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Posted: May 31, 2013
Researchers discover a general picture of solar storm Sun-to-Earth propagation
(Nanowerk News) True beauty lies in the sky or in space scientists’ eyes, in the vast and mysterious space with its order, extent and darkness. They explode with immense power in the solar atmosphere and are hurled out from the Sun at millions of kilometers per hour. They light up brilliant auroras in the mid-latitude skies upon impacting the Earth. Breathtakingly beautiful and yet catastrophically dangerous, they bear a name unfamiliar to the public, coronal mass ejections (CMEs).
CMEs are large-scale expulsions of ionized gas and magnetic field from the solar corona, often associated with forms of enhanced solar activity, most noticeably solar flares. They originate, in most cases, from active regions on Sun’s surface known as sunspots.
An animation from STEREO observations shows how a gigantic solar storm blows through interplanetary space. The spot with a vertical streak is the image of the Earth. (Image by Liu Ying)
CMEs are of great danger to life and technology on the Earth and in space, producing a form of solar cosmic rays, which are hazardous to spacecraft, satellites and astronauts, and disrupting power grids, satellite navigation and mobile phone networks on the Earth. These effects are now known as “space weather”, much of which is produced by CMEs propagating from the Sun into interplanetary space.
Will the Earth be hit by such large-scale ejections? Can we predict or forecast the impact so that the damage can be avoided? “These are among the top concerns of space physicists, and how CMEs propagate through the space between the Sun and Earth is key to answering these questions,” says Liu Ying, space physicist from National Space Science Center (NSSC) in Beijing, Chinese Academy of Sciences.
With data from NASA’s twin spacecraft, STEREO, Liu and his colleagues from US and Europe developed a novel technique, called geometric triangulation, which can determine the trajectory and velocity of CMEs continuously when they travel in interplanetary space ("On Sun-to-Earth Propagation of Coronal Mass Ejections"). Triangulation literally means use of two separated points to observe a third, as done in fields such as surveying and navigation. STEREO for the first time gave us those needed two “eyes” off the Sun-Earth line.
The unique capability of the geometric triangulation technique enables a detailed study of how CMEs propagate through the vast Sun-Earth space. It can also predict when a CME will reach the Earth and at what velocity. With its assistance Liu et al. discovered a scenario that seems to generalize the whole Sun-to-Earth propagation of those fast and dangerous ones: first an impulsive acceleration, then a rapid deceleration, and finally a nearly constant speed propagation or gradual deceleration.
While this general picture of CME Sun-to-Earth propagation is crucial to space weather forecasting, it also has its importance in physical understanding of solar storms and their interplanetary consequences, as Liu envisions. For example, he says: “The quick deceleration of CMEs is a surprising finding, and may change our understanding of how the energy carried by CMEs dissipates into interplanetary space.”
Based on their triangulation concept, Liu et al. further proposed an audacious yet practical strategy for space weather forecasting, which places dedicated spacecraft at L4 and L5 to make routine observations. L4 and L5, where Sun/Earth’s gravity cancels and a spacecraft can be stationary, co-move with the Earth around the Sun but lie at 60 degrees ahead and behind. “We cannot predict when and where a CME will happen on the Sun, but once a CME has occurred, we will be able to track it continuously and determine its path and velocity with the triangulation measurements, in much the same way the terrestrial weather forecast works,” says Liu.