| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 234.54 | 1091.03 | 121.60 | 564.26 | -18.78 | 323.99 | -11.56 | 139.13 | 0.2822 | -47.7 | 35.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-12 22:00:29 UT
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 | 1.65 | 0.00 | 0.84 | -18.69 | 330.53 | -5.03 | 157.38 | 0.2169 | -89.0 | 17.5 | |
| 13.44 | 392.59 | 6.80 | 198.81 | -17.40 | 329.78 | -5.77 | 151.59 | 0.2027 | 1502.4 | 495.6 | |
| 48.23 | -2.00 | 24.44 | -2.00 | -17.79 | 329.33 | -6.23 | 150.73 | 0.2122 | 1397.8 | 999999 | |
| 3.82 | -2.00 | 1.94 | -2.00 | -17.84 | 328.70 | -6.86 | 148.47 | 0.2184 | 957.8 | 999999 | |
| 1.13 | -2.00 | 0.57 | -2.00 | -18.11 | 328.53 | -7.03 | 148.53 | 0.2237 | 701.9 | 999999 | |
| 0.69 | -2.00 | 0.35 | -2.00 | -17.99 | 328.31 | -7.24 | 147.45 | 0.2239 | 881.8 | 999999 | |
| 0.00 | 3.73 | 0.00 | 1.90 | -18.83 | 327.96 | -7.60 | 148.27 | 0.2391 | 611.0 | 413.9 | |
| 1.56 | 3.21 | 0.79 | 1.63 | -17.86 | 327.97 | -7.58 | 145.93 | 0.2253 | 1063.7 | 771.8 | |
| 0.00 | 1.47 | 0.00 | 0.75 | -17.44 | 327.93 | -7.63 | 144.64 | 0.2199 | 925.0 | 732.4 | |
| 0.00 | 0.87 | 0.00 | 0.44 | -19.47 | 327.77 | -7.79 | 149.08 | 0.2498 | -804.0 | -706.6 | |
| 0.00 | 1.56 | 0.00 | 0.80 | -18.28 | 327.80 | -7.76 | 146.40 | 0.2328 | 807.0 | 650.2 | |
| 0.00 | 1.30 | 0.00 | 0.66 | -17.98 | 327.68 | -7.87 | 145.25 | 0.2297 | 958.0 | 800.1 | |
| 5.12 | 68.70 | 2.61 | 35.02 | -18.12 | 327.39 | -8.17 | 144.67 | 0.2345 | 1104.4 | 455.7 | |
| 0.00 | 2.00 | 0.00 | 1.02 | -18.46 | 327.31 | -8.25 | 145.26 | 0.2398 | 124.0 | 206.7 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -17.00 | 327.26 | -8.30 | 141.11 | 0.2210 | 872.0 | 670.3 | |
| 8.24 | -13.00 | 4.20 | -13.00 | -17.79 | 327.12 | -8.43 | 142.91 | 0.2326 | 1222.0 | 999999 | |
| 2.34 | -13.00 | 1.19 | -13.00 | -18.02 | 326.67 | -8.89 | 142.12 | 0.2404 | 871.4 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.62 | -17.92 | 326.32 | -9.23 | 140.82 | 0.2427 | 775.0 | 638.8 | |
| 0.00 | 3.12 | 0.00 | 1.60 | -18.13 | 326.00 | -9.56 | 140.42 | 0.2489 | 920.0 | 762.4 | |
| 0.00 | 1.04 | 0.00 | 0.53 | -17.41 | 325.18 | -10.38 | 136.16 | 0.2493 | 866.0 | 741.6 | |
| 0.00 | 1.47 | 0.00 | 0.76 | -20.35 | 324.60 | -10.96 | 142.16 | 0.2918 | -834.0 | -673.9 | |
| 0.00 | 2.17 | 0.00 | 1.12 | -19.23 | 323.75 | -11.81 | 137.47 | 0.2871 | -748.0 | -732.4 | |
| 0.00 | 1.21 | 0.00 | 0.62 | -14.50 | 323.39 | -12.17 | 122.42 | 0.2428 | 959.0 | 813.6 | |
| 6.85 | 187.10 | 3.55 | 97.14 | -18.72 | 322.98 | -12.58 | 134.45 | 0.2902 | 5.8 | -298.3 | |
| 36.17 | -24.00 | 18.77 | -24.00 | -19.29 | 322.77 | -12.78 | 135.46 | 0.2991 | -1177.2 | 999999 | |
| 0.61 | -24.00 | 0.31 | -24.00 | -18.83 | 322.59 | -12.97 | 133.89 | 0.2961 | -1030.1 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -20.54 | 322.41 | -13.15 | 137.63 | 0.3175 | 730.0 | 558.3 | |
| 0.00 | 3.64 | 0.00 | 1.89 | -18.25 | 322.37 | -13.18 | 131.93 | 0.2924 | 1005.0 | 758.9 | |
| 15.79 | -24.00 | 8.24 | -24.00 | -20.16 | 322.08 | -13.47 | 136.10 | 0.3168 | 1010.9 | 999999 | |
| 0.00 | 2.43 | 0.00 | 1.27 | -20.64 | 321.84 | -13.71 | 136.72 | 0.3250 | 753.0 | 559.2 | |
| 0.00 | 0.78 | 0.00 | 0.40 | -18.27 | 322.02 | -13.54 | 131.26 | 0.2971 | 764.0 | 651.3 | |
| 0.00 | 1.13 | 0.00 | 0.59 | -20.43 | 321.80 | -13.76 | 136.14 | 0.3231 | 656.0 | 456.3 | |
| 0.00 | 1.04 | 0.00 | 0.54 | -15.54 | 321.87 | -13.69 | 123.04 | 0.2732 | 852.0 | 638.8 | |
| 0.00 | 1.13 | 0.00 | 0.59 | -18.40 | 321.49 | -14.07 | 130.59 | 0.3051 | 711.0 | 517.3 | |
| 0.00 | 1.04 | 0.00 | 0.55 | -20.40 | 320.75 | -14.81 | 134.08 | 0.3349 | -687.0 | -552.8 | |
| 0.00 | 1.30 | 0.00 | 0.68 | -20.00 | 320.73 | -14.83 | 133.11 | 0.3310 | -988.0 | -808.3 | |
| 0.00 | 2.00 | 0.00 | 1.03 | -16.06 | 321.00 | -14.55 | 123.13 | 0.2897 | 703.0 | 608.3 | |
| 0.00 | 0.61 | 0.00 | 0.32 | -23.55 | 320.07 | -15.49 | 139.38 | 0.3777 | -672.0 | -466.3 | |
| 9.11 | 40.86 | 4.76 | 21.34 | -18.49 | 320.22 | -15.34 | 128.51 | 0.3221 | -1171.2 | -612.3 | |
| 0.00 | 1.04 | 0.00 | 0.55 | -20.12 | 319.86 | -15.70 | 131.87 | 0.3427 | -825.0 | -676.2 | |
| 0.00 | 0.87 | 0.00 | 0.46 | -23.19 | 319.41 | -16.15 | 137.57 | 0.3807 | 613.0 | 410.0 | |
| 0.00 | 1.73 | 0.00 | 0.92 | -20.26 | 319.35 | -16.21 | 131.33 | 0.3503 | -968.0 | -790.8 | |
| 24.20 | 96.11 | 12.84 | 51.04 | -21.02 | 319.16 | -16.39 | 132.73 | 0.3602 | -1165.9 | -247.6 | |
| 0.00 | 3.04 | 0.00 | 1.61 | -20.44 | 319.20 | -16.36 | 131.49 | 0.3539 | -861.0 | -619.0 | |
| 0.69 | 212.43 | 0.37 | 112.07 | -19.19 | 319.30 | -16.26 | 128.74 | 0.3405 | -978.6 | -432.0 | |
| 6.85 | -45.00 | 3.60 | -45.00 | -18.79 | 319.21 | -16.35 | 127.62 | 0.3380 | -1414.2 | 999999 | |
| 1.39 | -45.00 | 0.73 | -45.00 | -18.56 | 318.90 | -16.66 | 126.59 | 0.3399 | -797.5 | 999999 | |
| 29.06 | -45.00 | 15.33 | -45.00 | -19.01 | 318.79 | -16.77 | 127.53 | 0.3455 | -1202.1 | 999999 | |
| 1.73 | 40.68 | 0.92 | 21.67 | -20.53 | 318.49 | -17.07 | 130.59 | 0.3636 | -1133.4 | -392.1 | |
| 10.41 | -45.00 | 5.51 | -45.00 | -19.37 | 318.45 | -17.10 | 127.87 | 0.3530 | -1000.5 | 999999 | |
| 2.17 | -49.00 | 1.15 | -49.00 | -20.53 | 318.32 | -17.24 | 130.32 | 0.3656 | -1069.2 | 999999 | |
| 4.94 | -49.00 | 2.63 | -49.00 | -20.43 | 318.07 | -17.49 | 129.72 | 0.3677 | -989.6 | 999999 | |
| 0.00 | 2.43 | 0.00 | 1.28 | -18.20 | 318.09 | -17.47 | 124.50 | 0.3476 | -753.0 | -593.6 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |