SDO HMI 2014-11-03 13:00:28 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 |
| 32.09 | 94.08 | 16.61 | 48.97 | -4.52 | 86.73 | -15.59 | 119.06 | 0.3075 | 622.4 | 456.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-03 13:00:28 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 |
| 0.00 | 1.38 | 0.00 | 0.71 | -5.75 | 89.68 | -12.64 | 127.97 | 0.2774 | 889.0 | 673.9 | |
| 2.51 | 4.15 | 1.29 | 2.14 | -5.24 | 89.39 | -12.93 | 125.85 | 0.2762 | 1174.7 | 867.7 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -5.43 | 88.46 | -13.86 | 124.54 | 0.2908 | 917.0 | 795.7 | |
| 1.82 | 51.62 | 0.94 | 26.73 | -4.06 | 87.97 | -14.35 | 119.57 | 0.2855 | -598.9 | 473.4 | |
| 0.00 | 1.99 | 0.00 | 1.03 | -5.02 | 87.95 | -14.37 | 122.39 | 0.2941 | 765.0 | 598.9 | |
| 0.00 | 1.64 | 0.00 | 0.85 | -5.35 | 87.85 | -14.47 | 123.16 | 0.2986 | 747.0 | 577.8 | |
| 1.99 | -4.00 | 1.03 | -4.00 | -4.09 | 87.81 | -14.50 | 119.40 | 0.2880 | 594.3 | 999999 | |
| 0.00 | 3.20 | 0.00 | 1.66 | -4.94 | 87.61 | -14.71 | 121.55 | 0.2982 | 961.0 | 862.8 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -5.12 | 87.58 | -14.74 | 122.01 | 0.3003 | 725.0 | 592.4 | |
| 16.69 | -4.00 | 8.64 | -4.00 | -4.04 | 87.51 | -14.81 | 118.72 | 0.2921 | 1105.8 | 999999 | |
| 7.61 | -4.00 | 3.95 | -4.00 | -4.13 | 87.20 | -15.12 | 118.50 | 0.2974 | 948.7 | 999999 | |
| 0.00 | 1.56 | 0.00 | 0.81 | -5.01 | 87.11 | -15.20 | 120.90 | 0.3058 | 884.0 | 707.2 | |
| 1.47 | -4.00 | 0.76 | -4.00 | -4.23 | 87.04 | -15.28 | 118.53 | 0.3005 | 776.4 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -4.95 | 86.90 | -15.42 | 120.38 | 0.3084 | 716.0 | 531.4 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -4.47 | 86.85 | -15.47 | 118.93 | 0.3052 | 751.0 | 554.2 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -4.15 | 86.42 | -15.90 | 117.35 | 0.3089 | -592.0 | -440.7 | |
| 0.00 | 6.05 | 0.00 | 3.16 | -4.54 | 86.32 | -16.00 | 118.31 | 0.3135 | 763.0 | 684.4 | |
| 0.00 | 2.08 | 0.00 | 1.08 | -4.00 | 86.12 | -16.20 | 116.48 | 0.3124 | 780.0 | 601.5 | |
| 0.00 | 2.08 | 0.00 | 1.08 | -4.49 | 85.95 | -16.37 | 117.61 | 0.3185 | 845.0 | 705.2 | |
| 0.00 | 1.04 | 0.00 | 0.54 | -5.75 | 85.88 | -16.44 | 120.94 | 0.3297 | 730.0 | 590.4 | |
| 0.00 | 0.61 | 0.00 | 0.32 | -6.21 | 85.77 | -16.54 | 121.95 | 0.3351 | 722.0 | 576.6 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -3.06 | 85.23 | -17.09 | 112.59 | 0.3192 | -868.0 | -710.4 | |
| 0.00 | 1.82 | 0.00 | 0.95 | -5.25 | 85.15 | -17.17 | 118.55 | 0.3361 | 720.0 | 543.2 | |
| 0.00 | 0.52 | 0.00 | 0.27 | -5.11 | 84.78 | -17.54 | 117.66 | 0.3404 | 691.0 | 540.3 | |
| 0.00 | 1.30 | 0.00 | 0.69 | -5.36 | 83.20 | -19.12 | 116.26 | 0.3653 | 725.0 | 583.3 | |
| 0.00 | 1.38 | 0.00 | 0.74 | -5.64 | 82.90 | -19.42 | 116.59 | 0.3716 | 772.0 | 642.6 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -2.66 | 82.89 | -19.43 | 108.97 | 0.3529 | 734.0 | 535.2 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -7.15 | 80.40 | -21.92 | 117.22 | 0.4182 | -771.0 | -631.2 | |
| 0.00 | 1.73 | 0.00 | 0.94 | -5.75 | 79.63 | -22.69 | 113.40 | 0.4200 | -810.0 | -611.0 | |
| 0.00 | 0.69 | 0.00 | 0.38 | -6.03 | 79.26 | -23.06 | 113.67 | 0.4271 | -547.0 | -445.9 | |
| 0.00 | 1.64 | 0.00 | 0.90 | -6.65 | 78.87 | -23.45 | 114.62 | 0.4366 | -808.0 | -622.1 | |
| 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. | |