SDO HMI 2014-08-06 16:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.72 | 110.07 | 9.84 | 68.28 | -8.13 | 229.43 | 33.80 | 247.11 | 0.5987 | 382.7 | 332.1 | |
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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 | 2.71 | 0.00 | 1.83 | -6.83 | 236.61 | 40.98 | 253.06 | 0.6830 | 664.0 | 449.3 | |
| 0.00 | 0.90 | 0.00 | 0.61 | -7.69 | 236.05 | 40.43 | 251.60 | 0.6796 | 474.0 | 406.4 | |
| 0.00 | 0.81 | 0.00 | 0.55 | -7.74 | 235.94 | 40.31 | 251.47 | 0.6784 | 711.0 | 558.3 | |
| 0.00 | 1.17 | 0.00 | 0.78 | -6.82 | 235.64 | 40.01 | 252.65 | 0.6711 | 518.0 | 431.3 | |
| 0.00 | 2.35 | 0.00 | 1.57 | -7.04 | 235.62 | 40.00 | 252.33 | 0.6717 | 681.0 | 623.5 | |
| 0.00 | 1.27 | 0.00 | 0.85 | -8.06 | 235.57 | 39.95 | 250.86 | 0.6753 | 632.0 | 550.3 | |
| 0.00 | 1.36 | 0.00 | 0.90 | -6.77 | 235.43 | 39.81 | 252.63 | 0.6684 | 750.0 | 656.4 | |
| 0.00 | 2.35 | 0.00 | 1.56 | -8.35 | 234.85 | 39.22 | 250.10 | 0.6677 | 770.0 | 530.8 | |
| 1.08 | 11.75 | 0.71 | 7.72 | -7.89 | 234.44 | 38.81 | 250.57 | 0.6606 | 736.1 | 544.5 | |
| 0.00 | 2.26 | 0.00 | 1.49 | -8.17 | 234.43 | 38.81 | 250.16 | 0.6617 | 787.0 | 606.7 | |
| 0.00 | 0.90 | 0.00 | 0.61 | -11.48 | 234.85 | 39.23 | 245.76 | 0.6820 | 743.0 | 612.5 | |
| 4.79 | -9.00 | 3.14 | -9.00 | -7.69 | 234.30 | 38.67 | 250.78 | 0.6581 | 859.5 | 999999 | |
| 0.00 | 1.81 | 0.00 | 1.18 | -8.11 | 234.11 | 38.48 | 250.08 | 0.6575 | 766.0 | 677.5 | |
| 0.00 | 1.36 | 0.00 | 0.89 | -7.86 | 234.04 | 38.42 | 250.41 | 0.6556 | 926.0 | 926.2 | |
| 0.00 | 1.63 | 0.00 | 1.07 | -9.49 | 234.04 | 38.42 | 248.08 | 0.6629 | 669.0 | 607.1 | |
| 0.00 | 1.54 | 0.00 | 0.99 | -6.37 | 233.66 | 38.04 | 252.41 | 0.6446 | 735.0 | 561.8 | |
| 0.00 | 0.63 | 0.00 | 0.41 | -8.37 | 233.78 | 38.16 | 249.54 | 0.6547 | 460.0 | 551.0 | |
| 0.00 | 1.45 | 0.00 | 0.95 | -9.28 | 233.70 | 38.07 | 248.20 | 0.6578 | 750.0 | 573.2 | |
| 0.00 | 2.17 | 0.00 | 1.38 | -7.37 | 232.36 | 36.74 | 250.28 | 0.6324 | -54.0 | -143.2 | |
| 0.90 | 3.34 | 0.57 | 2.10 | -7.64 | 231.17 | 35.54 | 249.24 | 0.6184 | 871.8 | 707.9 | |
| 0.00 | 1.45 | 0.00 | 0.91 | -7.91 | 231.04 | 35.42 | 248.75 | 0.6181 | 835.0 | 667.6 | |
| 0.00 | 0.99 | 0.00 | 0.62 | -8.73 | 230.67 | 35.05 | 247.29 | 0.6176 | 275.0 | 239.7 | |
| 0.00 | 0.72 | 0.00 | 0.45 | -8.44 | 230.60 | 34.98 | 247.69 | 0.6152 | 654.0 | 564.4 | |
| 0.00 | 1.27 | 0.00 | 0.79 | -8.06 | 230.42 | 34.79 | 248.17 | 0.6109 | 848.0 | 718.3 | |
| 0.00 | 7.77 | 0.00 | 4.86 | -8.43 | 230.34 | 34.72 | 247.55 | 0.6118 | 725.0 | 652.5 | |
| 0.00 | 0.99 | 0.00 | 0.62 | -8.47 | 230.01 | 34.39 | 247.29 | 0.6078 | 739.0 | 569.5 | |
| 0.00 | 1.08 | 0.00 | 0.67 | -7.39 | 229.20 | 33.58 | 248.48 | 0.5918 | 659.0 | 535.7 | |
| 1.99 | 3.89 | 1.22 | 2.38 | -7.60 | 229.11 | 33.49 | 248.09 | 0.5917 | 881.1 | 689.7 | |
| 1.08 | 2.35 | 0.67 | 1.44 | -8.59 | 228.87 | 33.25 | 246.39 | 0.5938 | -729.2 | -557.9 | |
| 0.00 | 1.27 | 0.00 | 0.76 | -5.22 | 228.28 | 32.66 | 251.47 | 0.5689 | 718.0 | 556.5 | |
| 0.00 | 0.90 | 0.00 | 0.54 | -6.70 | 227.58 | 31.96 | 248.59 | 0.5668 | 686.0 | 538.6 | |
| 1.45 | 10.57 | 0.87 | 6.36 | -7.97 | 227.43 | 31.80 | 246.41 | 0.5716 | 603.8 | 622.7 | |
| 0.00 | 1.08 | 0.00 | 0.65 | -5.96 | 227.24 | 31.62 | 249.60 | 0.5584 | 649.0 | 592.2 | |
| 0.00 | 1.45 | 0.00 | 0.86 | -6.27 | 227.15 | 31.53 | 249.03 | 0.5588 | 816.0 | 656.2 | |
| 4.43 | -32.00 | 2.66 | -32.00 | -7.89 | 227.20 | 31.58 | 246.38 | 0.5683 | 928.1 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -8.11 | 227.18 | 31.56 | 246.02 | 0.5693 | 447.0 | 296.7 | |
| 0.00 | 1.72 | 0.00 | 1.02 | -6.09 | 226.71 | 31.09 | 249.05 | 0.5519 | 741.0 | 645.1 | |
| 0.00 | 1.81 | 0.00 | 1.07 | -6.15 | 226.18 | 30.56 | 248.60 | 0.5450 | 856.0 | 779.7 | |
| 0.00 | 2.35 | 0.00 | 1.39 | -6.67 | 226.07 | 30.45 | 247.63 | 0.5464 | 949.0 | 767.0 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -6.45 | 225.98 | 30.36 | 247.95 | 0.5440 | 833.0 | 732.7 | |
| 0.00 | 1.63 | 0.00 | 0.96 | -6.98 | 226.02 | 30.40 | 247.07 | 0.5474 | 717.0 | 653.9 | |
| 0.00 | 1.17 | 0.00 | 0.73 | -14.40 | 226.63 | 31.01 | 236.03 | 0.6039 | -702.0 | -567.3 | |
| 0.00 | 1.54 | 0.00 | 0.95 | -14.36 | 226.41 | 30.78 | 235.90 | 0.6009 | -731.0 | -568.1 | |
| 0.00 | 2.17 | 0.00 | 1.28 | -7.05 | 225.60 | 29.98 | 246.65 | 0.5422 | 611.0 | 555.2 | |
| 0.00 | 0.99 | 0.00 | 0.61 | -14.45 | 226.31 | 30.69 | 235.69 | 0.6005 | -741.0 | -602.2 | |
| 0.00 | 1.99 | 0.00 | 1.23 | -15.25 | 226.11 | 30.48 | 234.39 | 0.6042 | -553.0 | -480.5 | |
| 0.00 | 1.63 | 0.00 | 0.95 | -11.85 | 222.20 | 26.58 | 235.78 | 0.5316 | -641.0 | -518.8 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -4.87 | 219.94 | 24.32 | 246.14 | 0.4506 | -735.0 | -538.8 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -10.73 | 220.10 | 24.48 | 235.41 | 0.4965 | -822.0 | -576.2 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -4.06 | 218.62 | 22.99 | 246.59 | 0.4264 | -893.0 | -631.1 | |
| 0.00 | 2.17 | 0.00 | 1.18 | -3.78 | 218.54 | 22.92 | 247.12 | 0.4235 | -812.0 | -576.1 | |
| 0.00 | 3.89 | 0.00 | 2.12 | -3.58 | 218.21 | 22.58 | 247.25 | 0.4174 | -887.0 | -756.4 | |
| 0.00 | 1.17 | 0.00 | 0.67 | -11.99 | 218.45 | 22.83 | 231.39 | 0.4876 | -700.0 | -586.1 | |
| 0.00 | 1.81 | 0.00 | 1.05 | -16.37 | 217.92 | 22.30 | 224.13 | 0.5248 | -131.0 | -219.6 | |
| 0.00 | 1.17 | 0.00 | 0.68 | -16.76 | 217.86 | 22.24 | 223.53 | 0.5283 | -557.0 | -535.8 | |
| 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. | |