| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 78.92 | 365.66 | 43.86 | 202.21 | 10.28 | 143.18 | -19.90 | 48.91 | 0.4438 | -99.7 | -131.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-26 00:00:31 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 |
| 1.40 | 190.46 | 0.76 | 103.13 | 10.40 | 146.21 | -16.86 | 44.38 | 0.4097 | -869.8 | -405.8 | |
| 32.34 | -1.00 | 17.51 | -1.00 | 9.97 | 146.17 | -16.90 | 45.21 | 0.4052 | -1233.9 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 10.76 | 145.11 | -17.97 | 45.59 | 0.4260 | -520.0 | -464.3 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 10.71 | 144.73 | -18.35 | 46.28 | 0.4298 | -970.0 | -796.5 | |
| 0.00 | 2.36 | 0.00 | 1.30 | 10.87 | 144.68 | -18.39 | 46.08 | 0.4320 | -644.0 | -527.9 | |
| 0.00 | 1.66 | 0.00 | 0.91 | 10.22 | 144.47 | -18.61 | 47.53 | 0.4275 | -634.0 | -540.4 | |
| 2.01 | 4.55 | 1.10 | 2.48 | 9.79 | 144.36 | -18.71 | 48.45 | 0.4242 | -1001.7 | -766.2 | |
| 0.00 | 0.70 | 0.00 | 0.38 | 10.24 | 143.95 | -19.12 | 48.28 | 0.4338 | -722.0 | -504.5 | |
| 0.00 | 2.62 | 0.00 | 1.44 | 10.52 | 143.93 | -19.14 | 47.81 | 0.4369 | -655.0 | -569.0 | |
| 0.00 | 1.84 | 0.00 | 1.01 | 10.69 | 143.70 | -19.38 | 47.88 | 0.4414 | -847.0 | -580.9 | |
| 2.45 | 4.37 | 1.35 | 2.41 | 9.96 | 143.32 | -19.75 | 49.70 | 0.4382 | -1056.9 | -819.5 | |
| 0.87 | 19.06 | 0.48 | 10.52 | 10.03 | 142.96 | -20.11 | 50.08 | 0.4433 | -1035.9 | -695.1 | |
| 1.57 | 3.76 | 0.87 | 2.08 | 10.64 | 142.76 | -20.31 | 49.32 | 0.4518 | -850.3 | -733.1 | |
| 3.15 | -12.00 | 1.74 | -12.00 | 9.92 | 142.62 | -20.46 | 50.76 | 0.4464 | -819.4 | 999999 | |
| 0.00 | 2.53 | 0.00 | 1.41 | 10.53 | 142.28 | -20.79 | 50.16 | 0.4564 | -870.0 | -680.6 | |
| 0.00 | 1.22 | 0.00 | 0.67 | 8.41 | 142.38 | -20.69 | 53.82 | 0.4349 | -316.0 | -388.5 | |
| 0.00 | 0.87 | 0.00 | 0.49 | 11.18 | 141.81 | -21.26 | 49.71 | 0.4684 | 730.0 | 537.7 | |
| 0.00 | 1.49 | 0.00 | 0.83 | 9.42 | 140.76 | -22.32 | 54.08 | 0.4645 | 857.0 | 750.2 | |
| 1.57 | 3.06 | 0.88 | 1.71 | 9.24 | 140.54 | -22.53 | 54.66 | 0.4657 | 937.1 | 771.1 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 10.89 | 140.02 | -23.05 | 52.47 | 0.4869 | 788.0 | 622.4 | |
| 3.32 | 5.16 | 1.89 | 2.93 | 11.34 | 139.79 | -23.29 | 52.01 | 0.4938 | 882.3 | 661.9 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 10.14 | 139.35 | -23.72 | 54.51 | 0.4884 | 634.0 | 503.5 | |
| 0.00 | 0.87 | 0.00 | 0.50 | 10.12 | 139.12 | -23.95 | 54.81 | 0.4911 | 772.0 | 681.3 | |
| 25.52 | 54.72 | 14.58 | 31.25 | 11.07 | 139.01 | -24.06 | 53.37 | 0.5007 | 1011.6 | 536.9 | |
| 0.00 | 1.49 | 0.00 | 0.85 | 10.50 | 139.02 | -24.05 | 54.28 | 0.4956 | 904.0 | 744.2 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 10.22 | 138.98 | -24.09 | 54.80 | 0.4937 | 950.0 | 786.7 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 10.17 | 138.82 | -24.26 | 55.07 | 0.4952 | 964.0 | 726.6 | |
| 0.00 | 13.99 | 0.00 | 7.94 | 9.64 | 138.79 | -24.28 | 55.99 | 0.4911 | 547.0 | 755.4 | |
| 0.00 | 2.71 | 0.00 | 1.54 | 10.02 | 138.76 | -24.31 | 55.39 | 0.4946 | 778.0 | 642.1 | |
| 0.96 | 38.11 | 0.55 | 21.90 | 11.13 | 138.50 | -24.57 | 53.85 | 0.5073 | 661.0 | 298.8 | |
| 1.66 | -30.00 | 0.95 | -30.00 | 10.94 | 138.49 | -24.59 | 54.17 | 0.5059 | 952.1 | 999999 | |
| 2.10 | -30.00 | 1.20 | -30.00 | 10.78 | 138.50 | -24.57 | 54.41 | 0.5044 | 952.9 | 999999 | |
| 0.00 | 1.75 | 0.00 | 1.00 | 10.16 | 137.88 | -25.19 | 56.12 | 0.5068 | 626.0 | 464.5 | |
| 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. | |