The cold pole problem is due largely to the absence of gravity-wave forcing, which many models now include. ❋ Unknown (2009)
Differences in gravity-wave and planetary-wave simulations as well as model resolution can lead to very different projections of polar temperatures and transport of ozone to the poles. ❋ Unknown (2009)
For future possibilities we highlighted two vision missions: a Big Bang Observer to directly detect the gravity-wave background from inflation, and a Black Hole Imager to resolve X-rays from right next to the event horizons of black holes. ❋ Sean (2007)
Might gravity-wave detectors eventually give us a way of directly observing dark matter in this way? ❋ Sean (2007)
How likely is it that gravity-wave detectors, say a future version of something like LISA, might eventually allow us to specifically observe the locations and quantities of dark matter involved in formations like this? ❋ Sean (2007)
And even though they've all moved on to greater things, like retiring from movies forever or making dull-looking films about gravity-wave strengths and their temporal signatures as observed on the Earth or, um, Firewall – Indiana Jones 4 has never been too far from the surface. ❋ Unknown (2007)
But, although it must be galling for Steven Spielberg to see all his carefully-kept secrets being spewed everywhere, at least there's a plus side to all this – Spielberg is going to make damn sure that nobody steals any secrets from his film about gravity-wave strengths and their temporal signatures as observed on the Earth, possibly because we can't see anyone actually going to see it after it's been released anyway. ❋ Unknown (2007)
A film about gravity-wave strengths and their temporal signatures as observed on the Earth, that's what. ❋ Unknown (2006)
"They could measure the effects of shadow matter on their system," Peter said, "and they could record the gravity-wave messages and when they interpreted the messages properly, the ships they built worked, and they were propelled toward their remote destinations by unseen forces." ❋ Unknown (2004)
One screen displayed stars and other stellar phenomena, not according to their output of visible light, but in gravity-wave sche'matics. ❋ Foster, Alan Dean (1979)
The team must keep its detectors at a chilling minus 253 degrees Celsius (minus 423 degrees Fahrenheit, close to absolute zero) to boost the odds of detecting the extremely weak gravity-wave signals. ❋ Unknown (2009)
We’re still looking for the gravity-wave/tensor perturbations. ❋ Sean (2006)
They weren’t designed for any other purpose, and Geordi could see that they would need extensive modifications before they could serve as gravity-wave emitters. ❋ W.R. THOMPSON (2000)
