Every eleven years on average, around the peak in the
solar-terrestrial activity cycle, there are great magnetic storms
which disrupt regional electrical power systems, interfere
(sometimes fatally) with commercial and government satellites,
expose astronauts to radiation hazard, and spread aurorae from
their polar home across the skies of temperate climes. Quick to
respond, the news media consult experts at appropriate
observatories, universities or government agencies and report,
"Scientists say that last nights extraordinary display of
the northern lights was caused by the explosion on the Sun of a
violent solar flare".
Wrong, says Jack Gosling (Los Alamos National Laboratory),
whose year-long efforts to spread a new gospel of
solar-terrestrial lore culminated with the publication of his
article "The solar flare myth" (J. geophys. Res 98,
18937-18949; 1993), and the success of a session he organised for
a meeting in December 1993 entitled, innocently enough "The
solar-terrestrial connection". The article and session
conveyed a revolutionary message: solar flares do not cause
magnetic storms and attendant auroral displays, nor do they cause
most of the associated, hazardous fluxes of solar energetic
particles; coronal mass ejections do.
The traditional version of causal chin for
solar-terrestrial events.
Coronal mass ejections are rapid reconfigurations of
coronal structures that involve the ejection into the solar wind
of immense quantities (even by solar standards) of coronal
material. Detectable only from space-borne coronographs -
instruments that eclipse the Suns bright disk - they appear
as gigantic loop-like bubbles subtending up to a quarter of the
Suns circumference. The bubbles lift off into space,
leaving behind only bright legs rooted to the sun. As coronal
mass ejections are space-age latecomers to the
solar-terrestrial scene (they were discovered in the early
1970s), space physicists are only now appreciating their central
relevance to the field.
So explained the sessions lead speaker, Steve Kahler
(Air Force Phillips Laboratory), who traced the history of
studies that established a clear, although far from perfect,
correlation between flares and aurorae, or more commonly between
flares and the magnetic storms that accompany aurorae. The reason
that the misconception about flares is so entrenched in
solar-terrestrial physics, he argued, is that correlation was
mistaken for cause, a textbook case of the famous logical
fallacy. Usually establishing correlation is the first step
towards establishing cause. But in the case of flares and
aurorae, both are side-effects of a common cause, coronal mass
ejections (see Fig. 2).
The revised version of causal chin for
solar-terrestrial events
On the other hand, not all flares are cause by coronal mass
ejections, as flares occur much more frequently. Art
Hundhausen (NCAR High Altitude Observatory) explained that flares
may be cause by "magnetic reconnection", a process in
which magnetic fields pointing in opposite directions annihilate
each other and release energy in the form of X-rays and energetic
particles. Because the solar surface is constantly in motion,
like a boiling liquid, and because its rotation rate is not
uniform in latitude or with depth, its embedded magnetic fields
are constantly shifting, deforming and twisting on a hierarchy of
scale sizes. As a result, oppositely directed magnetic fields are
frequently brought together, triggering reconnection and
consequent flares. Coronal mass ejections involve a
specific form of large-scale magnetic field deformation. As a
mass ejection rises off the surface, it draws out the oppositely
directed magnetic fields in the legs of its loop-like form, which
can then reconnect and cause a flare. Thus flares can be
side-effects of coronal mass ejections as well as a common
phenomenon elsewhere on the Sun.
Don Reames (NASA Goddard Space Flight Center) corrected the
misconception that flares produce large-scale expulsions of solar
energetic particles. Although flares do impart energy to
particles (possibly directly through reconnection or indirectly
by generating instabilities and shock waves in the corona), the
huge shock waves that fast coronal mass ejections push
before them can energize particles on a much grander scale.
Particles accelerated by these shocks can be distinguished from
those associated with flares through measurements of composition
and charge state. These show that flare-associated particles are
limited to narrow cone angles, where as ejection-association
particles can span cones covering half of interplanetary space.
Jack Gosling adduced convincing evidence that coronal mass
ejections cause all of the larger magnetic storms and
accompanying aurorae. The properties of mass ejections
responsible for storms are the strength and configuration of
their magnetic fields, and their high speeds - not the energetic
particles, contrary to most popular and some scientific accounts.
The magnetic field in the quiet solar wind usually lies in the
ecliptic plane. But the loop-like fields in mass ejections
have strong, north-south components.
As the Earths magnetic field points northward, any
oncoming southward fields reconnect with it; and the stronger the
fields and the faster they approach, the faster the reconnection
rate. Without reconnection, the Earths field acts as a
barrier to shield the near-Earth region, the magnetosphere, from
the solar wind. But reconnection breaks the barrier and allows
solar wind particles and energy to pour into the magnetosphere at
a rate proportional to the reconnection rate. Through a series of
magnetospheric processes, the energy gained drives the currents
that make the magnetic storm and accelerates both the
infiltrating solar wind particles and local particles to create
the aurorae. So although it is true that aurorae are caused by
energetic particles, they are locally energized from those
associated with mass ejections and flares.
Thanks to Gosling, a new solar-terrestrial exhibit planned for
the Smithsonians Air and Space Museum in Washington DC will
get the flare story right. Early exhibit plans that actually
promulgated the "solar flare myth" are what sparked his
revisionist crusade. The exhibit now recognizes the central role
of coronal mass ejections. Although solar flares are
intrinsically interesting phenomena, and predictions of their
occurrence are important for protecting space travellers from
potentially lethal X-ray doses, we now understand that they do
not cause aurorae, magnetic storms or major energetic particle
events.
Nancy Crooker is at the Center for Space Physics, Boston
University, Boston, Massachusetts 02215, USA.
UKSMG Six News issue
44,
Jan 1995 |
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