Lab astrophysics aims for the stars
2012-11-25 05:51:56
Earth experiments deployed to understand data from space.
The giant orange magnets were built decades ago to confine hydrogen nuclei in
the quest for fusion energy. But since 1998, Jan Egedal, a plasma physicist at
the Massachusetts Institute of Technology in Cambridge, has used the magnets,
from a massive, doughnut-shaped tokamak, to simulate magnetic fields in the thin
wind of charged particles streaming from the Sun. Egedal hopes to learn how the
solar wind transfers energy.
In the past, أ¢â‚¬ثœlaboratory astrophysicsأ¢â‚¬â„¢ experiments such as Egedalأ¢â‚¬â„¢s أ¢â‚¬â€ efforts to
mimic the behaviour of space plasmas and other astrophysical phenomena أ¢â‚¬â€ have
had to piggyback on the apparatus of energy research or fundamental physics.
Now, practitioners are trying to enshrine the field as a discipline in its own
right, with dedicated funding and equipment. In June, the American Astronomical
Society (AAS) in Washington DC created its first new division in 30 years,
dedicated to lab astrophysics. The American Physical Societyأ¢â‚¬â„¢s plasma-physics
meeting last month in Providence, Rhode Island, saw an unprecedented number of
lab-astrophysics sessions. And some NASA scientists are saying that the agency
should devote a small amount of funding from every space mission to lab
astrophysics. أ¢â‚¬إ“Thereأ¢â‚¬â„¢s an increasing number of papers on lab astrophysics,أ¢â‚¬آ says
Fred Skiff, a plasma physicist at the University of Iowa in Iowa City, who
chaired the physical-society meeting. أ¢â‚¬إ“Itأ¢â‚¬â„¢s come of age.أ¢â‚¬آ
One goal is to make the most of the data streaming in from spacecraft. Egedal,
for example, is exploring questions posed by two solar-wind missions: the
European Space Agencyأ¢â‚¬â„¢s Cluster and NASAأ¢â‚¬â„¢s Wind. أ¢â‚¬إ“Weأ¢â‚¬â„¢re in the heyday of Solar
System spacecraft, and thatأ¢â‚¬â„¢s fuelled the growth of lab-astrophysics
experiments,أ¢â‚¬آ he explains. Farid Salama, a lab astrophysicist at NASAأ¢â‚¬â„¢s Ames
Research Center in Moffett Field, California, says that the work is also
attractive in times of tight budgets, because the cost of experiments tends to
be hundreds of thousands of dollars, compared with hundreds of millions for
space missions.
Significant results are emerging. Last month, Skiff and his colleagues described
the first lab measurement of astrophysical turbulence in which two magnetic
waves collide to generate a third one أ¢â‚¬â€ a phenomenon that has been invoked to
explain why the Sunأ¢â‚¬â„¢s atmosphere, or corona, is thousands of time hotter than
its surface and how massive amounts of energy move between galaxies. Using the
Large Plasma Device, a 21-metre-long plasma generator at the University of
California, Los Angeles, Skiff made two of these أ¢â‚¬ثœAlfvأƒآ©nأ¢â‚¬â„¢ waves, collided them
and mapped the daughter wave, confirming the mechanism (G. G. Howes et al. Phys.
Rev. Lett. Preprint at http://arxiv.org/abs/1210.4568; 2012). أ¢â‚¬إ“This is the first
clear lab demo of something that is a cornerstone of theory,أ¢â‚¬آ says Amitava
Bhattacharjee, a theoretical astrophysicist at Princeton University in New
Jersey. The experiment cost less than US$100,000.
NASA has always funded some lab astrophysics, but Salama says that the agency
should consider doing so as a matter of course for all space missions. A good
first candidate for this funding model, he says, would be work connected with
the Herschel Space Observatory, a European mission with NASA involvement that is
collecting infrared spectra from thousands of different molecules in Galactic
clouds of dust and gas. Many of the molecules have yet to be identified, but
researchers could pin them down by synthesizing candidates and checking their
spectra in the lab. Daniel Savin, an astrochemist at Columbia University in New
York who was involved in the creation of the AAS lab-astrophysics division, says
that theoretical work in lab astrophysics is also needed to set priorities for
which experiments to do. For example, synthesizing every possible molecule that
might be observed in space is not financially feasible. Models of cloud
chemistry could guide the work by indicating which are the most important.
Dedicated funding for lab astrophysics would be good news for Egedal, who is
beginning to outgrow his current apparatus. His group has predicted the
existence of a plasma regime in which electrons can be unexpectedly and
powerfully energized, a previously unexplained effect seen by spacecraft
observing the solar wind. But to explore the mechanism, he needs to do
experiments using a larger volume of plasma and higher magnetic fields (J.
Egedal et al. Nature Phys. 8, 321أ¢â‚¬â€œ324; 2012). If lab astrophysics establishes
itself as a worthy discipline, he might be able to graduate from his
hand-me-down tokamak, he says. أ¢â‚¬إ“I want to build a new one.أ¢â‚¬آ
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