SDO HMI 2014-05-18 16:00:38 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 |
| 1.62 | 50.13 | 1.01 | 30.24 | -18.00 | 143.06 | -31.18 | 119.73 | 0.5673 | 247.5 | 216.0 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-05-18 16:00:38 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 | 1.80 | 0.00 | 1.02 | -19.89 | 150.57 | -23.68 | 129.00 | 0.4878 | 632.0 | 577.5 | |
| 0.00 | 1.71 | 0.00 | 0.99 | -19.75 | 148.03 | -26.21 | 126.19 | 0.5172 | 679.0 | 547.5 | |
| 0.00 | 3.06 | 0.00 | 1.76 | -18.70 | 147.82 | -26.42 | 124.22 | 0.5118 | 759.0 | 638.6 | |
| 0.00 | 1.71 | 0.00 | 0.99 | -18.79 | 147.66 | -26.58 | 124.23 | 0.5145 | 732.0 | 601.3 | |
| 0.00 | 2.79 | 0.00 | 1.62 | -19.74 | 147.42 | -26.82 | 125.61 | 0.5245 | 806.0 | 667.9 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -20.21 | 147.04 | -27.20 | 126.04 | 0.5326 | 758.0 | 552.0 | |
| 0.00 | 1.53 | 0.00 | 0.89 | -19.00 | 146.97 | -27.27 | 123.98 | 0.5245 | 943.0 | 795.4 | |
| 0.00 | 1.35 | 0.00 | 0.79 | -18.87 | 146.42 | -27.82 | 123.28 | 0.5304 | 826.0 | 674.3 | |
| 0.00 | 0.90 | 0.00 | 0.54 | -21.70 | 145.82 | -28.43 | 127.31 | 0.5582 | 661.0 | 500.7 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -21.60 | 145.65 | -28.59 | 127.01 | 0.5593 | 571.0 | 423.8 | |
| 0.00 | 1.89 | 0.00 | 1.11 | -19.14 | 145.86 | -28.38 | 123.27 | 0.5392 | 730.0 | 546.8 | |
| 0.00 | 1.53 | 0.00 | 0.89 | -17.15 | 146.10 | -28.14 | 120.11 | 0.5229 | 872.0 | 735.2 | |
| 0.00 | 0.27 | 0.00 | 0.16 | -16.56 | 145.99 | -28.26 | 118.97 | 0.5207 | 425.0 | 487.0 | |
| 0.00 | 1.80 | 0.00 | 1.06 | -19.04 | 145.33 | -28.91 | 122.67 | 0.5450 | 850.0 | 646.2 | |
| 0.00 | 1.44 | 0.00 | 0.84 | -16.99 | 145.63 | -28.62 | 119.45 | 0.5281 | 650.0 | 632.9 | |
| 0.00 | 0.72 | 0.00 | 0.43 | -19.22 | 145.15 | -29.10 | 122.83 | 0.5485 | 613.0 | 393.6 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -18.34 | 145.28 | -28.96 | 121.47 | 0.5410 | 715.0 | 549.5 | |
| 0.00 | 0.63 | 0.00 | 0.37 | -17.17 | 145.49 | -28.76 | 119.66 | 0.5310 | 589.0 | 494.9 | |
| 0.00 | 1.62 | 0.00 | 0.95 | -16.69 | 144.99 | -29.25 | 118.47 | 0.5346 | 604.0 | 396.1 | |
| 0.00 | 1.44 | 0.00 | 0.84 | -15.35 | 145.17 | -29.07 | 116.25 | 0.5245 | -804.0 | -565.6 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -17.10 | 144.70 | -29.54 | 118.95 | 0.5407 | 589.0 | 377.5 | |
| 0.90 | 2.61 | 0.54 | 1.56 | -17.86 | 143.49 | -30.75 | 119.38 | 0.5606 | 974.0 | 708.2 | |
| 0.00 | 2.43 | 0.00 | 1.40 | -11.93 | 144.42 | -29.82 | 109.56 | 0.5183 | 4.0 | 66.0 | |
| 0.00 | 1.17 | 0.00 | 0.70 | -10.42 | 141.20 | -33.04 | 105.42 | 0.5584 | 636.0 | 509.6 | |
| 0.00 | 1.62 | 0.00 | 1.04 | -18.03 | 136.86 | -37.39 | 115.81 | 0.6436 | -858.0 | -685.7 | |
| 0.00 | 0.99 | 0.00 | 0.63 | -17.27 | 137.04 | -37.20 | 114.78 | 0.6381 | -529.0 | -464.1 | |
| 0.72 | 2.43 | 0.47 | 1.58 | -17.89 | 136.33 | -37.92 | 115.35 | 0.6494 | -861.8 | -698.8 | |
| 0.00 | 1.89 | 0.00 | 1.23 | -18.20 | 136.20 | -38.04 | 115.76 | 0.6522 | -675.0 | -508.0 | |
| 0.00 | 1.80 | 0.00 | 1.19 | -18.69 | 135.54 | -38.70 | 116.16 | 0.6621 | -706.0 | -494.0 | |
| 0.00 | 1.80 | 0.00 | 1.19 | -18.40 | 135.09 | -39.15 | 115.53 | 0.6662 | -596.0 | -512.8 | |
| 0.00 | 0.72 | 0.00 | 0.48 | -18.88 | 134.37 | -39.87 | 115.90 | 0.6766 | -546.0 | -469.9 | |
| 0.00 | 1.17 | 0.00 | 0.80 | -19.18 | 133.31 | -40.93 | 115.85 | 0.6899 | -625.0 | -484.5 | |
| 0.00 | 0.72 | 0.00 | 0.49 | -17.01 | 132.87 | -41.37 | 112.66 | 0.6872 | -395.0 | -355.4 | |
| 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. | |