SDO HMI 2014-08-09 17:00:39 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 |
| 118.51 | 689.89 | 66.19 | 385.19 | 12.42 | 128.61 | -26.80 | 74.44 | 0.4589 | -111.6 | -69.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-08-09 17:00:39 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 |
| 1.17 | 376.42 | 0.64 | 204.71 | 14.72 | 132.05 | -23.35 | 68.03 | 0.4151 | -868.1 | -429.6 | |
| 1.26 | -1.00 | 0.69 | -1.00 | 13.46 | 132.05 | -23.35 | 70.97 | 0.4095 | -942.8 | 999999 | |
| 61.47 | -1.00 | 33.42 | -1.00 | 14.13 | 131.95 | -23.46 | 69.46 | 0.4139 | -1267.7 | 999999 | |
| 0.27 | -1.00 | 0.15 | -1.00 | 14.01 | 131.17 | -24.23 | 70.24 | 0.4249 | -684.3 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.84 | 12.94 | 130.67 | -24.73 | 72.96 | 0.4283 | -595.0 | -377.4 | |
| 0.00 | 1.26 | 0.00 | 0.70 | 12.88 | 129.98 | -25.42 | 73.43 | 0.4383 | -806.0 | -615.6 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 13.03 | 129.83 | -25.57 | 73.18 | 0.4411 | -475.0 | -438.5 | |
| 0.00 | 1.72 | 0.00 | 0.95 | 12.19 | 129.54 | -25.86 | 75.18 | 0.4429 | 858.0 | 648.9 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 13.18 | 129.05 | -26.35 | 73.22 | 0.4533 | -718.0 | -553.1 | |
| 0.00 | 1.35 | 0.00 | 0.76 | 12.12 | 127.45 | -27.95 | 76.10 | 0.4740 | 966.0 | 723.7 | |
| 0.00 | 2.17 | 0.00 | 1.23 | 11.73 | 126.47 | -28.93 | 77.20 | 0.4876 | 977.0 | 663.1 | |
| 0.00 | 2.62 | 0.00 | 1.48 | 9.99 | 126.37 | -29.03 | 80.80 | 0.4861 | 782.0 | 731.3 | |
| 1.26 | 7.76 | 0.72 | 4.41 | 11.53 | 126.14 | -29.26 | 77.70 | 0.4922 | -811.4 | -191.9 | |
| 0.00 | 1.35 | 0.00 | 0.77 | 11.34 | 125.88 | -29.52 | 78.16 | 0.4957 | 39.0 | 143.8 | |
| 0.00 | 1.72 | 0.00 | 0.98 | 11.18 | 125.75 | -29.65 | 78.52 | 0.4972 | 576.0 | 492.3 | |
| 0.00 | 1.17 | 0.00 | 0.67 | 11.42 | 125.69 | -29.71 | 78.05 | 0.4986 | -100.0 | -56.6 | |
| 0.00 | 1.35 | 0.00 | 0.77 | 9.76 | 125.58 | -29.82 | 81.39 | 0.4977 | 874.0 | 779.6 | |
| 0.00 | 1.26 | 0.00 | 0.72 | 11.71 | 125.37 | -30.03 | 77.55 | 0.5039 | 813.0 | 663.8 | |
| 0.00 | 1.62 | 0.00 | 0.93 | 11.49 | 125.39 | -30.01 | 77.97 | 0.5031 | 662.0 | 488.3 | |
| 2.35 | 283.71 | 1.34 | 163.64 | 10.09 | 125.40 | -30.00 | 80.76 | 0.5007 | 1030.2 | 361.2 | |
| 0.27 | -20.00 | 0.16 | -20.00 | 10.69 | 125.16 | -30.24 | 79.62 | 0.5051 | 1198.7 | 999999 | |
| 0.63 | -20.00 | 0.36 | -20.00 | 10.01 | 125.13 | -30.28 | 80.96 | 0.5047 | 895.7 | 999999 | |
| 2.17 | -20.00 | 1.24 | -20.00 | 10.16 | 124.97 | -30.43 | 80.70 | 0.5073 | 1054.5 | 999999 | |
| 19.95 | -20.00 | 11.47 | -20.00 | 10.61 | 124.85 | -30.55 | 79.83 | 0.5096 | 1093.7 | 999999 | |
| 2.89 | -20.00 | 1.66 | -20.00 | 10.05 | 124.62 | -30.78 | 80.97 | 0.5123 | 1045.7 | 999999 | |
| 0.90 | -20.00 | 0.52 | -20.00 | 10.89 | 124.38 | -31.02 | 79.38 | 0.5169 | 672.5 | 999999 | |
| 10.02 | -20.00 | 5.79 | -20.00 | 10.55 | 124.35 | -31.05 | 80.04 | 0.5169 | 906.8 | 999999 | |
| 12.64 | -20.00 | 7.30 | -20.00 | 9.97 | 124.30 | -31.10 | 81.17 | 0.5168 | 941.7 | 999999 | |
| 1.26 | -20.00 | 0.73 | -20.00 | 10.62 | 124.01 | -31.39 | 79.95 | 0.5219 | 523.8 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.58 | 11.09 | 122.61 | -32.80 | 79.32 | 0.5430 | -736.0 | -575.7 | |
| 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. | |