Tracking a solar eruption through the solar system

August 15, 2017

WASHINGTON D.C. -- Ten spacecraft, from ESA's Venus Express to NASA's Voyager-2, felt the effect of a solar eruption as it washed through the solar system while three other satellites watched, providing a unique perspective on this space weather event.

Scientists working on ESA's Mars Express were looking forward to investigating the effects of the close encounter of Comet Siding Spring on the Red Planet's atmosphere on October 19, 2014, but instead they found what turned out to be the imprint of a solar event.

While this made the analysis of any comet-related effects far more complex than anticipated, it triggered one of the largest collaborative efforts to trace the journey of an interplanetary coronal mass ejection - a CME - from the sun to the far reaches of the outer solar system.

Although Earth itself was not in the firing line, a number of sun-watching satellites near Earth - ESA's Proba-2, the ESA/NASA SOHO and NASA's Solar Dynamics Observatory - had witnessed a powerful solar eruption a few days earlier, on October 14, 2014.

NASA's STEREO-A not only captured images of the other side of the sun with respect to Earth, but also collected in situ information as the CME rushed passed.

Thanks to the fortuitous locations of other satellites lying in the direction of the CME's travel, unambiguous detections were made by three Mars orbiters - ESA's Mars Express, NASA's MAVEN and Mars Odyssey - and NASA's Curiosity Rover operating on the Red Planet's surface, ESA's Rosetta at Comet 67P/Churyumov-Gerasimenko, and the international Cassini mission at Saturn.

Hints were even found as far out as NASA's New Horizons, which was approaching Pluto at the time, and beyond to Voyager-2. However, at these large distances it is possible that evidence of this specific eruption may have merged with the background solar wind.

"CME speeds with distance from the sun is not well understood, in particular in the outer solar system," said Olivier Witasse, a planetary scientist for the European Space Agency and lead author of the study published in Journal of Geophysical Research: Space Physics, a journal of the American Geophysical Union. "Thanks to the precise timings of numerous in situ measurements, we can better understand the process, and feed our results back into models."

The measurements give an indication of the speed and direction of travel of the CME, which spread out over an angle of at least 116 degrees to reach Venus Express and STEREO-A on the eastern flank, and the spacecraft at Mars and Comet 67P Churyumov-Gerasimenko on the western flank.

From an initial maximum of about 1000 kilometers per second (621 miles per second) estimated at the sun, a strong drop to 647 kilometers per second (402 miles per second) was measured by Mars Express three days later, falling further to 550 kilometers per second (342 miles per second) at Rosetta after five days. This was followed by a more gradual decrease to 450-500 kilometers per second (280-311 miles per second) at the distance of Saturn a month since the event.

The data also revealed the evolution of the CME's magnetic structure, with the effects felt by spacecraft for several days, providing useful insights on space weather effects at different planetary bodies. The signatures at the various spacecraft typically included an initial shock, a strengthening of the magnetic field, and increases in the solar wind speed.

In the case of ESA's Venus Express, its science package was not switched on because Venus was "behind" the sun as seen from Earth, limiting communication capabilities. A faint indication was inferred from its star tracker being overwhelmed with radiation at the expected time of passage.

Furthermore, several craft carrying radiation monitors - Curiosity, Mars Odyssey, Rosetta and Cassini - revealed an interesting and well-known effect: a sudden decrease in galactic cosmic rays. As a CME passes by, it acts like a protective bubble, temporarily sweeping aside the cosmic rays and partially shielding the planet or spacecraft.

A drop of about 20 percent in cosmic rays was observed at Mars - one of the deepest recorded at the Red Planet - and persisted for about 35 hours. At Rosetta, a reduction of 17 percent was seen that lasted for 60 hours, while at Saturn the reduction was slightly lower and lasted for about four days. The increase in the duration of the cosmic ray depression corresponds to a slowing of the CME and the wider region over which it was dispersed at greater distances.

"The comparison of the decrease in galactic cosmic ray influx at three widely separated locations due to the same CME is quite novel," Witasse said. "While multispacecraft observations of CMEs have been done in the past, it is uncommon for the circumstances to be such to include so many spread across the inner and outer solar system like this."

"Finally, coming back to our original intended observation of the passage of Comet Siding Spring at Mars, the results show the importance of having a space weather context for understanding how these solar events might influence or even mask the comet's signature in a planet's atmosphere," he said.
The American Geophysical Union is dedicated to advancing the Earth and space sciences for the benefit of humanity through its scholarly publications, conferences, and outreach programs. AGU is a not-for-profit, professional, scientific organization representing 60,000 members in 137 countries. Join the conversation on Facebook, Twitter, YouTube, and our other social media channels.

American Geophysical Union

Related Mars Articles from Brightsurf:

Water on ancient Mars
A meteorite that originated on Mars billions of years ago reveals details of ancient impact events on the red planet.

Surprise on Mars
NASA's InSight mission provides data from the surface of Mars.

Going nuclear on the moon and Mars
It might sound like science fiction, but scientists are preparing to build colonies on the moon and, eventually, Mars.

Mars: Where mud flows like lava
An international research team including recreated martian conditions in a low-pressure chamber to observe the flow of mud.

What's Mars made of?
Earth-based experiments on iron-sulfur alloys thought to comprise the core of Mars reveal details about the planet's seismic properties for the first time.

The seismicity of Mars
Fifteen months after the successful landing of the NASA InSight mission on Mars, first scientific analyses of ETH Zurich researchers and their partners reveal that the planet is seismically active.

Journey to the center of Mars
While InSight's seismometer has been patiently waiting for the next big marsquake to illuminate its interior and define its crust-mantle-core structure, two scientists, have built a new compositional model for Mars.

Getting mac and cheese to Mars
Washington State University scientists have developed a way to triple the shelf life of ready-to-eat macaroni and cheese, a development that could have benefits for everything from space travel to military use.

Life on Mars?
Researchers from Hungary have discovered embedded organic material in a Martian meteorite found in the late 1970s.

New evidence of deep groundwater on Mars
Researchers at the USC Arid Climate and Water Research Center (AWARE) have published a study that suggests deep groundwater could still be active on Mars and could originate surface streams in some near-equatorial areas on Mars.

Read More: Mars News and Mars Current Events is a participant in the Amazon Services LLC Associates Program, an affiliate advertising program designed to provide a means for sites to earn advertising fees by advertising and linking to