SDO HMI 2014-08-08 11:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.31 | 160.59 | 11.57 | 79.93 | 8.99 | 174.73 | 2.79 | 322.02 | 0.0893 | 152.1 | 86.9 | |
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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 | 0.81 | 0.00 | 0.42 | 15.55 | 187.23 | 15.29 | 303.02 | 0.3044 | -738.0 | -463.4 | |
| 0.00 | 6.69 | 0.00 | 3.37 | 6.38 | 182.47 | 10.54 | 271.24 | 0.1826 | -1021.0 | -734.6 | |
| 0.00 | 6.33 | 0.00 | 3.18 | 6.60 | 182.17 | 10.23 | 272.49 | 0.1774 | -670.0 | -708.1 | |
| 0.00 | 1.90 | 0.00 | 0.95 | 6.53 | 181.48 | 9.55 | 272.12 | 0.1656 | -892.0 | -700.9 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 10.51 | 181.49 | 9.56 | 294.84 | 0.1807 | -941.0 | -758.5 | |
| 0.00 | 1.72 | 0.00 | 0.86 | 6.54 | 180.86 | 8.93 | 272.27 | 0.1550 | -931.0 | -701.4 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 10.92 | 180.97 | 9.04 | 298.14 | 0.1757 | -845.0 | -675.2 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 8.89 | 180.39 | 8.45 | 287.92 | 0.1533 | -815.0 | -680.5 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 8.65 | 179.91 | 7.98 | 287.29 | 0.1444 | -915.0 | -753.0 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 8.50 | 179.79 | 7.85 | 286.52 | 0.1416 | -961.0 | -762.6 | |
| 0.00 | 6.78 | 0.00 | 3.39 | 9.05 | 179.74 | 7.80 | 290.31 | 0.1436 | -451.0 | -724.9 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 9.42 | 179.44 | 7.50 | 293.50 | 0.1410 | -1018.0 | -850.9 | |
| 0.00 | 1.81 | 0.00 | 0.90 | 8.96 | 179.39 | 7.46 | 290.54 | 0.1375 | -1259.0 | -1059.4 | |
| 0.00 | 1.90 | 0.00 | 0.95 | 9.61 | 179.19 | 7.25 | 295.42 | 0.1385 | -1029.0 | -956.3 | |
| 0.00 | 3.43 | 0.00 | 1.72 | 9.73 | 178.88 | 6.95 | 297.22 | 0.1347 | -863.0 | -793.0 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 8.35 | 177.80 | 5.87 | 290.06 | 0.1082 | -997.0 | -677.9 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 2.64 | 177.13 | 5.19 | 235.23 | 0.1106 | -200.0 | -392.8 | |
| 0.00 | 1.99 | 0.00 | 0.99 | 10.31 | 176.82 | 4.88 | 310.27 | 0.1102 | -990.0 | -836.5 | |
| 0.00 | 2.08 | 0.00 | 1.03 | 8.57 | 176.73 | 4.79 | 296.22 | 0.0925 | -1116.0 | -862.2 | |
| 0.00 | 2.98 | 0.00 | 1.48 | 8.79 | 176.51 | 4.58 | 299.37 | 0.0909 | -706.0 | -748.6 | |
| 0.00 | 1.17 | 0.00 | 0.58 | 8.82 | 176.30 | 4.36 | 300.86 | 0.0880 | -786.0 | -606.8 | |
| 0.00 | 1.36 | 0.00 | 0.67 | 8.52 | 176.26 | 4.33 | 297.96 | 0.0849 | -1001.0 | -809.5 | |
| 0.54 | 3.16 | 0.27 | 1.57 | 8.21 | 176.14 | 4.20 | 295.33 | 0.0806 | -1127.3 | -917.9 | |
| 0.00 | 2.08 | 0.00 | 1.03 | 8.58 | 175.96 | 4.02 | 300.41 | 0.0807 | -1118.0 | -858.0 | |
| 0.00 | 3.52 | 0.00 | 1.75 | 8.64 | 175.77 | 3.84 | 302.26 | 0.0786 | -979.0 | -815.5 | |
| 0.00 | 1.36 | 0.00 | 0.67 | 9.16 | 175.78 | 3.84 | 307.50 | 0.0838 | -1088.0 | -843.7 | |
| 0.00 | 0.81 | 0.00 | 0.40 | 8.91 | 175.78 | 3.84 | 305.12 | 0.0812 | -828.0 | -623.1 | |
| 0.00 | 1.54 | 0.00 | 0.76 | 9.46 | 175.63 | 3.69 | 311.44 | 0.0851 | -923.0 | -764.1 | |
| 0.00 | 1.17 | 0.00 | 0.58 | 10.32 | 175.42 | 3.49 | 319.86 | 0.0932 | 842.0 | 636.9 | |
| 0.63 | 3.80 | 0.31 | 1.89 | 9.84 | 174.09 | 2.15 | 329.37 | 0.0729 | 1088.3 | 949.5 | |
| 0.00 | 1.72 | 0.00 | 0.85 | 9.38 | 173.93 | 1.99 | 327.80 | 0.0647 | 757.0 | 604.4 | |
| 0.00 | 1.81 | 0.00 | 0.90 | 8.08 | 173.89 | 1.95 | 313.19 | 0.0465 | 881.0 | 684.6 | |
| 0.00 | 2.17 | 0.00 | 1.08 | 8.99 | 173.68 | 1.75 | 327.72 | 0.0566 | 678.0 | 572.5 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 9.87 | 173.59 | 1.66 | 335.66 | 0.0695 | 961.0 | 758.9 | |
| 0.00 | 2.53 | 0.00 | 1.25 | 7.90 | 173.52 | 1.59 | 316.16 | 0.0397 | 821.0 | 766.9 | |
| 0.00 | 2.62 | 0.00 | 1.30 | 8.11 | 173.37 | 1.43 | 322.49 | 0.0408 | 1111.0 | 873.8 | |
| 0.72 | 3.71 | 0.36 | 1.84 | 8.38 | 173.22 | 1.28 | 329.15 | 0.0433 | 1227.8 | 944.1 | |
| 0.00 | 1.17 | 0.00 | 0.58 | 9.97 | 173.16 | 1.23 | 341.93 | 0.0683 | 668.0 | 620.7 | |
| 0.00 | 1.72 | 0.00 | 0.85 | 8.63 | 173.10 | 1.16 | 334.15 | 0.0461 | 963.0 | 826.5 | |
| 0.00 | 1.63 | 0.00 | 0.81 | 8.75 | 172.94 | 1.01 | 338.21 | 0.0470 | 1048.0 | 882.2 | |
| 0.00 | 2.08 | 0.00 | 1.03 | 8.78 | 172.70 | 0.76 | 343.39 | 0.0461 | 988.0 | 791.6 | |
| 1.08 | 6.24 | 0.54 | 3.10 | 10.18 | 172.55 | 0.61 | 351.28 | 0.0695 | 936.8 | 780.5 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 8.42 | 172.08 | 0.14 | 356.21 | 0.0378 | 788.0 | 559.1 | |
| 0.00 | 1.36 | 0.00 | 0.67 | 7.47 | 172.02 | 0.08 | 356.19 | 0.0213 | 736.0 | 509.6 | |
| 14.55 | 36.06 | 7.22 | 17.90 | 9.69 | 171.87 | -0.07 | 1.15 | 0.0601 | 1213.4 | 805.9 | |
| 0.00 | 1.54 | 0.00 | 0.76 | 9.27 | 171.68 | -0.25 | 4.78 | 0.0529 | 1023.0 | 812.8 | |
| 0.00 | 1.90 | 0.00 | 0.94 | 8.33 | 171.59 | -0.35 | 9.46 | 0.0367 | 1087.0 | 790.4 | |
| 1.81 | -45.00 | 0.90 | -45.00 | 10.00 | 171.50 | -0.44 | 6.61 | 0.0659 | 1025.4 | 999999 | |
| 2.62 | 6.87 | 1.30 | 3.41 | 9.42 | 171.47 | -0.47 | 8.36 | 0.0559 | 1289.2 | 918.4 | |
| 0.00 | 1.36 | 0.00 | 0.67 | 8.36 | 171.37 | -0.56 | 14.89 | 0.0380 | 1034.0 | 830.3 | |
| 0.00 | 1.17 | 0.00 | 0.58 | 9.15 | 171.31 | -0.62 | 12.06 | 0.0517 | 863.0 | 623.5 | |
| 1.36 | 6.87 | 0.67 | 3.41 | 9.48 | 171.00 | -0.93 | 15.95 | 0.0587 | 1090.1 | 884.6 | |
| 0.00 | 2.17 | 0.00 | 1.08 | 8.84 | 170.91 | -1.02 | 21.41 | 0.0486 | 894.0 | 833.1 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 8.23 | 169.35 | -2.59 | 52.38 | 0.0567 | 814.0 | 587.9 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 13.77 | 167.33 | -4.61 | 30.77 | 0.1532 | 726.0 | 474.2 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 11.04 | 163.73 | -8.21 | 58.93 | 0.1644 | 990.0 | 801.2 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 9.18 | 161.37 | -10.57 | 73.78 | 0.1894 | 819.0 | 640.2 | |
| 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. | |