| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.02 | 225.50 | 34.56 | 136.63 | 7.49 | 134.61 | 32.07 | 294.13 | 0.5789 | 110.0 | -55.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-03 06:43:58 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 | 1.21 | 0.00 | 0.79 | 5.54 | 141.67 | 39.13 | 287.09 | 0.6595 | -555.0 | -494.0 | |
| 0.00 | 2.07 | 0.00 | 1.31 | 2.68 | 139.86 | 37.33 | 283.59 | 0.6254 | -83.0 | -73.8 | |
| 0.00 | 2.16 | 0.00 | 1.37 | 3.99 | 139.73 | 37.20 | 285.68 | 0.6287 | -611.0 | -546.3 | |
| 0.00 | 1.73 | 0.00 | 1.09 | 4.09 | 139.44 | 36.91 | 285.96 | 0.6253 | -657.0 | -589.3 | |
| 0.00 | 3.02 | 0.00 | 1.89 | 7.10 | 137.26 | 34.72 | 291.74 | 0.6108 | 592.0 | 367.2 | |
| 0.00 | 1.12 | 0.00 | 0.70 | 7.34 | 137.17 | 34.64 | 292.15 | 0.6109 | -466.0 | -389.7 | |
| 4.75 | 31.28 | 2.97 | 19.47 | 7.84 | 137.00 | 34.47 | 293.03 | 0.6114 | -707.1 | -739.4 | |
| 1.21 | -7.00 | 0.75 | -7.00 | 7.66 | 136.95 | 34.41 | 292.78 | 0.6097 | -819.3 | 999999 | |
| 0.35 | -7.00 | 0.21 | -7.00 | 7.31 | 136.80 | 34.27 | 292.34 | 0.6061 | -797.0 | 999999 | |
| 2.85 | -7.00 | 1.77 | -7.00 | 7.49 | 136.78 | 34.25 | 292.63 | 0.6068 | -995.3 | 999999 | |
| 0.00 | 1.56 | 0.00 | 0.96 | 7.18 | 136.72 | 34.19 | 292.19 | 0.6043 | -772.0 | -605.4 | |
| 2.68 | -7.00 | 1.67 | -7.00 | 7.76 | 136.66 | 34.13 | 293.12 | 0.6067 | -994.9 | 999999 | |
| 0.60 | 4.49 | 0.37 | 2.78 | 7.05 | 136.56 | 34.03 | 292.09 | 0.6016 | -830.0 | -662.5 | |
| 1.99 | 7.00 | 1.24 | 4.37 | 8.40 | 136.62 | 34.08 | 294.12 | 0.6097 | -825.0 | -627.0 | |
| 0.00 | 0.86 | 0.00 | 0.53 | 6.62 | 136.13 | 33.60 | 291.69 | 0.5938 | -689.0 | -509.6 | |
| 0.00 | 1.21 | 0.00 | 0.74 | 8.24 | 135.59 | 33.06 | 294.56 | 0.5958 | -203.0 | -162.7 | |
| 0.00 | 1.21 | 0.00 | 0.74 | 8.45 | 135.54 | 33.01 | 294.92 | 0.5963 | 502.0 | 343.1 | |
| 2.85 | 6.57 | 1.73 | 3.98 | 6.66 | 134.99 | 32.46 | 292.49 | 0.5791 | -943.8 | -700.8 | |
| 0.00 | 2.07 | 0.00 | 1.27 | 8.20 | 135.01 | 32.48 | 294.89 | 0.5882 | -733.0 | -556.5 | |
| 0.00 | 0.52 | 0.00 | 0.32 | 8.47 | 134.93 | 32.40 | 295.37 | 0.5888 | 278.0 | 279.0 | |
| 1.12 | 150.34 | 0.68 | 90.09 | 7.72 | 134.33 | 31.80 | 294.63 | 0.5766 | 499.7 | 132.6 | |
| 0.69 | -21.00 | 0.42 | -21.00 | 7.06 | 134.07 | 31.53 | 293.76 | 0.5693 | 578.2 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.52 | 8.86 | 133.91 | 31.37 | 296.74 | 0.5782 | 661.0 | 577.8 | |
| 7.43 | -21.00 | 4.47 | -21.00 | 7.93 | 133.79 | 31.25 | 295.36 | 0.5708 | 783.8 | 999999 | |
| 19.96 | -21.00 | 11.98 | -21.00 | 7.46 | 133.71 | 31.18 | 294.67 | 0.5671 | 884.4 | 999999 | |
| 3.63 | -21.00 | 2.17 | -21.00 | 6.97 | 133.64 | 31.10 | 293.92 | 0.5631 | -847.5 | 999999 | |
| 0.00 | 2.59 | 0.00 | 1.56 | 8.48 | 133.24 | 30.70 | 296.65 | 0.5672 | 586.0 | 527.3 | |
| 0.00 | 1.12 | 0.00 | 0.67 | 8.50 | 133.06 | 30.53 | 296.81 | 0.5651 | 589.0 | 543.8 | |
| 6.05 | -21.00 | 3.61 | -21.00 | 7.97 | 132.98 | 30.45 | 296.03 | 0.5607 | 869.1 | 999999 | |
| 0.86 | -21.00 | 0.52 | -21.00 | 8.42 | 132.81 | 30.28 | 296.89 | 0.5614 | 896.6 | 999999 | |
| 0.00 | 1.56 | 0.00 | 0.92 | 8.08 | 132.30 | 29.76 | 296.75 | 0.5526 | 754.0 | 699.7 | |
| 0.00 | 0.95 | 0.00 | 0.56 | 7.33 | 131.58 | 29.05 | 296.09 | 0.5384 | 678.0 | 579.1 | |
| 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. | |