«We are looking at several cubic miles of lava in rapidly emplaced flows,» said Davies, who has developed models to predict the volume of magma erupted based
on spectroscopic observations.
The appearance of the plumes in this graphic is based
on spectroscopic observations of oxygen and hydrogen in the auroral emissions.
Not exact matches
Measurements of surface chemical composition, either by direct sampling (as has been done
on Earth, the moon, and Mars) or through
spectroscopic observations, can be used to estimate elemental abundances and the degree of chemical differentiation that occurred as the planets condensed from the solar nebula.
Recently, Hallinan et al. (2015) reported simultaneous radio and optical
spectroscopic observations (obtained with the Karl G. Jansky Very Large Array (VLA) radio telescope and the Double Spectrograph (DBSP)
on the 5.1 - m Hale telescope, respectively) of auroral emissions of an object at the end of the stellar main sequence (i.e. at the boundary between stars and brown dwarfs).
Spectroscopic observations from the W. M. Keck Observatory
on Maunakea, Hawaii and the Very Large Telescope in Chile confirmed the four candidates to be massive clusters.
The
spectroscopic observations provided redshifts for the sources and information
on their gas content (the fuel for star formation).
With photometric and
spectroscopic observations, we have been able to learn about the surface properties and the physical processes acting
on these large planetoids.
By using advanced high contrast imagers, it is possible to conduct high resolution spectroscopy
on imageable exoplanets, after the star light is first suppress... ▽ More
Spectroscopic observations are extremely important for determining the composition, structure, and surface gravity of exoplanetary atmospheres.
Using the twin telescopes of the Keck Observatory
on Maunakea, Hawaii, the researchers were able to gather
spectroscopic data from the afterglow of the supernova and
observations of its host galaxy to better understand what might be driving this oddity.
Current research in the Hida Observatory of Kyoto University has emphasis
on the followings; (a) Study of solar MHD processes with
spectroscopic and spectro - polarimetric
observations using the 60 cm Domeless Solar Vacuum Tower Telescope (DST) combining with data from space solar missions (such as Hinode).
The «clear sky radiative forcing due to CO2» (3.7 W / m ^ 2 for a doubling per Myhre et al. 1998b and IPCC TAR) is not a measured entity based
on empirical data from actual physical
observations or reproducible experimentation, but rather an estimated value based
on laboratory studies of
spectroscopic data.