SDO HMI 2014-11-03 23:00:28 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 102.26 | 518.73 | 53.69 | 272.58 | 12.15 | 114.48 | 17.68 | 296.19 | 0.3314 | -37.6 | -85.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-03 23:00:28 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 |
| 3.20 | 246.18 | 1.71 | 131.16 | 12.23 | 117.91 | 21.11 | 292.52 | 0.3827 | -882.9 | -439.5 | |
| 0.00 | 2.68 | 0.00 | 1.44 | 12.84 | 117.70 | 20.90 | 294.20 | 0.3830 | -63.0 | -106.1 | |
| 10.11 | -1.00 | 5.39 | -1.00 | 12.10 | 117.19 | 20.38 | 292.83 | 0.3711 | -1130.9 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 13.31 | 116.93 | 20.13 | 296.11 | 0.3746 | -703.0 | -485.3 | |
| 32.16 | -1.00 | 17.10 | -1.00 | 12.35 | 116.69 | 19.89 | 293.94 | 0.3651 | -1317.9 | 999999 | |
| 4.67 | 42.62 | 2.47 | 22.50 | 11.41 | 116.16 | 19.36 | 291.94 | 0.3519 | -1084.4 | -722.1 | |
| 3.54 | -6.00 | 1.87 | -6.00 | 11.20 | 116.12 | 19.31 | 291.42 | 0.3501 | -981.5 | 999999 | |
| 4.49 | -1.00 | 2.38 | -1.00 | 12.19 | 116.06 | 19.26 | 294.13 | 0.3548 | -1168.8 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.64 | 10.82 | 115.70 | 18.90 | 290.75 | 0.3418 | -921.0 | -722.3 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 14.03 | 115.86 | 19.06 | 299.07 | 0.3640 | -739.0 | -635.4 | |
| 0.00 | 4.06 | 0.00 | 2.15 | 12.41 | 115.69 | 18.89 | 295.09 | 0.3507 | -806.0 | -815.0 | |
| 0.00 | 2.51 | 0.00 | 1.32 | 11.84 | 115.49 | 18.69 | 293.78 | 0.3442 | -290.0 | -290.5 | |
| 0.00 | 1.64 | 0.00 | 0.86 | 11.29 | 114.84 | 18.04 | 292.91 | 0.3312 | 531.0 | 337.9 | |
| 0.78 | 4.93 | 0.41 | 2.58 | 12.09 | 113.94 | 17.14 | 296.21 | 0.3226 | 936.6 | 725.8 | |
| 0.00 | 0.86 | 0.00 | 0.45 | 11.82 | 113.57 | 16.77 | 295.91 | 0.3154 | -540.0 | -400.5 | |
| 0.00 | 1.04 | 0.00 | 0.54 | 11.39 | 112.72 | 15.92 | 295.70 | 0.2998 | 684.0 | 497.6 | |
| 0.00 | 1.21 | 0.00 | 0.63 | 10.95 | 112.54 | 15.74 | 294.55 | 0.2941 | 819.0 | 695.6 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 10.53 | 112.45 | 15.65 | 293.33 | 0.2902 | 815.0 | 698.2 | |
| 0.00 | 3.54 | 0.00 | 1.84 | 11.91 | 112.28 | 15.48 | 297.90 | 0.2968 | 888.0 | 717.0 | |
| 0.00 | 1.56 | 0.00 | 0.80 | 10.92 | 112.19 | 15.39 | 294.93 | 0.2887 | 850.0 | 762.7 | |
| 0.00 | 1.12 | 0.00 | 0.59 | 13.81 | 112.28 | 15.48 | 303.41 | 0.3118 | 745.0 | 677.7 | |
| 0.00 | 1.73 | 0.00 | 0.89 | 11.38 | 112.03 | 15.23 | 296.59 | 0.2893 | 924.0 | 729.0 | |
| 0.00 | 2.07 | 0.00 | 1.07 | 11.62 | 111.89 | 15.08 | 297.57 | 0.2889 | 1011.0 | 796.2 | |
| 0.00 | 1.38 | 0.00 | 0.71 | 11.38 | 111.87 | 15.07 | 296.83 | 0.2869 | 909.0 | 743.5 | |
| 1.64 | 194.15 | 0.85 | 100.20 | 11.86 | 111.68 | 14.88 | 298.64 | 0.2876 | 872.1 | 465.6 | |
| 1.04 | -25.00 | 0.54 | -25.00 | 12.50 | 111.59 | 14.79 | 300.72 | 0.2912 | 687.9 | 999999 | |
| 40.37 | -25.00 | 20.84 | -25.00 | 12.23 | 111.14 | 14.33 | 300.66 | 0.2826 | 1247.0 | 999999 | |
| 0.26 | -25.00 | 0.13 | -25.00 | 11.85 | 110.71 | 13.91 | 300.17 | 0.2733 | 1118.7 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 11.92 | 110.05 | 13.25 | 301.56 | 0.2644 | 865.0 | 704.8 | |
| 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. | |