SDO HMI 2014-11-26 23:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 131.25 | 564.47 | 65.60 | 282.40 | 4.26 | 160.58 | 6.98 | 296.90 | 0.1357 | -26.7 | -137.0 | |
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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 | 1.11 | 0.00 | 0.56 | -2.37 | 164.00 | 10.41 | 249.96 | 0.1931 | 731.0 | 543.5 | |
| 2.48 | 350.14 | 1.25 | 175.77 | 3.79 | 163.06 | 9.47 | 284.18 | 0.1701 | -818.0 | -424.9 | |
| 35.68 | -2.00 | 17.92 | -2.00 | 4.06 | 162.71 | 9.11 | 286.28 | 0.1654 | -1360.6 | 999999 | |
| 22.50 | -2.00 | 11.29 | -2.00 | 3.47 | 162.61 | 9.02 | 282.90 | 0.1612 | -1343.9 | 999999 | |
| 8.04 | -2.00 | 4.04 | -2.00 | 4.42 | 162.38 | 8.79 | 288.97 | 0.1618 | -1229.6 | 999999 | |
| 0.51 | -2.00 | 0.26 | -2.00 | 4.68 | 162.05 | 8.46 | 291.24 | 0.1581 | -1079.3 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.64 | 4.51 | 161.78 | 8.19 | 290.79 | 0.1526 | -862.0 | -566.8 | |
| 0.00 | 1.37 | 0.00 | 0.69 | 4.12 | 161.45 | 7.86 | 289.10 | 0.1449 | -911.0 | -776.1 | |
| 2.22 | -2.00 | 1.11 | -2.00 | 4.81 | 161.37 | 7.77 | 293.67 | 0.1478 | -1170.2 | 999999 | |
| 1.97 | 3.85 | 0.98 | 1.92 | 2.82 | 161.26 | 7.66 | 280.42 | 0.1361 | -1103.0 | -823.0 | |
| 0.00 | 1.20 | 0.00 | 0.60 | 4.63 | 161.18 | 7.59 | 293.03 | 0.1438 | -118.0 | -119.4 | |
| 0.00 | 0.94 | 0.00 | 0.47 | 5.19 | 161.01 | 7.42 | 297.10 | 0.1451 | -777.0 | -701.7 | |
| 0.00 | 2.31 | 0.00 | 1.15 | 4.22 | 160.82 | 7.23 | 291.24 | 0.1353 | 788.0 | 467.3 | |
| 0.00 | 6.08 | 0.00 | 3.04 | 4.84 | 160.59 | 7.00 | 296.16 | 0.1358 | 30.0 | 18.7 | |
| 0.00 | 1.28 | 0.00 | 0.64 | 1.32 | 160.29 | 6.70 | 269.12 | 0.1172 | -904.0 | -732.8 | |
| 0.00 | 2.48 | 0.00 | 1.24 | 4.78 | 160.26 | 6.67 | 296.86 | 0.1303 | 83.0 | 227.2 | |
| 2.31 | 4.96 | 1.15 | 2.48 | 4.84 | 159.90 | 6.31 | 298.57 | 0.1253 | 1114.1 | 722.1 | |
| 0.43 | 3.34 | 0.21 | 1.66 | 3.30 | 159.62 | 6.03 | 287.37 | 0.1103 | 1110.2 | 921.2 | |
| 0.00 | 2.22 | 0.00 | 1.11 | 3.63 | 159.50 | 5.91 | 290.53 | 0.1102 | -793.0 | -615.3 | |
| 0.77 | 1.80 | 0.38 | 0.90 | 4.55 | 159.27 | 5.68 | 298.91 | 0.1132 | 1046.2 | 932.6 | |
| 0.00 | 1.11 | 0.00 | 0.55 | 4.82 | 158.95 | 5.35 | 302.45 | 0.1107 | -845.0 | -661.7 | |
| 0.00 | 1.37 | 0.00 | 0.68 | 5.14 | 158.68 | 5.09 | 306.27 | 0.1101 | -1087.0 | -857.1 | |
| 0.00 | 1.80 | 0.00 | 0.89 | 3.40 | 158.64 | 5.05 | 291.38 | 0.0947 | 1159.0 | 847.7 | |
| 0.00 | 1.28 | 0.00 | 0.64 | 4.96 | 158.53 | 4.94 | 305.74 | 0.1062 | -919.0 | -565.8 | |
| 0.51 | 13.86 | 0.26 | 6.90 | 4.52 | 158.38 | 4.79 | 302.99 | 0.0996 | 866.0 | 729.1 | |
| 0.00 | 4.11 | 0.00 | 2.05 | 5.41 | 158.39 | 4.79 | 309.86 | 0.1089 | -1089.0 | -741.9 | |
| 0.34 | 4.79 | 0.17 | 2.38 | 4.25 | 158.29 | 4.69 | 301.15 | 0.0958 | 829.0 | 777.2 | |
| 0.00 | 2.22 | 0.00 | 1.11 | 5.14 | 158.29 | 4.70 | 308.45 | 0.1047 | -914.0 | -624.3 | |
| 0.00 | 1.63 | 0.00 | 0.81 | 5.53 | 158.09 | 4.50 | 312.51 | 0.1064 | -930.0 | -793.8 | |
| 1.88 | -25.00 | 0.94 | -25.00 | 4.40 | 158.02 | 4.43 | 304.00 | 0.0933 | 1218.1 | 999999 | |
| 0.86 | -25.00 | 0.43 | -25.00 | 4.37 | 157.87 | 4.28 | 304.65 | 0.0909 | 1045.3 | 999999 | |
| 1.54 | -25.00 | 0.77 | -25.00 | 4.38 | 157.63 | 4.04 | 306.19 | 0.0875 | 1031.3 | 999999 | |
| 0.00 | 2.14 | 0.00 | 1.06 | 4.08 | 157.60 | 4.01 | 303.55 | 0.0841 | 911.0 | 739.8 | |
| 0.00 | 1.20 | 0.00 | 0.60 | 5.38 | 157.55 | 3.96 | 315.09 | 0.0978 | 675.0 | 526.3 | |
| 0.00 | 1.20 | 0.00 | 0.60 | 3.96 | 157.39 | 3.80 | 303.76 | 0.0799 | 972.0 | 788.8 | |
| 0.00 | 1.37 | 0.00 | 0.68 | 3.16 | 157.09 | 3.50 | 296.41 | 0.0684 | 853.0 | 636.7 | |
| 0.00 | 1.71 | 0.00 | 0.85 | 2.99 | 157.06 | 3.47 | 294.21 | 0.0666 | 1265.0 | 911.2 | |
| 2.57 | 5.65 | 1.27 | 2.80 | 3.58 | 157.01 | 3.41 | 302.26 | 0.0706 | 1154.5 | 874.9 | |
| 4.71 | 28.32 | 2.34 | 14.07 | 4.61 | 156.77 | 3.18 | 315.13 | 0.0788 | 1137.1 | 748.2 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 4.35 | 156.71 | 3.12 | 313.18 | 0.0748 | 676.0 | 449.7 | |
| 6.59 | 24.04 | 3.28 | 11.96 | 5.36 | 156.69 | 3.10 | 321.86 | 0.0875 | 1121.5 | 466.2 | |
| 2.40 | -39.00 | 1.19 | -39.00 | 4.82 | 156.54 | 2.94 | 319.15 | 0.0786 | 1142.8 | 999999 | |
| 0.00 | 1.71 | 0.00 | 0.85 | 6.28 | 156.49 | 2.89 | 329.29 | 0.0987 | 761.0 | 581.8 | |
| 0.00 | 0.94 | 0.00 | 0.47 | 7.64 | 156.50 | 2.90 | 335.11 | 0.1198 | 769.0 | 600.1 | |
| 4.19 | -39.00 | 2.08 | -39.00 | 4.70 | 156.33 | 2.74 | 320.22 | 0.0747 | 1282.4 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 5.95 | 156.34 | 2.74 | 328.87 | 0.0925 | 764.0 | 644.1 | |
| 4.79 | 57.93 | 2.38 | 28.78 | 5.27 | 156.18 | 2.59 | 326.09 | 0.0810 | 1043.5 | 481.0 | |
| 0.00 | 1.11 | 0.00 | 0.55 | 6.07 | 156.19 | 2.59 | 330.90 | 0.0930 | 661.0 | 566.2 | |
| 0.00 | 3.08 | 0.00 | 1.53 | 5.89 | 156.13 | 2.53 | 330.51 | 0.0898 | 963.0 | 690.3 | |
| 0.00 | 1.63 | 0.00 | 0.81 | 5.71 | 156.04 | 2.44 | 330.40 | 0.0863 | 792.0 | 560.6 | |
| 0.86 | 2.99 | 0.42 | 1.49 | 4.35 | 155.97 | 2.38 | 320.92 | 0.0659 | 1087.5 | 796.4 | |
| 23.10 | -47.00 | 11.48 | -47.00 | 5.21 | 155.83 | 2.23 | 329.51 | 0.0768 | 1364.6 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.30 | 4.23 | 155.64 | 2.05 | 323.87 | 0.0608 | 689.0 | 504.9 | |
| 0.00 | 1.37 | 0.00 | 0.68 | 3.43 | 155.61 | 2.02 | 314.83 | 0.0498 | 940.0 | 843.9 | |
| 0.00 | 7.10 | 0.00 | 3.53 | 5.15 | 155.32 | 1.73 | 335.17 | 0.0718 | 140.0 | 136.8 | |
| 0.00 | 0.86 | 0.00 | 0.42 | 4.53 | 155.05 | 1.46 | 334.86 | 0.0600 | 900.0 | 632.5 | |
| 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. | |