| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.15 | 117.78 | 16.46 | 77.36 | 16.30 | 350.57 | -39.39 | 68.10 | 0.6584 | -36.1 | 107.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-06-30 17:59:11 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 | 1.27 | 0.00 | 0.77 | 19.09 | 357.71 | -32.25 | 60.28 | 0.5828 | -761.0 | -626.2 | |
| 0.00 | 1.27 | 0.00 | 0.78 | 15.72 | 355.76 | -34.19 | 66.79 | 0.5908 | -441.0 | -421.7 | |
| 0.00 | 1.18 | 0.00 | 0.77 | 20.69 | 352.88 | -37.08 | 60.69 | 0.6491 | -693.0 | -605.6 | |
| 0.00 | 0.64 | 0.00 | 0.40 | 16.53 | 353.37 | -36.59 | 66.63 | 0.6247 | -670.0 | -616.7 | |
| 0.00 | 2.18 | 0.00 | 1.40 | 18.07 | 352.89 | -37.07 | 64.52 | 0.6370 | -795.0 | -606.0 | |
| 0.00 | 1.82 | 0.00 | 1.15 | 15.77 | 353.10 | -36.86 | 67.92 | 0.6252 | -880.0 | -689.5 | |
| 0.00 | 7.63 | 0.00 | 4.86 | 16.04 | 352.72 | -37.23 | 67.66 | 0.6309 | -579.0 | -775.3 | |
| 0.00 | 1.82 | 0.00 | 1.15 | 15.61 | 352.77 | -37.18 | 68.31 | 0.6286 | -721.0 | -605.2 | |
| 0.00 | 0.73 | 0.00 | 0.46 | 15.51 | 352.60 | -37.36 | 68.54 | 0.6305 | -552.0 | -471.5 | |
| 12.26 | 22.43 | 7.87 | 14.39 | 16.19 | 352.17 | -37.79 | 67.68 | 0.6384 | -664.7 | -454.8 | |
| 0.00 | 0.73 | 0.00 | 0.48 | 19.93 | 351.11 | -38.84 | 62.65 | 0.6661 | -576.0 | -456.5 | |
| 0.00 | 0.91 | 0.00 | 0.59 | 17.97 | 351.57 | -38.38 | 65.28 | 0.6525 | -519.0 | -354.2 | |
| 3.63 | 8.35 | 2.35 | 5.41 | 16.45 | 351.58 | -38.37 | 67.52 | 0.6466 | -608.0 | -378.5 | |
| 0.00 | 3.00 | 0.00 | 1.93 | 15.33 | 351.83 | -38.12 | 69.11 | 0.6395 | -558.0 | -489.6 | |
| 0.00 | 0.91 | 0.00 | 0.59 | 16.54 | 351.19 | -38.76 | 67.55 | 0.6517 | -362.0 | -198.5 | |
| 0.00 | 1.18 | 0.00 | 0.77 | 16.65 | 350.92 | -39.04 | 67.48 | 0.6554 | -413.0 | -317.5 | |
| 0.00 | 1.09 | 0.00 | 0.71 | 16.25 | 351.02 | -38.94 | 68.05 | 0.6528 | 651.0 | 497.7 | |
| 0.00 | 2.72 | 0.00 | 1.81 | 18.69 | 350.26 | -39.70 | 64.80 | 0.6710 | -551.0 | -444.1 | |
| 0.00 | 0.64 | 0.00 | 0.42 | 18.44 | 350.29 | -39.67 | 65.15 | 0.6696 | -467.0 | -430.4 | |
| 0.00 | 1.54 | 0.00 | 1.02 | 16.38 | 350.28 | -39.67 | 68.13 | 0.6622 | 354.0 | 266.7 | |
| 1.82 | 8.44 | 1.20 | 5.58 | 15.71 | 349.87 | -40.09 | 69.26 | 0.6651 | 870.1 | 633.1 | |
| 0.00 | 2.54 | 0.00 | 1.68 | 15.40 | 349.94 | -40.01 | 69.69 | 0.6633 | 802.0 | 577.4 | |
| 0.00 | 0.73 | 0.00 | 0.48 | 16.05 | 349.62 | -40.34 | 68.86 | 0.6692 | 763.0 | 685.5 | |
| 1.82 | 15.34 | 1.21 | 10.28 | 15.92 | 349.44 | -40.51 | 69.11 | 0.6710 | 868.5 | 628.5 | |
| 0.00 | 1.27 | 0.00 | 0.84 | 15.39 | 349.53 | -40.43 | 69.85 | 0.6683 | 687.0 | 606.6 | |
| 0.00 | 1.27 | 0.00 | 0.85 | 15.70 | 349.41 | -40.54 | 69.44 | 0.6706 | 734.0 | 628.7 | |
| 1.54 | -24.00 | 1.04 | -24.00 | 16.28 | 348.85 | -41.11 | 68.80 | 0.6792 | 742.2 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.79 | 14.52 | 348.93 | -41.02 | 71.30 | 0.6730 | 698.0 | 604.9 | |
| 0.00 | 3.90 | 0.00 | 2.62 | 14.67 | 348.65 | -41.31 | 71.18 | 0.6769 | 508.0 | 629.4 | |
| 0.00 | 0.91 | 0.00 | 0.61 | 14.45 | 348.70 | -41.26 | 71.48 | 0.6757 | 749.0 | 702.5 | |
| 0.36 | 14.71 | 0.25 | 10.03 | 17.10 | 347.99 | -41.97 | 67.92 | 0.6920 | 754.0 | 799.8 | |
| 3.72 | -31.00 | 2.54 | -31.00 | 16.54 | 348.10 | -41.86 | 68.68 | 0.6889 | 842.0 | 999999 | |
| 0.00 | 1.09 | 0.00 | 0.73 | 13.74 | 348.73 | -41.22 | 72.51 | 0.6735 | 708.0 | 622.1 | |
| 0.00 | 1.09 | 0.00 | 0.75 | 16.78 | 347.77 | -42.18 | 68.45 | 0.6935 | 523.0 | 427.2 | |
| 0.00 | 2.09 | 0.00 | 1.45 | 18.13 | 347.34 | -42.61 | 66.72 | 0.7027 | 795.0 | 611.4 | |
| 0.00 | 1.18 | 0.00 | 0.81 | 16.15 | 347.86 | -42.10 | 69.31 | 0.6906 | 601.0 | 533.0 | |
| 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. | |