SDO HMI 2014-03-01 02:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73.85 | 390.97 | 39.09 | 207.33 | -1.32 | 151.33 | 19.87 | 286.28 | 0.3550 | -285.0 | -226.4 | |
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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 | 1.12 | 0.00 | 0.61 | -1.25 | 155.34 | 23.88 | 283.00 | 0.4171 | 691.0 | 581.2 | |
| 0.00 | 1.12 | 0.00 | 0.61 | 0.25 | 154.72 | 23.26 | 286.89 | 0.4144 | -633.0 | -475.8 | |
| 37.87 | 210.49 | 20.35 | 113.14 | -1.57 | 153.63 | 22.17 | 283.33 | 0.3893 | -1228.0 | -372.6 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 0.38 | 152.44 | 20.98 | 289.12 | 0.3806 | -737.0 | -594.5 | |
| 0.00 | 1.04 | 0.00 | 0.55 | -0.02 | 152.22 | 20.75 | 288.32 | 0.3749 | -726.0 | -628.8 | |
| 0.00 | 1.73 | 0.00 | 0.92 | -0.66 | 151.96 | 20.50 | 286.91 | 0.3676 | -785.0 | -592.7 | |
| 0.52 | 1.38 | 0.28 | 0.74 | -0.03 | 151.87 | 20.41 | 288.60 | 0.3695 | -824.5 | -724.5 | |
| 0.00 | 2.50 | 0.00 | 1.33 | -0.91 | 151.74 | 20.28 | 286.45 | 0.3629 | -842.0 | -686.9 | |
| 0.00 | 3.11 | 0.00 | 1.64 | -4.01 | 151.69 | 20.23 | 277.99 | 0.3499 | -6.0 | -9.9 | |
| 0.00 | 5.43 | 0.00 | 2.88 | -0.83 | 151.49 | 20.03 | 286.88 | 0.3594 | -786.0 | -726.8 | |
| 0.00 | 1.47 | 0.00 | 0.78 | -1.19 | 151.46 | 20.00 | 285.94 | 0.3571 | -856.0 | -732.2 | |
| 0.00 | 0.43 | 0.00 | 0.23 | -1.52 | 151.43 | 19.97 | 285.08 | 0.3551 | -596.0 | -493.2 | |
| 0.00 | 3.97 | 0.00 | 2.11 | -0.41 | 151.39 | 19.93 | 288.06 | 0.3601 | -926.0 | -812.4 | |
| 0.00 | 0.69 | 0.00 | 0.37 | -1.43 | 151.33 | 19.87 | 285.39 | 0.3540 | -569.0 | -422.8 | |
| 0.00 | 1.98 | 0.00 | 1.05 | -2.06 | 151.21 | 19.75 | 283.75 | 0.3492 | -794.0 | -596.2 | |
| 0.00 | 8.71 | 0.00 | 4.60 | -1.56 | 151.05 | 19.59 | 285.26 | 0.3489 | -813.0 | -656.0 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -0.19 | 151.05 | 19.58 | 288.98 | 0.3560 | -734.0 | -692.2 | |
| 0.00 | 2.42 | 0.00 | 1.28 | -1.03 | 151.05 | 19.59 | 286.74 | 0.3515 | -854.0 | -692.6 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -1.93 | 150.93 | 19.47 | 284.35 | 0.3453 | -611.0 | -448.7 | |
| 0.00 | 1.81 | 0.00 | 0.96 | -0.97 | 150.83 | 19.36 | 287.07 | 0.3483 | -758.0 | -603.0 | |
| 12.77 | 34.42 | 6.73 | 18.13 | -1.52 | 150.70 | 19.24 | 285.68 | 0.3437 | -1090.4 | -620.8 | |
| 0.00 | 2.59 | 0.00 | 1.36 | -0.75 | 150.51 | 19.05 | 287.99 | 0.3446 | -997.0 | -802.2 | |
| 2.76 | -21.00 | 1.45 | -21.00 | -1.38 | 150.42 | 18.96 | 286.32 | 0.3399 | -1021.2 | 999999 | |
| 0.00 | 4.14 | 0.00 | 2.17 | -2.28 | 150.24 | 18.78 | 283.89 | 0.3328 | -991.0 | -787.0 | |
| 0.00 | 1.12 | 0.00 | 0.59 | 0.11 | 150.23 | 18.77 | 290.61 | 0.3452 | -792.0 | -557.7 | |
| 0.00 | 2.93 | 0.00 | 1.54 | -0.49 | 150.20 | 18.73 | 289.01 | 0.3412 | -808.0 | -709.0 | |
| 0.00 | 2.59 | 0.00 | 1.36 | -2.55 | 150.21 | 18.75 | 283.13 | 0.3312 | -589.0 | -522.8 | |
| 0.00 | 2.76 | 0.00 | 1.45 | -0.74 | 150.04 | 18.58 | 288.48 | 0.3374 | -786.0 | -691.1 | |
| 0.00 | 1.73 | 0.00 | 0.90 | -1.47 | 149.70 | 18.24 | 286.73 | 0.3281 | -867.0 | -718.8 | |
| 0.00 | 1.47 | 0.00 | 0.76 | -3.12 | 148.63 | 17.16 | 282.64 | 0.3033 | -754.0 | -519.1 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -0.93 | 147.95 | 16.49 | 290.21 | 0.3038 | 449.0 | 367.0 | |
| 0.00 | 1.98 | 0.00 | 1.03 | -1.09 | 147.77 | 16.31 | 289.95 | 0.3000 | 786.0 | 578.1 | |
| 0.00 | 3.54 | 0.00 | 1.84 | -0.73 | 147.74 | 16.27 | 291.10 | 0.3017 | 599.0 | 540.9 | |
| 0.00 | 1.38 | 0.00 | 0.72 | -0.50 | 147.61 | 16.15 | 291.98 | 0.3013 | 791.0 | 651.1 | |
| 1.47 | 7.51 | 0.76 | 3.89 | -1.05 | 147.24 | 15.78 | 290.73 | 0.2920 | 777.0 | 664.3 | |
| 0.00 | 2.50 | 0.00 | 1.30 | -0.07 | 147.12 | 15.66 | 293.98 | 0.2967 | 790.0 | 618.8 | |
| 8.80 | 18.55 | 4.55 | 9.58 | -1.21 | 146.93 | 15.47 | 290.62 | 0.2862 | 1046.0 | 685.8 | |
| 0.00 | 2.33 | 0.00 | 1.21 | 0.29 | 146.90 | 15.44 | 295.37 | 0.2960 | 893.0 | 757.8 | |
| 2.07 | 5.26 | 1.07 | 2.72 | -1.54 | 146.78 | 15.32 | 289.71 | 0.2818 | 930.7 | 845.2 | |
| 0.00 | 2.24 | 0.00 | 1.16 | -0.95 | 146.50 | 15.04 | 292.03 | 0.2812 | 761.0 | 575.9 | |
| 0.00 | 1.29 | 0.00 | 0.67 | 3.47 | 145.95 | 14.49 | 306.04 | 0.3102 | 699.0 | 519.9 | |
| 0.00 | 1.73 | 0.00 | 0.89 | 1.74 | 145.35 | 13.88 | 302.40 | 0.2853 | 629.0 | 541.3 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 1.64 | 145.10 | 13.64 | 302.59 | 0.2810 | 704.0 | 521.9 | |
| 7.59 | 10.70 | 3.90 | 5.49 | -0.37 | 145.06 | 13.60 | 296.24 | 0.2633 | 1018.3 | 701.3 | |
| 0.00 | 2.16 | 0.00 | 1.11 | 1.75 | 144.64 | 13.18 | 303.83 | 0.2756 | 818.0 | 612.5 | |
| 0.00 | 1.73 | 0.00 | 0.88 | -2.18 | 144.43 | 12.96 | 290.73 | 0.2408 | 939.0 | 799.2 | |
| 0.00 | 2.07 | 0.00 | 1.05 | -2.55 | 144.06 | 12.60 | 289.84 | 0.2328 | 951.0 | 763.7 | |
| 0.00 | 1.38 | 0.00 | 0.70 | -2.78 | 144.07 | 12.60 | 288.87 | 0.2314 | 739.0 | 651.6 | |
| 0.00 | 1.12 | 0.00 | 0.57 | -1.09 | 143.81 | 12.35 | 295.94 | 0.2389 | 777.0 | 668.7 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 1.33 | 143.70 | 12.23 | 304.58 | 0.2584 | 861.0 | 801.7 | |
| 0.00 | 2.50 | 0.00 | 1.27 | -2.02 | 143.70 | 12.23 | 292.56 | 0.2303 | 823.0 | 661.8 | |
| 0.00 | 1.64 | 0.00 | 0.84 | 1.51 | 143.48 | 12.02 | 305.61 | 0.2573 | 922.0 | 740.5 | |
| 0.00 | 2.76 | 0.00 | 1.41 | 0.99 | 143.39 | 11.93 | 304.18 | 0.2509 | 913.0 | 710.8 | |
| 0.00 | 4.31 | 0.00 | 2.20 | -0.81 | 143.27 | 11.80 | 298.10 | 0.2329 | 988.0 | 781.6 | |
| 0.00 | 1.98 | 0.00 | 1.01 | -0.42 | 143.17 | 11.71 | 299.74 | 0.2348 | 915.0 | 699.3 | |
| 0.00 | 1.12 | 0.00 | 0.57 | 1.50 | 141.97 | 10.51 | 309.39 | 0.2369 | 616.0 | 416.4 | |
| 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. | |