SDO HMI 2014-11-03 20:00:28 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 |
| 105.76 | 596.15 | 55.13 | 310.44 | 12.08 | 114.47 | 16.01 | 298.17 | 0.3064 | -104.9 | -76.7 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-03 20:00:28 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 |
| 4.06 | 266.96 | 2.15 | 140.82 | 12.25 | 117.91 | 19.46 | 294.07 | 0.3581 | -865.1 | -410.8 | |
| 3.37 | -1.00 | 1.78 | -1.00 | 12.20 | 117.56 | 19.10 | 294.30 | 0.3524 | -891.2 | 999999 | |
| 12.88 | -1.00 | 6.80 | -1.00 | 12.03 | 117.25 | 18.79 | 294.15 | 0.3468 | -1171.4 | 999999 | |
| 1.64 | -1.00 | 0.86 | -1.00 | 11.88 | 116.99 | 18.53 | 294.04 | 0.3420 | -1130.6 | 999999 | |
| 32.67 | -1.00 | 17.19 | -1.00 | 12.22 | 116.69 | 18.23 | 295.28 | 0.3396 | -1392.7 | 999999 | |
| 0.95 | -1.00 | 0.50 | -1.00 | 12.50 | 116.23 | 17.77 | 296.58 | 0.3347 | -1093.5 | 999999 | |
| 3.54 | 73.63 | 1.86 | 38.50 | 11.48 | 116.13 | 17.67 | 293.84 | 0.3266 | -1223.8 | -673.9 | |
| 3.80 | -1.00 | 1.99 | -1.00 | 12.09 | 116.11 | 17.65 | 295.57 | 0.3301 | -1194.2 | 999999 | |
| 0.86 | -7.00 | 0.45 | -7.00 | 11.61 | 115.88 | 17.42 | 294.47 | 0.3237 | -1137.1 | 999999 | |
| 0.95 | -7.00 | 0.50 | -7.00 | 11.46 | 115.84 | 17.38 | 294.09 | 0.3221 | -1204.2 | 999999 | |
| 0.00 | 1.38 | 0.00 | 0.72 | 10.96 | 115.62 | 17.16 | 292.86 | 0.3157 | -887.0 | -707.8 | |
| 0.00 | 1.21 | 0.00 | 0.63 | 10.78 | 115.54 | 17.08 | 292.41 | 0.3136 | -854.0 | -538.1 | |
| 0.00 | 1.30 | 0.00 | 0.67 | 11.55 | 114.64 | 16.18 | 295.80 | 0.3046 | 713.0 | 584.9 | |
| 0.00 | 5.79 | 0.00 | 3.01 | 12.16 | 114.05 | 15.59 | 298.45 | 0.3001 | 766.0 | 719.9 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 10.16 | 113.46 | 15.01 | 292.89 | 0.2779 | 811.0 | 582.5 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 10.58 | 113.33 | 14.87 | 294.48 | 0.2784 | 806.0 | 559.7 | |
| 0.00 | 2.33 | 0.00 | 1.20 | 10.99 | 112.60 | 14.14 | 296.89 | 0.2701 | 834.0 | 636.5 | |
| 0.00 | 1.04 | 0.00 | 0.54 | 13.75 | 112.66 | 14.20 | 305.40 | 0.2937 | 779.0 | 641.8 | |
| 0.00 | 1.30 | 0.00 | 0.67 | 12.07 | 112.53 | 14.07 | 300.54 | 0.2773 | 684.0 | 534.7 | |
| 0.00 | 3.20 | 0.00 | 1.64 | 10.42 | 112.39 | 13.93 | 295.28 | 0.2630 | 755.0 | 656.3 | |
| 0.00 | 1.64 | 0.00 | 0.85 | 11.83 | 112.42 | 13.97 | 299.96 | 0.2739 | 728.0 | 586.8 | |
| 0.00 | 1.56 | 0.00 | 0.80 | 10.43 | 112.17 | 13.71 | 295.62 | 0.2597 | 948.0 | 744.3 | |
| 0.00 | 0.86 | 0.00 | 0.44 | 10.97 | 112.16 | 13.70 | 297.51 | 0.2634 | 887.0 | 758.7 | |
| 0.00 | 0.78 | 0.00 | 0.40 | 11.00 | 112.01 | 13.55 | 297.88 | 0.2613 | 768.0 | 590.6 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 11.66 | 111.98 | 13.52 | 300.16 | 0.2660 | 819.0 | 767.7 | |
| 0.00 | 1.47 | 0.00 | 0.75 | 11.45 | 111.87 | 13.41 | 299.65 | 0.2628 | 772.0 | 647.1 | |
| 5.01 | 227.29 | 2.57 | 116.54 | 12.33 | 111.48 | 13.02 | 303.28 | 0.2645 | 1116.6 | 435.2 | |
| 9.94 | -27.00 | 5.10 | -27.00 | 12.12 | 111.47 | 13.01 | 302.61 | 0.2625 | 1212.4 | 999999 | |
| 1.38 | -27.00 | 0.71 | -27.00 | 12.54 | 111.46 | 13.00 | 303.99 | 0.2661 | 836.2 | 999999 | |
| 21.17 | -27.00 | 10.85 | -27.00 | 12.24 | 111.10 | 12.64 | 303.75 | 0.2584 | 1388.2 | 999999 | |
| 3.02 | -27.00 | 1.55 | -27.00 | 12.43 | 110.93 | 12.47 | 304.71 | 0.2576 | 1170.4 | 999999 | |
| 0.52 | -27.00 | 0.27 | -27.00 | 12.16 | 110.73 | 12.27 | 304.24 | 0.2524 | 1016.8 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 11.99 | 110.16 | 11.70 | 304.88 | 0.2429 | 940.0 | 754.8 | |
| 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. | |