SDO HMI 2014-05-26 01:00:39 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 |
| 28.41 | 119.31 | 14.40 | 60.33 | -10.75 | 81.79 | 5.14 | 207.12 | 0.1972 | 1.8 | 88.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-05-26 01:00:39 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 |
| 18.94 | 44.72 | 9.62 | 22.72 | -9.89 | 86.16 | 9.51 | 227.77 | 0.2208 | 1207.6 | 480.4 | |
| 0.00 | 2.16 | 0.00 | 1.10 | -11.40 | 84.57 | 7.93 | 217.89 | 0.2211 | 707.0 | 553.8 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -10.05 | 82.61 | 5.97 | 214.25 | 0.1827 | 1025.0 | 789.7 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -11.84 | 82.59 | 5.94 | 209.22 | 0.2084 | 817.0 | 530.6 | |
| 0.00 | 1.71 | 0.00 | 0.86 | -10.26 | 82.34 | 5.69 | 212.36 | 0.1832 | 981.0 | 740.9 | |
| 0.00 | 1.71 | 0.00 | 0.86 | -10.57 | 82.34 | 5.70 | 211.48 | 0.1877 | 733.0 | 607.0 | |
| 0.00 | 1.62 | 0.00 | 0.82 | -9.62 | 81.99 | 5.34 | 212.71 | 0.1706 | 878.0 | 710.8 | |
| 0.00 | 9.74 | 0.00 | 4.90 | -9.96 | 81.81 | 5.16 | 210.78 | 0.1739 | 434.0 | 815.5 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -10.05 | 80.94 | 4.30 | 206.14 | 0.1682 | 892.0 | 645.0 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -9.77 | 80.75 | 4.11 | 205.87 | 0.1625 | 714.0 | 569.2 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -11.56 | 80.62 | 3.97 | 201.07 | 0.1897 | 637.0 | 462.6 | |
| 0.00 | 3.25 | 0.00 | 1.63 | -10.17 | 80.42 | 3.77 | 203.02 | 0.1663 | 1183.0 | 880.5 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -10.39 | 80.39 | 3.74 | 202.36 | 0.1696 | 90.0 | 137.9 | |
| 0.00 | 1.26 | 0.00 | 0.63 | -10.27 | 80.17 | 3.52 | 201.45 | 0.1662 | 403.0 | 389.5 | |
| 0.81 | 2.07 | 0.41 | 1.04 | -10.11 | 79.89 | 3.25 | 200.22 | 0.1620 | -844.7 | -649.3 | |
| 0.00 | 2.34 | 0.00 | 1.18 | -11.84 | 79.88 | 3.23 | 196.95 | 0.1901 | -795.0 | -668.4 | |
| 0.00 | 1.71 | 0.00 | 0.86 | -9.84 | 79.70 | 3.06 | 199.73 | 0.1564 | -1000.0 | -767.3 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -11.07 | 79.72 | 3.07 | 197.39 | 0.1766 | -818.0 | -649.2 | |
| 0.00 | 1.53 | 0.00 | 0.79 | -17.99 | 79.55 | 2.90 | 189.58 | 0.2907 | -847.0 | -541.8 | |
| 0.00 | 1.62 | 0.00 | 0.82 | -11.96 | 79.44 | 2.80 | 194.61 | 0.1901 | -1005.0 | -753.9 | |
| 0.00 | 1.98 | 0.00 | 1.00 | -9.99 | 79.43 | 2.78 | 197.76 | 0.1574 | -896.0 | -698.0 | |
| 0.00 | 1.62 | 0.00 | 0.81 | -10.36 | 78.97 | 2.32 | 194.36 | 0.1613 | -736.0 | -443.1 | |
| 0.00 | 1.89 | 0.00 | 0.95 | -11.07 | 78.07 | 1.43 | 188.30 | 0.1703 | -1057.0 | -836.1 | |
| 0.00 | 2.61 | 0.00 | 1.32 | -11.93 | 77.92 | 1.28 | 186.81 | 0.1847 | -806.0 | -657.0 | |
| 0.00 | 0.81 | 0.00 | 0.41 | -10.02 | 77.89 | 1.24 | 188.10 | 0.1519 | -939.0 | -799.7 | |
| 0.00 | 1.08 | 0.00 | 0.54 | -11.13 | 77.83 | 1.18 | 186.83 | 0.1708 | -858.0 | -719.8 | |
| 0.00 | 1.53 | 0.00 | 0.77 | -11.13 | 77.55 | 0.90 | 185.23 | 0.1702 | -1064.0 | -857.9 | |
| 0.00 | 1.17 | 0.00 | 0.58 | -8.18 | 77.48 | 0.84 | 186.99 | 0.1193 | -982.0 | -747.5 | |
| 8.66 | 13.53 | 4.37 | 6.82 | -12.21 | 77.02 | 0.38 | 181.96 | 0.1883 | -1122.2 | -793.6 | |
| 0.00 | 2.34 | 0.00 | 1.17 | -9.37 | 76.50 | -0.15 | 178.95 | 0.1392 | -1031.0 | -840.2 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -11.28 | 76.34 | -0.31 | 178.25 | 0.1722 | -811.0 | -543.4 | |
| 0.00 | 1.71 | 0.00 | 0.87 | -14.28 | 75.27 | -1.38 | 174.03 | 0.2250 | -31.0 | -100.3 | |
| 0.00 | 2.80 | 0.00 | 1.42 | -14.00 | 73.11 | -3.54 | 164.64 | 0.2270 | -633.0 | -562.1 | |
| 0.00 | 0.99 | 0.00 | 0.51 | -17.22 | 71.81 | -4.84 | 163.53 | 0.2854 | -624.0 | -497.7 | |
| 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. | |