How to pronounce “spectra” in English

Spectral changes, and very slight changes in loudness.

Spectral signatures can be identified that are diagnostic for particular landscape features.

A spectral Corey nearly tore the older women to shreds, offering her a diabolical pact to sign.

fine spectral details here.

by taking their spectra, luminosity, and by every possible means to understand what's going on there, what are the kinds of matter, in what

But we consider these spectras like sexuality, sexual orientation, gender expression, gender identity, and biological sex-- all of them fall on a spectra.

There's 268 spectra from microplastic.

And with spectra we're going to be able to tell.

and then photographing the spectra.

the plates of the spectra for her own research.

That ALICE spectra that I talked about, that instrument is actually a slit.

about reflectance spectra was about phototrophic organisms,

from the falling spectra of multiple classes around 125 GeV, about the same place of the excess that we

or two-photon mass spectra being updated with final granularity or refined style.

And here's spectra of three supernovae that I studied in the early 1990s.

and lots of spectra.

but it also took spectra of millions of objects.

There's millions of spectra that were recovered during the course of the survey.

You just take spectra of these little blobs here, all these are little galaxies.

So you take their spectra, and that gives the redshift.

So here are some spectra that my team took a little over 20 years ago.

You can get atmospheric spectra.

Once you get spectra, you can start to understand what's in their atmospheres.

The way we get spectra is we have to put a slit, a one-dimensional slit, on an image.

Dust spilled spectral red, yellow, blue, indigo, and violet, all stacked and blended together across the western sky.

You look at the spectral lines of a star, and the recoil kind of going around gives you a Doppler shift, periodic Doppler shift.

is a pure spectral yellow as a physical phenomenon.

You mentioned how useful spectral imaging could be, and I wasn't sure-- were you saying that you found a reliable source of spectral imaging in these remote areas,

So these various spectral lines, due for example to neutral sodium and hydrogen and singly ionized calcium, the whole pattern was shifted to the red.

And about 100,000 quasar spectra were analyzed by hand, by many astronomers.

So he was getting hundreds of spectra in each image.

had been set up by the spectra, that what they really signified was stellar temperature.

And then she was looking at the spectra to assess the relative abundance of different chemicals.

There's the ALICE's last spectra.

And we hope that this spectra of different pigments will help astronomers.

Those are water absorption features on these spectra.

So by getting a series of spectra over time-- from 12 days before peak brightness, in this case, to several months after peak brightness--

We really need very high resolution spectra here which just means we really stretch the light out to an extreme to get to really, really

And you'll see here the round spectra.

And just over 4 million spectra-- again, all those holes have been plugged by hand-- have been obtained mostly on galaxies.

And so we rely on spectra to nail down the difference between these two stars.

He also looked at their spectra.

And we started noticing-- we took these spectra at Lick-- we started noticing that the spectra of these things are not all identical.

And there is a particular spectral line.

Hubble Space Telescope has only limited spectral capability, but James Webb Space Telescope is going to have superb special capability.

You have no access to the spectral qualities of surfaces, but nor do you have access to inside someone's head.

And this is actually measuring cross spectral density coherence, which is a measure of the synchrony of the oscillatory activity.

And by being able to do spectral analysis of our electromagnetic-- your heart field, science now,

So we started looking for these spectral lines from aliens, and we wanted more than a one-channel receiver, which is what he used for his search in 1960.