SDO HMI 2014-07-13 20:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.31 | 196.22 | 18.68 | 100.28 | 7.38 | 163.86 | 12.97 | 284.33 | 0.2360 | -180.4 | -138.6 | |
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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 | 1.91 | 0.00 | 1.01 | 7.63 | 171.14 | 20.26 | 280.65 | 0.3507 | -672.0 | -495.3 | |
| 2.63 | 8.26 | 1.39 | 4.36 | 7.91 | 170.67 | 19.78 | 281.69 | 0.3438 | -1043.7 | -680.5 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 8.20 | 170.45 | 19.57 | 282.60 | 0.3412 | -872.0 | -744.3 | |
| 4.54 | 7.80 | 2.38 | 4.10 | 7.26 | 170.05 | 19.16 | 280.04 | 0.3321 | -1109.5 | -722.4 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 8.41 | 169.36 | 18.47 | 283.86 | 0.3242 | -817.0 | -571.9 | |
| 0.00 | 2.18 | 0.00 | 1.13 | 6.86 | 168.80 | 17.91 | 279.34 | 0.3109 | -1022.0 | -762.5 | |
| 0.00 | 3.72 | 0.00 | 1.93 | 5.84 | 168.31 | 17.43 | 276.16 | 0.3010 | -909.0 | -784.1 | |
| 6.44 | 23.14 | 3.34 | 11.99 | 6.30 | 167.98 | 17.09 | 277.83 | 0.2961 | -1179.7 | -671.6 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 7.10 | 167.88 | 16.99 | 280.54 | 0.2963 | -698.0 | -606.6 | |
| 0.00 | 0.36 | 0.00 | 0.19 | 6.28 | 167.34 | 16.45 | 278.01 | 0.2855 | -572.0 | -455.0 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 5.77 | 167.29 | 16.40 | 276.21 | 0.2838 | -814.0 | -662.1 | |
| 0.00 | 1.91 | 0.00 | 0.99 | 8.33 | 167.26 | 16.37 | 285.10 | 0.2901 | -832.0 | -626.0 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 6.93 | 167.04 | 16.15 | 280.42 | 0.2820 | -920.0 | -745.7 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 6.02 | 166.82 | 15.93 | 277.28 | 0.2764 | -799.0 | -660.6 | |
| 0.00 | 2.45 | 0.00 | 1.26 | 7.98 | 166.76 | 15.87 | 284.27 | 0.2807 | -910.0 | -698.4 | |
| 0.00 | 0.73 | 0.00 | 0.37 | 5.64 | 166.04 | 15.16 | 276.13 | 0.2628 | 706.0 | 565.2 | |
| 4.36 | 13.07 | 2.24 | 6.71 | 7.75 | 165.83 | 14.94 | 284.20 | 0.2646 | -1043.5 | -838.3 | |
| 1.09 | -17.00 | 0.56 | -17.00 | 7.93 | 165.74 | 14.85 | 284.96 | 0.2639 | -1073.0 | 999999 | |
| 5.54 | 14.97 | 2.83 | 7.66 | 4.41 | 165.38 | 14.49 | 271.42 | 0.2507 | 1144.9 | 834.4 | |
| 0.00 | 1.72 | 0.00 | 0.88 | 8.25 | 165.18 | 14.29 | 286.67 | 0.2561 | -899.0 | -639.4 | |
| 0.00 | 2.18 | 0.00 | 1.12 | 8.83 | 165.17 | 14.28 | 288.86 | 0.2587 | -1108.0 | -894.2 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 6.27 | 165.02 | 14.13 | 279.04 | 0.2468 | 991.0 | 797.3 | |
| 4.08 | 9.17 | 2.08 | 4.68 | 3.90 | 164.86 | 13.98 | 269.32 | 0.2421 | -1040.4 | -775.6 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 4.54 | 164.85 | 13.96 | 271.98 | 0.2417 | -449.0 | -359.3 | |
| 0.00 | 3.81 | 0.00 | 1.95 | 8.64 | 164.11 | 13.23 | 289.38 | 0.2409 | -1085.0 | -903.9 | |
| 0.00 | 2.09 | 0.00 | 1.06 | 2.97 | 163.63 | 12.74 | 264.99 | 0.2221 | -866.0 | -659.9 | |
| 0.00 | 4.08 | 0.00 | 2.08 | 7.24 | 163.56 | 12.67 | 284.21 | 0.2255 | -858.0 | -718.5 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 7.49 | 163.57 | 12.68 | 285.26 | 0.2266 | -598.0 | -543.9 | |
| 0.00 | 4.99 | 0.00 | 2.55 | 10.05 | 163.54 | 12.65 | 295.76 | 0.2405 | 832.0 | 657.6 | |
| 2.00 | 3.90 | 1.01 | 1.98 | 6.24 | 163.19 | 12.30 | 280.06 | 0.2161 | 1041.5 | 797.8 | |
| 0.00 | 3.99 | 0.00 | 2.03 | 9.91 | 162.83 | 11.95 | 296.44 | 0.2287 | 842.0 | 798.0 | |
| 0.00 | 4.36 | 0.00 | 2.22 | 11.45 | 162.55 | 11.66 | 302.86 | 0.2369 | 663.0 | 743.0 | |
| 1.18 | 20.24 | 0.60 | 10.24 | 8.36 | 162.15 | 11.26 | 291.03 | 0.2079 | -1151.0 | -795.7 | |
| 4.45 | -33.00 | 2.25 | -33.00 | 8.12 | 162.08 | 11.19 | 290.02 | 0.2054 | -1190.5 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 8.92 | 162.01 | 11.12 | 293.75 | 0.2092 | -1006.0 | -778.2 | |
| 0.00 | 0.54 | 0.00 | 0.28 | 8.61 | 162.00 | 11.11 | 292.40 | 0.2071 | -869.0 | -625.8 | |
| 0.00 | 3.81 | 0.00 | 1.93 | 8.04 | 161.61 | 10.72 | 290.39 | 0.1974 | -1059.0 | -848.8 | |
| 0.00 | 2.36 | 0.00 | 1.18 | 8.28 | 159.24 | 8.35 | 296.67 | 0.1616 | 901.0 | 705.1 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 5.85 | 158.55 | 7.66 | 282.63 | 0.1365 | 880.0 | 597.3 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 7.77 | 158.33 | 7.44 | 296.21 | 0.1437 | -838.0 | -626.6 | |
| 0.00 | 3.18 | 0.00 | 1.59 | 9.15 | 157.64 | 6.76 | 306.87 | 0.1459 | 982.0 | 815.3 | |
| 0.00 | 2.00 | 0.00 | 1.00 | 8.54 | 157.63 | 6.75 | 303.37 | 0.1397 | 768.0 | 620.1 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 8.79 | 157.61 | 6.72 | 304.93 | 0.1417 | 763.0 | 616.0 | |
| 0.00 | 2.90 | 0.00 | 1.45 | 8.52 | 157.26 | 6.37 | 304.69 | 0.1341 | 938.0 | 763.2 | |
| 0.00 | 2.63 | 0.00 | 1.32 | 9.78 | 156.48 | 5.59 | 315.54 | 0.1376 | 758.0 | 595.0 | |
| 0.00 | 4.72 | 0.00 | 2.36 | 9.23 | 156.31 | 5.42 | 313.40 | 0.1290 | 812.0 | 778.8 | |
| 0.00 | 3.09 | 0.00 | 1.54 | 9.56 | 156.22 | 5.34 | 315.73 | 0.1320 | 927.0 | 853.8 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 8.92 | 155.90 | 5.02 | 313.82 | 0.1203 | 1129.0 | 945.2 | |
| 0.00 | 0.91 | 0.00 | 0.45 | 9.26 | 155.91 | 5.02 | 315.77 | 0.1244 | 1034.0 | 912.5 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 5.42 | 155.40 | 4.51 | 285.55 | 0.0817 | 949.0 | 717.4 | |
| 0.00 | 2.18 | 0.00 | 1.09 | 8.75 | 155.00 | 4.12 | 318.33 | 0.1072 | 832.0 | 620.5 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 12.55 | 154.12 | 3.24 | 339.28 | 0.1565 | 840.0 | 688.9 | |
| 0.00 | 2.81 | 0.00 | 1.40 | 6.04 | 153.93 | 3.05 | 301.56 | 0.0623 | 830.0 | 834.9 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 5.83 | 153.72 | 2.83 | 300.34 | 0.0572 | 973.0 | 744.5 | |
| 0.00 | 1.00 | 0.00 | 0.49 | 4.89 | 152.00 | 1.11 | 302.48 | 0.0230 | 839.0 | 712.6 | |
| 0.00 | 1.91 | 0.00 | 0.95 | 12.23 | 150.25 | -0.63 | 4.42 | 0.1410 | 829.0 | 645.4 | |
| 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. | |