| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.55 | 74.95 | 4.39 | 43.21 | -12.48 | 224.28 | -27.10 | 119.55 | 0.5134 | -8.6 | -139.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-19 13:00:26 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 | 0.86 | 0.00 | 0.47 | -12.82 | 229.62 | -21.75 | 125.59 | 0.4462 | 656.0 | 548.1 | |
| 0.60 | 2.92 | 0.34 | 1.63 | -13.33 | 228.69 | -22.69 | 125.41 | 0.4625 | 887.7 | 779.7 | |
| 0.00 | 1.72 | 0.00 | 0.95 | -12.13 | 228.80 | -22.57 | 123.32 | 0.4510 | 612.0 | 419.2 | |
| 0.00 | 3.18 | 0.00 | 1.79 | -14.02 | 227.82 | -23.56 | 125.66 | 0.4793 | 910.0 | 726.2 | |
| 0.00 | 1.20 | 0.00 | 0.68 | -13.57 | 227.20 | -24.18 | 124.19 | 0.4833 | 496.0 | 329.6 | |
| 0.00 | 0.69 | 0.00 | 0.39 | -13.05 | 227.16 | -24.22 | 123.21 | 0.4797 | 820.0 | 709.8 | |
| 1.12 | 2.23 | 0.63 | 1.26 | -12.68 | 226.89 | -24.48 | 122.29 | 0.4802 | 797.5 | 702.8 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -12.01 | 226.90 | -24.48 | 121.06 | 0.4751 | 528.0 | 397.3 | |
| 0.00 | 2.66 | 0.00 | 1.50 | -12.47 | 226.52 | -24.86 | 121.53 | 0.4836 | 753.0 | 605.0 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -11.68 | 226.50 | -24.88 | 120.05 | 0.4780 | 749.0 | 618.5 | |
| 0.00 | 1.54 | 0.00 | 0.90 | -16.76 | 225.84 | -25.53 | 128.07 | 0.5263 | -885.0 | -625.1 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -10.87 | 225.97 | -25.41 | 118.04 | 0.4793 | 622.0 | 560.5 | |
| 0.00 | 1.20 | 0.00 | 0.72 | -19.37 | 224.55 | -26.83 | 130.66 | 0.5634 | -625.0 | -586.9 | |
| 0.00 | 1.63 | 0.00 | 0.93 | -11.82 | 225.61 | -25.77 | 119.47 | 0.4907 | 410.0 | 353.5 | |
| 0.94 | 6.27 | 0.54 | 3.58 | -11.52 | 224.90 | -26.48 | 118.30 | 0.4982 | 1034.5 | 738.1 | |
| 0.00 | 1.12 | 0.00 | 0.64 | -12.97 | 224.33 | -27.05 | 120.36 | 0.5156 | -824.0 | -612.2 | |
| 0.00 | 1.46 | 0.00 | 0.84 | -11.81 | 224.19 | -27.19 | 118.21 | 0.5096 | 573.0 | 509.8 | |
| 0.00 | 1.63 | 0.00 | 0.94 | -11.60 | 224.18 | -27.20 | 117.82 | 0.5083 | 649.0 | 563.7 | |
| 0.00 | 1.46 | 0.00 | 0.85 | -13.13 | 223.90 | -27.48 | 120.26 | 0.5223 | 774.0 | 685.6 | |
| 0.00 | 0.43 | 0.00 | 0.25 | -12.60 | 223.07 | -28.31 | 118.65 | 0.5295 | 286.0 | 147.8 | |
| 0.00 | 9.18 | 0.00 | 5.33 | -11.62 | 223.15 | -28.23 | 117.02 | 0.5222 | -791.0 | -629.0 | |
| 0.60 | 1.63 | 0.35 | 0.94 | -10.46 | 223.17 | -28.21 | 114.99 | 0.5149 | -965.1 | -831.7 | |
| 0.00 | 1.12 | 0.00 | 0.64 | -10.67 | 223.08 | -28.30 | 115.30 | 0.5174 | -675.0 | -511.5 | |
| 0.00 | 1.37 | 0.00 | 0.80 | -10.98 | 222.88 | -28.50 | 115.70 | 0.5220 | -769.0 | -609.6 | |
| 2.66 | 4.21 | 1.56 | 2.46 | -12.82 | 222.63 | -28.75 | 118.67 | 0.5367 | -935.9 | -763.1 | |
| 0.00 | 8.50 | 0.00 | 4.95 | -11.65 | 222.77 | -28.61 | 116.79 | 0.5275 | -363.0 | -702.0 | |
| 0.94 | 3.78 | 0.56 | 2.22 | -13.44 | 222.44 | -28.94 | 119.55 | 0.5431 | -820.8 | -664.8 | |
| 0.00 | 1.80 | 0.00 | 1.05 | -11.32 | 222.56 | -28.81 | 116.06 | 0.5282 | -704.0 | -608.0 | |
| 0.00 | 5.15 | 0.00 | 3.04 | -13.26 | 222.19 | -29.19 | 119.05 | 0.5452 | -972.0 | -764.9 | |
| 0.69 | 2.57 | 0.41 | 1.52 | -13.23 | 221.91 | -29.47 | 118.79 | 0.5486 | -600.6 | -503.6 | |
| 0.00 | 0.86 | 0.00 | 0.50 | -11.82 | 222.05 | -29.32 | 116.54 | 0.5379 | -680.0 | -604.1 | |
| 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. | |