SDO HMI 2014-11-19 08:00:26 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.36 | 85.87 | 12.15 | 51.10 | -12.50 | 223.69 | -30.42 | 116.95 | 0.5567 | -84.1 | -199.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-19 08:00:26 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 |
| 1.46 | 3.09 | 0.83 | 1.76 | -13.20 | 228.66 | -25.45 | 122.27 | 0.4969 | 894.9 | 734.6 | |
| 0.00 | 1.72 | 0.00 | 0.99 | -13.99 | 227.88 | -26.23 | 122.88 | 0.5127 | 892.0 | 794.8 | |
| 0.00 | 1.37 | 0.00 | 0.79 | -14.30 | 227.78 | -26.33 | 123.30 | 0.5164 | 780.0 | 634.5 | |
| 0.00 | 0.69 | 0.00 | 0.40 | -13.87 | 227.56 | -26.55 | 122.37 | 0.5159 | 476.0 | 402.5 | |
| 0.00 | 1.03 | 0.00 | 0.60 | -14.69 | 226.94 | -27.17 | 123.15 | 0.5298 | -726.0 | -637.0 | |
| 0.00 | 0.77 | 0.00 | 0.44 | -11.91 | 227.17 | -26.94 | 118.63 | 0.5070 | 556.0 | 466.0 | |
| 0.43 | 1.72 | 0.25 | 0.99 | -12.72 | 226.77 | -27.33 | 119.69 | 0.5177 | 927.4 | 781.7 | |
| 0.00 | 1.72 | 0.00 | 1.00 | -12.63 | 226.34 | -27.77 | 119.18 | 0.5228 | 429.0 | 497.1 | |
| 0.00 | 0.60 | 0.00 | 0.37 | -19.38 | 224.56 | -29.55 | 128.13 | 0.5937 | -652.0 | -561.9 | |
| 0.00 | 0.86 | 0.00 | 0.50 | -11.86 | 225.02 | -29.09 | 116.80 | 0.5353 | 773.0 | 710.0 | |
| 3.43 | 6.96 | 2.01 | 4.07 | -11.41 | 224.86 | -29.25 | 115.91 | 0.5346 | 926.2 | 701.3 | |
| 0.00 | 1.72 | 0.00 | 1.02 | -12.95 | 224.39 | -29.72 | 118.15 | 0.5501 | -808.0 | -626.5 | |
| 0.00 | 2.49 | 0.00 | 1.47 | -11.60 | 224.25 | -29.86 | 115.79 | 0.5439 | 758.0 | 556.3 | |
| 0.00 | 1.89 | 0.00 | 1.12 | -11.85 | 224.18 | -29.93 | 116.16 | 0.5462 | 617.0 | 473.2 | |
| 1.72 | 4.55 | 1.02 | 2.71 | -13.08 | 223.92 | -30.19 | 118.01 | 0.5571 | 734.0 | 343.6 | |
| 0.52 | 3.09 | 0.31 | 1.84 | -12.83 | 223.95 | -30.16 | 117.63 | 0.5551 | 809.5 | 502.4 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -11.48 | 224.08 | -30.02 | 115.48 | 0.5453 | 593.0 | 417.4 | |
| 0.00 | 1.03 | 0.00 | 0.61 | -10.34 | 223.41 | -30.70 | 113.08 | 0.5481 | -714.0 | -564.2 | |
| 0.00 | 1.03 | 0.00 | 0.62 | -12.73 | 222.97 | -31.14 | 116.76 | 0.5671 | 191.0 | 168.9 | |
| 0.00 | 1.03 | 0.00 | 0.61 | -10.25 | 223.17 | -30.94 | 112.78 | 0.5508 | -798.0 | -610.1 | |
| 1.29 | 3.26 | 0.76 | 1.94 | -10.56 | 223.07 | -31.04 | 113.23 | 0.5538 | -946.3 | -715.6 | |
| 4.29 | 8.67 | 2.59 | 5.23 | -12.89 | 222.59 | -31.52 | 116.76 | 0.5729 | -918.4 | -697.7 | |
| 0.86 | 19.66 | 0.52 | 11.75 | -11.94 | 222.69 | -31.42 | 115.28 | 0.5663 | -788.7 | -698.7 | |
| 0.69 | 1.63 | 0.42 | 0.99 | -13.45 | 222.44 | -31.67 | 117.54 | 0.5781 | -913.0 | -780.9 | |
| 0.00 | 0.34 | 0.00 | 0.21 | -14.47 | 222.21 | -31.90 | 118.97 | 0.5871 | -450.0 | -527.0 | |
| 0.43 | 1.12 | 0.26 | 0.67 | -11.61 | 222.59 | -31.52 | 114.67 | 0.5657 | -905.6 | -807.4 | |
| 4.55 | 7.73 | 2.76 | 4.69 | -13.27 | 222.11 | -32.00 | 117.03 | 0.5813 | -848.9 | -620.2 | |
| 0.00 | 1.03 | 0.00 | 0.62 | -11.80 | 222.10 | -32.01 | 114.67 | 0.5732 | -623.0 | -559.2 | |
| 0.69 | 3.18 | 0.42 | 1.94 | -13.31 | 221.81 | -32.30 | 116.89 | 0.5852 | -666.8 | -512.4 | |
| 0.00 | 1.03 | 0.00 | 0.64 | -15.07 | 220.42 | -33.68 | 118.65 | 0.6126 | -586.0 | -485.8 | |
| 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. | |