SDO HMI 2014-11-28 04:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 137.60 | 646.72 | 74.25 | 350.65 | 4.08 | 161.38 | 23.71 | 277.58 | 0.4060 | -105.6 | -160.0 | |
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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 | 0.94 | 0.00 | 0.53 | 1.93 | 166.08 | 28.41 | 271.71 | 0.4777 | 653.0 | 514.3 | |
| 1.28 | 4.88 | 0.72 | 2.73 | 3.24 | 165.51 | 27.84 | 274.53 | 0.4697 | 765.3 | 563.0 | |
| 0.00 | 1.80 | 0.00 | 1.00 | 3.86 | 165.19 | 27.52 | 275.92 | 0.4655 | -949.0 | -754.1 | |
| 3.42 | 416.20 | 1.89 | 228.76 | 3.28 | 163.88 | 26.21 | 274.86 | 0.4444 | -718.8 | -426.3 | |
| 65.12 | -4.00 | 35.81 | -4.00 | 3.67 | 163.36 | 25.69 | 275.84 | 0.4368 | -1340.5 | 999999 | |
| 2.65 | -4.00 | 1.46 | -4.00 | 4.45 | 163.16 | 25.49 | 277.65 | 0.4348 | -831.8 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.61 | 6.82 | 163.17 | 25.51 | 283.03 | 0.4407 | -601.0 | -435.6 | |
| 1.54 | -4.00 | 0.84 | -4.00 | 3.32 | 162.99 | 25.32 | 275.09 | 0.4305 | -1241.3 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 5.76 | 162.49 | 24.82 | 280.89 | 0.4272 | -601.0 | -589.8 | |
| 0.94 | -4.00 | 0.51 | -4.00 | 4.22 | 162.26 | 24.60 | 277.35 | 0.4203 | -1151.0 | 999999 | |
| 0.43 | -4.00 | 0.23 | -4.00 | 4.37 | 162.27 | 24.60 | 277.70 | 0.4207 | -895.6 | 999999 | |
| 1.11 | -4.00 | 0.61 | -4.00 | 4.16 | 162.13 | 24.46 | 277.24 | 0.4181 | -1137.0 | 999999 | |
| 0.00 | 2.14 | 0.00 | 1.16 | 4.55 | 161.85 | 24.18 | 278.25 | 0.4144 | -927.0 | -736.6 | |
| 0.00 | 1.97 | 0.00 | 1.07 | 4.76 | 161.76 | 24.09 | 278.78 | 0.4134 | -282.0 | -413.0 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 4.70 | 161.27 | 23.61 | 278.80 | 0.4056 | -796.0 | -564.1 | |
| 0.00 | 3.94 | 0.00 | 2.12 | 5.39 | 160.69 | 23.02 | 280.72 | 0.3979 | -891.0 | -755.3 | |
| 6.08 | 18.65 | 3.26 | 10.03 | 3.67 | 160.37 | 22.70 | 276.48 | 0.3893 | 968.1 | 432.3 | |
| 0.00 | 2.05 | 0.00 | 1.10 | 4.77 | 160.34 | 22.67 | 279.29 | 0.3909 | 64.0 | 95.6 | |
| 0.00 | 2.65 | 0.00 | 1.42 | 3.94 | 160.21 | 22.55 | 277.21 | 0.3873 | -95.0 | 5.7 | |
| 0.00 | 1.88 | 0.00 | 1.01 | 5.51 | 160.21 | 22.54 | 281.23 | 0.3907 | -992.0 | -754.6 | |
| 0.00 | 1.88 | 0.00 | 1.01 | 3.11 | 160.10 | 22.43 | 275.09 | 0.3842 | 787.0 | 618.6 | |
| 2.57 | 19.94 | 1.38 | 10.67 | 4.98 | 160.02 | 22.36 | 279.95 | 0.3864 | 810.6 | 424.8 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 5.43 | 159.95 | 22.28 | 281.13 | 0.3863 | -644.0 | -572.6 | |
| 1.63 | 3.68 | 0.87 | 1.97 | 3.18 | 159.84 | 22.17 | 275.30 | 0.3801 | 849.4 | 473.4 | |
| 5.73 | -22.00 | 3.07 | -22.00 | 4.89 | 159.73 | 22.07 | 279.84 | 0.3815 | 1046.1 | 999999 | |
| 0.00 | 5.31 | 0.00 | 2.83 | 2.94 | 159.32 | 21.66 | 274.79 | 0.3715 | 983.0 | 731.8 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 5.64 | 159.38 | 21.71 | 281.94 | 0.3779 | 948.0 | 799.3 | |
| 0.00 | 2.14 | 0.00 | 1.14 | 2.86 | 158.75 | 21.08 | 274.67 | 0.3621 | 963.0 | 759.1 | |
| 1.03 | 4.36 | 0.55 | 2.32 | 5.68 | 158.71 | 21.04 | 282.37 | 0.3674 | -1037.9 | -782.9 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 4.17 | 158.40 | 20.73 | 278.39 | 0.3585 | 760.0 | 480.2 | |
| 4.71 | 8.30 | 2.50 | 4.40 | 4.85 | 158.39 | 20.72 | 280.28 | 0.3599 | -1006.3 | -637.4 | |
| 0.00 | 0.86 | 0.00 | 0.45 | 3.19 | 157.84 | 20.17 | 275.81 | 0.3476 | 809.0 | 599.5 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 3.76 | 157.76 | 20.09 | 277.45 | 0.3472 | 653.0 | 480.2 | |
| 0.00 | 5.13 | 0.00 | 2.71 | 4.53 | 157.49 | 19.83 | 279.78 | 0.3446 | 457.0 | 627.5 | |
| 0.00 | 4.71 | 0.00 | 2.48 | 5.75 | 157.44 | 19.77 | 283.28 | 0.3474 | 479.0 | 650.3 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 6.16 | 157.33 | 19.66 | 284.52 | 0.3471 | 632.0 | 565.5 | |
| 2.05 | 4.54 | 1.08 | 2.39 | 4.12 | 157.11 | 19.44 | 278.74 | 0.3373 | 991.7 | 750.0 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 3.14 | 156.86 | 19.19 | 275.92 | 0.3315 | 819.0 | 653.2 | |
| 0.00 | 0.86 | 0.00 | 0.45 | 3.44 | 156.87 | 19.20 | 276.80 | 0.3321 | 869.0 | 779.1 | |
| 0.00 | 0.51 | 0.00 | 0.27 | 5.25 | 156.89 | 19.22 | 282.16 | 0.3368 | 690.0 | 480.7 | |
| 0.00 | 3.34 | 0.00 | 1.75 | 3.91 | 156.82 | 19.15 | 278.25 | 0.3322 | 923.0 | 867.9 | |
| 3.08 | 24.73 | 1.62 | 12.96 | 5.46 | 156.49 | 18.82 | 283.03 | 0.3311 | 856.3 | 679.6 | |
| 0.00 | 3.25 | 0.00 | 1.70 | 3.47 | 156.43 | 18.76 | 277.05 | 0.3250 | 988.0 | 815.3 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 4.04 | 156.38 | 18.71 | 278.79 | 0.3253 | 925.0 | 696.1 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 5.96 | 156.44 | 18.77 | 284.55 | 0.3322 | 753.0 | 552.6 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 6.23 | 156.39 | 18.72 | 285.37 | 0.3324 | 842.0 | 709.8 | |
| 8.56 | -42.00 | 4.48 | -42.00 | 5.40 | 156.26 | 18.60 | 282.99 | 0.3273 | 1118.6 | 999999 | |
| 3.42 | -42.00 | 1.79 | -42.00 | 5.25 | 156.01 | 18.34 | 282.71 | 0.3227 | 1151.7 | 999999 | |
| 0.94 | 2.91 | 0.49 | 1.52 | 5.91 | 155.97 | 18.30 | 284.72 | 0.3244 | 784.8 | 653.9 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 5.55 | 155.96 | 18.29 | 283.65 | 0.3228 | 916.0 | 761.5 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 4.51 | 155.74 | 18.07 | 280.58 | 0.3160 | 642.0 | 475.7 | |
| 1.88 | 23.79 | 0.98 | 12.42 | 5.82 | 155.71 | 18.05 | 284.64 | 0.3200 | 984.0 | 627.3 | |
| 1.97 | -52.00 | 1.03 | -52.00 | 5.55 | 155.61 | 17.94 | 283.89 | 0.3173 | 1181.2 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 4.19 | 155.54 | 17.87 | 279.66 | 0.3119 | 984.0 | 763.4 | |
| 1.37 | -52.00 | 0.71 | -52.00 | 5.91 | 155.44 | 17.77 | 285.12 | 0.3159 | 763.8 | 999999 | |
| 16.09 | 47.83 | 8.37 | 24.88 | 5.14 | 155.16 | 17.49 | 282.91 | 0.3086 | 1280.3 | 523.4 | |
| 0.00 | 2.65 | 0.00 | 1.38 | 4.02 | 154.95 | 17.28 | 279.39 | 0.3017 | 909.0 | 665.6 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 4.29 | 154.24 | 16.57 | 280.69 | 0.2907 | 758.0 | 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. | |