 | 11.08 | 203.48 | 0.4521 | 828.6 | 999999 | |
| 0.36 | 1.45 | 0.20 | 0.81 | -20.95 | 262.00 | 10.74 | 202.91 | 0.4490 | 650.5 | 542.0 | |
| 0.00 | 0.55 | 0.00 | 0.30 | -20.78 | 261.69 | 10.43 | 202.48 | 0.4446 | 735.0 | 619.0 | |
| 0.00 | 0.91 | 0.00 | 0.49 | -18.16 | 260.80 | 9.55 | 203.24 | 0.4012 | 708.0 | 569.1 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -18.87 | 259.83 | 8.58 | 200.43 | 0.4059 | -812.0 | -706.0 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -18.57 | 259.55 | 8.30 | 200.10 | 0.3999 | -833.0 | -572.5 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -20.52 | 259.49 | 8.24 | 198.31 | 0.4288 | -765.0 | -593.9 | |
| 0.00 | 1.45 | 0.00 | 0.81 | -23.42 | 258.89 | 7.63 | 195.12 | 0.4692 | -823.0 | -518.6 | |
| 0.00 | 0.73 | 0.00 | 0.40 | -21.47 | 257.20 | 5.95 | 192.90 | 0.4335 | 511.0 | 459.1 | |
| 3.63 | 9.54 | 2.01 | 5.26 | -22.15 | 256.76 | 5.51 | 191.65 | 0.4423 | -1089.4 | -727.0 | |
| 0.00 | 2.73 | 0.00 | 1.51 | -22.48 | 256.51 | 5.26 | 190.97 | 0.4467 | -842.0 | -766.7 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -22.14 | 256.23 | 4.98 | 190.56 | 0.4406 | -776.0 | -562.6 | |
| 0.00 | 1.64 | 0.00 | 0.91 | -23.57 | 255.98 | 4.73 | 189.46 | 0.4619 | -816.0 | -690.2 | |
| 95.22 | 565.14 | 51.15 | 303.49 | -18.87 | 255.68 | 4.43 | 190.90 | 0.3878 | 1510.2 | 445.1 | |
| 0.00 | 1.91 | 0.00 | 1.06 | -23.19 | 255.70 | 4.45 | 189.05 | 0.4554 | -1058.0 | -880.2 | |
| 0.00 | 3.36 | 0.00 | 1.83 | -21.22 | 254.10 | 2.85 | 186.35 | 0.4213 | 951.0 | 633.5 | |
| 0.00 | 3.09 | 0.00 | 1.65 | -18.46 | 253.96 | 2.71 | 186.86 | 0.3771 | 224.0 | 213.2 | |
| 0.00 | 1.18 | 0.00 | 0.63 | -18.63 | 253.58 | 2.33 | 185.85 | 0.3790 | 697.0 | 445.3 | |
| 0.00 | 0.82 | 0.00 | 0.45 | -21.79 | 253.59 | 2.34 | 185.08 | 0.4295 | -996.0 | -803.4 | |
| 0.00 | 1.91 | 0.00 | 1.02 | -18.49 | 253.16 | 1.91 | 184.83 | 0.3762 | -859.0 | -585.5 | |
| 0.00 | 1.64 | 0.00 | 0.88 | -18.79 | 252.77 | 1.52 | 183.80 | 0.3805 | 477.0 | 456.1 | |
| 0.00 | 0.64 | 0.00 | 0.34 | -18.82 | 252.39 | 1.14 | 182.84 | 0.3807 | -751.0 | -589.1 | |
| 0.00 | 1.64 | 0.00 | 0.91 | -23.55 | 252.35 | 1.10 | 182.22 | 0.4559 | -801.0 | -691.5 | |
| 0.00 | 0.73 | 0.00 | 0.39 | -20.78 | 252.27 | 1.02 | 182.32 | 0.4121 | -714.0 | -589.1 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -22.43 | 252.18 | 0.93 | 181.97 | 0.4382 | -774.0 | -604.9 | |
| 1.36 | 3.45 | 0.73 | 1.85 | -18.92 | 252.07 | 0.81 | 182.02 | 0.3821 | -943.9 | -735.8 | |
| 0.00 | 1.82 | 0.00 | 0.98 | -19.15 | 252.03 | 0.78 | 181.92 | 0.3858 | 267.0 | 225.9 | |
| 0.00 | 1.73 | 0.00 | 0.93 | -19.18 | 251.84 | 0.59 | 181.45 | 0.3862 | 762.0 | 610.3 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -18.26 | 251.65 | 0.39 | 181.01 | 0.3712 | -604.0 | -527.4 | |
| 0.00 | 1.73 | 0.00 | 0.93 | -20.04 | 251.49 | 0.23 | 180.55 | 0.4000 | -590.0 | -429.4 | |
| 1.82 | 4.91 | 0.97 | 2.63 | -19.15 | 251.13 | -0.12 | 179.70 | 0.3855 | -1058.5 | -845.9 | |
| 0.00 | 1.00 | 0.00 | 0.54 | -19.74 | 251.13 | -0.12 | 179.71 | 0.3952 | -789.0 | -634.2 | |
| 0.55 | -45.00 | 0.29 | -45.00 | -19.21 | 251.00 | -0.25 | 179.39 | 0.3866 | -976.5 | 999999 | |
| 0.00 | 1.64 | 0.00 | 0.88 | -19.91 | 250.19 | -1.06 | 177.48 | 0.3982 | -816.0 | -554.6 | |
| 0.00 | 2.27 | 0.00 | 1.31 | -27.07 | 249.85 | -1.41 | 177.54 | 0.5099 | -654.0 | -452.1 | |
| 0.00 | 1.09 | 0.00 | 0.59 | -19.74 | 249.90 | -1.35 | 176.77 | 0.3958 | -766.0 | -603.2 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -24.31 | 248.98 | -2.27 | 175.56 | 0.4686 | -843.0 | -672.7 | |
| 0.00 | 0.73 | 0.00 | 0.42 | -27.25 | 248.23 | -3.02 | 174.75 | 0.5143 | -621.0 | -492.5 | |
| 0.00 | 0.91 | 0.00 | 0.50 | -22.71 | 246.29 | -4.96 | 169.73 | 0.4493 | -647.0 | -549.1 | |
| 0.00 | 0.45 | 0.00 | 0.26 | -26.23 | 245.22 | -6.03 | 169.22 | 0.5055 | -453.0 | -461.8 | |
| 0.00 | 2.09 | 0.00 | 1.20 | -26.31 | 245.02 | -6.24 | 168.88 | 0.5071 | -714.0 | -591.3 | |
| 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. | |