32. http://www.aaa.org/s932/images/09fallclass2.pdf
... velocity = dark blue transit = dark green timing = dark purple astrometry = dark yellow direct imaging = dark red microlensing = dark orange 1990 1995 2000 2005 Detection Methods * Radial velocity or Doppler method: Variations in the speed with which the ...
33. http://www.izmiran.rssi.ru/~obridko/papers/435eng.pdf
... Coronal mass ejections are often related to flares and represent a magnetic cloud that approaches the Earth at a rela tively high velocity (6001000) km/s. These ejections usually have a sharp leading front and result in the origination of magnetic storms ...
34. Metagalaxy sector, archive 2011
... Service . Contacts . 2011: . Detection of galaxies with large peculiar velocities . ... with large negative peculiar velocities are distributed quite inhomogeneously over ...
37. http://www.astro-soc.odessa.ua/Program-2006.pdf
... excess one E-plane in the microwave (Naselski) and infrared (Hauser) diapasons, as well as the giant molecular clouds Taurus, r Oph, etc, the filaments of the high velocity HI (HVC) the parallel to the E-layers the density waves for any observer ...
38. Achievements - Page 3
... of giant planets with velocity w = (0.1-0.5) m/s determines the capacity of visible clouds and therefore affects their ... high density packing of particles, that can explain the observations, obtained for a number of solar system bodies (such as ...