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Discovery of waves in Jupiter's magnetosphere

25.07.2023

During nearly half of Jupiter's magnetosphere boundary crossings, the Juno space station encounters waves that cause the planet's magnetic field to interact with the solar wind, according to a new study. This phenomenon was previously detected on Earth and Saturn, but was first recorded on Jupiter.

Jupiter has the strongest magnetic field of all the planets in the solar system, surpassing the Sun by almost 15 times. Its magnetic field accelerates charged particles that enter the magnetosphere from the solar wind or are ejected by the moon Io. This is manifested in the bright auroras and unique dawn storms that the Juno space station has been studying for more than seven years. With the help of this station, astronomers from the University of Texas at San Antonio, together with colleagues, discovered a hitherto unknown phenomenon on Jupiter - Kelvin-Helmholtz instabilities.

Kelvin-Helmholtz instabilities occur at the boundary of two media with different velocities and directions, causing eddies. These wave structures can be observed on the surface of the water during strong winds, in the atmosphere of the Sun, and in the magnetospheres of the Earth and Saturn when they collide with streams of charged particles from the Sun.

However, waves in Jupiter's magnetosphere were discovered for the first time. Their presence was confirmed by the analysis of data on the flow of charged particles around Jupiter, received from the Juno, as well as plasma measurements during the station's passage through the planet's magnetopause - the boundary separating the magnetosphere and the environment.

Planetary scientists have found that in 25 out of 62 magnetopause crossings, the conditions around Juno met the requirements for the occurrence of Kelvin-Helmholtz instabilities. Scientists suggest that the resulting waves contribute to the transfer of solar wind particles deep into the planet's magnetosphere, influencing the local structure of the magnetic field and other processes. The researchers hope their study will help better understand Jupiter's magnetic field and how it interacts with space weather.

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Solar reactor produces hydrogen and captures waste 24.04.2023

EPFL engineers have built and tested a solar reactor that can generate hydrogen from sunlight and water. The system is not only highly efficient in producing hydrogen, but also captures oxygen and heat waste to also be used.

Hydrogen is set to become a key player in renewable energy, and one of the most efficient ways to produce it is to break down water into its constituent molecules. When this process is carried out using solar energy, it is called artificial photosynthesis, and this is the process that the new reactor uses.

The EPFL reactor looks like a satellite dish, and it works on a similar principle - a large curved surface collects as much light as possible and concentrates it on a small device suspended in the middle. In this case, the dish collects heat from the Sun and focuses it about 800 times on the photoelectrochemical reactor. Water is pumped into this reactor, where solar energy is used to split molecules into hydrogen and oxygen.

The reactor also captures two waste products of the process that are usually freshly released - oxygen and heat. Oxygen can be useful for hospitals or industrial uses, while heat passes through a heat exchanger and can be used to heat water or the interior of a building.

The reactor was tested on the EPFL campus for 13 days in August 2020, February and March 2021 to see how it performs under different weather conditions. Its solar-to-hydrogen efficiency has been found to average over 20%, producing about 500 g (1,1 lb) of hydrogen per day. The team says that with this capacity, for a year, the system could power 1,5 vehicles on medium-distance hydrogen fuel cells, or provide about half of the electricity needs of a household of four.

"With an output power of over 2 kilowatts, we have exceeded the 1 kilowatt limit for our pilot reactor while maintaining a record high efficiency for this large scale," said Sophia Haussener, corresponding author of the study. "The rate of hydrogen production achieved in this work is indeed an encouraging step towards the commercialization of this technology."

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