SDO HMI 2014-11-03 16:00:28 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 |
| 117.47 | 615.31 | 60.64 | 317.21 | 12.07 | 114.48 | 13.81 | 301.73 | 0.2744 | -159.5 | -39.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-03 16:00:28 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 |
| 4.93 | 279.52 | 2.58 | 145.69 | 12.25 | 117.87 | 17.20 | 296.54 | 0.3245 | -893.5 | -411.3 | |
| 0.00 | 1.99 | 0.00 | 1.04 | 10.63 | 117.74 | 17.07 | 291.96 | 0.3125 | -768.0 | -511.9 | |
| 0.26 | -1.00 | 0.14 | -1.00 | 12.01 | 117.64 | 16.97 | 296.16 | 0.3194 | -1027.0 | 999999 | |
| 2.94 | -1.00 | 1.54 | -1.00 | 12.20 | 117.55 | 16.88 | 296.79 | 0.3194 | -938.1 | 999999 | |
| 12.45 | -1.00 | 6.49 | -1.00 | 12.02 | 117.29 | 16.62 | 296.63 | 0.3143 | -1219.1 | 999999 | |
| 31.03 | -1.00 | 16.14 | -1.00 | 12.09 | 116.75 | 16.08 | 297.54 | 0.3069 | -1442.4 | 999999 | |
| 4.06 | -1.00 | 2.11 | -1.00 | 12.01 | 116.18 | 15.51 | 298.11 | 0.2979 | -1235.2 | 999999 | |
| 3.28 | -1.00 | 1.70 | -1.00 | 12.38 | 116.14 | 15.47 | 299.26 | 0.3000 | -1043.0 | 999999 | |
| 10.72 | 59.98 | 5.55 | 31.01 | 11.42 | 116.05 | 15.38 | 296.45 | 0.2917 | -1192.5 | -682.4 | |
| 4.75 | -9.00 | 2.46 | -9.00 | 11.63 | 115.72 | 15.05 | 297.61 | 0.2882 | -1254.4 | 999999 | |
| 0.00 | 6.05 | 0.00 | 3.13 | 12.29 | 115.72 | 15.05 | 299.64 | 0.2933 | -895.0 | -781.7 | |
| 2.25 | -9.00 | 1.16 | -9.00 | 11.37 | 115.42 | 14.75 | 297.21 | 0.2819 | -1039.1 | 999999 | |
| 0.00 | 2.16 | 0.00 | 1.11 | 12.64 | 114.67 | 14.00 | 302.45 | 0.2811 | 841.0 | 696.5 | |
| 0.00 | 0.95 | 0.00 | 0.49 | 11.53 | 114.61 | 13.94 | 299.01 | 0.2712 | 658.0 | 543.5 | |
| 0.00 | 1.64 | 0.00 | 0.85 | 12.29 | 114.34 | 13.67 | 301.93 | 0.2733 | 834.0 | 714.7 | |
| 1.82 | 3.63 | 0.93 | 1.87 | 12.14 | 114.02 | 13.35 | 302.05 | 0.2675 | 1065.5 | 799.3 | |
| 0.00 | 0.78 | 0.00 | 0.40 | 12.25 | 112.84 | 12.17 | 304.74 | 0.2519 | 576.0 | 471.1 | |
| 0.00 | 1.99 | 0.00 | 1.01 | 11.03 | 112.75 | 12.08 | 300.62 | 0.2399 | 908.0 | 727.3 | |
| 0.00 | 3.46 | 0.00 | 1.77 | 12.02 | 112.70 | 12.04 | 304.23 | 0.2478 | 792.0 | 516.1 | |
| 0.00 | 1.64 | 0.00 | 0.84 | 11.39 | 112.68 | 12.01 | 302.08 | 0.2418 | 810.0 | 666.9 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 11.57 | 112.19 | 11.52 | 303.80 | 0.2365 | 945.0 | 721.3 | |
| 0.00 | 1.82 | 0.00 | 0.92 | 10.95 | 112.10 | 11.43 | 301.68 | 0.2297 | 958.0 | 716.1 | |
| 0.26 | 243.13 | 0.13 | 123.74 | 12.00 | 111.90 | 11.23 | 305.97 | 0.2364 | 914.0 | 453.9 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 11.58 | 111.88 | 11.21 | 304.52 | 0.2322 | 869.0 | 671.4 | |
| 0.00 | 1.64 | 0.00 | 0.84 | 11.43 | 111.66 | 10.99 | 304.50 | 0.2277 | 1039.0 | 868.7 | |
| 36.99 | -23.00 | 18.83 | -23.00 | 12.25 | 111.32 | 10.65 | 308.25 | 0.2310 | 1358.6 | 999999 | |
| 1.47 | -23.00 | 0.75 | -23.00 | 11.77 | 111.11 | 10.45 | 307.07 | 0.2235 | 991.3 | 999999 | |
| 0.26 | -23.00 | 0.13 | -23.00 | 12.04 | 110.94 | 10.27 | 308.51 | 0.2239 | 1192.3 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.44 | 13.79 | 110.80 | 10.13 | 314.68 | 0.2413 | 783.0 | 696.5 | |
| 0.00 | 1.04 | 0.00 | 0.52 | 11.58 | 109.87 | 9.21 | 309.78 | 0.2049 | 810.0 | 691.3 | |
| 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. | |