Cosmic Ray Counts Hidden in Spacecraft Data Highlight Influence of Solar Cycle at Mars and Venus
Europlanet and Swedish Institute of Space Physics Joint Press Release
EMBARGOED for 11:00 UTC / noon CET on Monday, 5 December 2022
Measurements by ESA’s long-serving twin missions, Mars Express and Venus Express, have captured the dance between the intensity of high-energy cosmic rays and the influence of the Sun’s activity across our inner Solar System.
A comparison of data from the ASPERA plasma sensor, an instrument carried by both spacecraft, with the number of sunspots visible on the surface of the Sun shows how cosmic ray counts are suppressed during peaks of activity in the 11-year solar cycle. The international study, led by Dr Yoshifumi Futaana of the Swedish Institute of Space Physics, has been published today in the Astrophysical Journal.
Cosmic rays are particles travelling at almost the speed of light that originate outside our Solar System. They are a dangerous form of high energy radiation that can cause electronic failures in spacecraft and damage the DNA of humans in space.
As well as the decadal-long relationship with the solar cycle, the researchers also looked at how cosmic ray detections varied over the short timescales of an orbit. Surprisingly, they found that the area protected from cosmic rays behind Mars is more than 100 kilometres wider than the planet’s actual radius. The cause of why this blocked area should be so large is not yet clear.
“The study shows the range of valuable insights that can be derived from what is actually background count information collected by the ASPERA instruments. Understanding the various relationships between cosmic rays and the solar cycle, the atmospheres of planets and the performance of spacecraft instrumentation is very important for future robotic missions and human exploration,” said Dr Futaana.
Launched in 2003, Mars Express remains in service around the Red Planet, while Venus Express operated from 2006 until 2014. The researchers compared the 17-year dataset from Mars and eight-year dataset from Venus with Earth-based cosmic ray measurements from the Thule neutron monitor in Greenland. Scientists took median value of cosmic ray counts over three-month periods to minimise the influence of sporadic solar activity, such as flares or coronal mass ejections. The databases of background radiation counts extracted for the study have been published and can be accessed through the Europlanet SPIDER planetary space weather service (http://spider-europlanet.irap.omp.eu/).
All the datasets showed a decrease in the number of cosmic ray detections as the peak in activity for Solar Cycle 24 was reached. In particular, the Mars Express data and the observations from Earth showed very similar features. However, there was an apparent lag of around nine months between the maximum number of sunspots and the minimum in cosmic ray detections at Mars.
“Previous studies have suggested that there is a delay of several months between solar activity and the behaviour of cosmic rays at the Earth and at Mars. Our results appear to confirm this and also provide further evidence that Solar Cycle 24 was a bit unusual, perhaps due to the long solar minimum between Cycle 23 and 24, or the relatively low activity during Cycle 24,” said Dr Futaana.
The analysis of the Venus Express data has been complicated by changes in the way onboard processing was carried out from 2010 onwards. In addition, while the ASPERA instruments carried by Mars Express and Venus Express were based on a common design, they were each tailored to the very different planetary environments in which they operated. This means that a direct comparison of cosmic ray fluxes at Mars and Venus is not possible using the available datasets.
“The use of background counts to study the interaction of cosmic rays and high energy particles with planetary missions is relatively new. However, obtaining this information shows potential as a powerful tool, for example, in protecting the upcoming JUpiter Icy moon Explorer (JUICE) mission of the European Space Agency, which will explore the harsh environment around Jupiter’s icy moons,” said Nicolas Andre of the Institut de Recherche en Astrophysique et Planétologie (IRAP) in Toulouse, France, coordinator of the Europlanet SPIDER service and co-author of this study.
Futaana et al. Galactic Cosmic Rays at Mars and Venus: Temporal Variations from Hours to Decades Measured as the Background Signal of Onboard Micro-Channel Plates. The Astrophysical Journal. 2022. DOI: 10.3847/1538-4357/ac9a49
Images
Artists’ impressions of Mars Express (left) and Venus Express (right). Credit: ESA/D Ducros/AOES Medialab.
Artistic representation of galactic cosmic rays. Credit: M Eriksson/IRF.
Video
Interview with Dr Yoshifumi Futaana. https://youtu.be/5ZdwAEivOtY
Science Contacts
Dr Yoshifumi Futaana
Swedish Institute of Space Physics
Kiruna
Sweden
futaana@irf.se
Dr Nicolas André
Institut de Recherche en Astrophysique et Planétologie (IRAP)/OMP
Toulouse
France
nicolas.andre@irap.omp.eu
Media Contacts
Martin Eriksson
Information officer
Swedish Institute of Space Physics
Kiruna
+46 72 581 33 33
martin.eriksson@irf.se
Anita Heward
Press Officer
Europlanet 2024 Research Infrastructure (RI)
+44 7756 034243
aheward@europlanet-society.org
Further Information
About IRF
The Swedish Institute of Space Physics (IRF) is a governmental research institute under the Ministry of Education. IRF conducts basic research and postgraduate education in space physics, space technology, and atmospheric physics.
IRF has over 60 years of experience in developing instruments for space research projects and participates in several major international collaborative projects using satellites and ground-based equipment.
About Europlanet
Since 2005, Europlanet has provided Europe’s planetary science community with a platform to exchange ideas and personnel, share research tools, data and facilities, define key science goals for the future, and engage stakeholders, policy makers and European citizens with planetary science.
The Europlanet 2024 Research Infrastructure (RI) has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 871149 to provide access to state-of-the-art research facilities and a mechanism to coordinate Europe’s planetary science community. The project builds on a €2 million Framework 6 Coordination Action (EuroPlaNet), a €6 million Framework 7 Research Infrastructure (Europlanet RI) and a €10 million Horizon 2020 Research Infrastructure (Europlanet 2020 RI) funded by the European Commission.
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