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Interstellar neutrals slowed and warmed the solar wind beyond Pluto’s orbit

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Amit Kumar
Amit Kumar is editor-in-chief and founder of Revyuh Media. He has been ensuring journalistic quality and shaping the future of Revyuh.com - in terms of content, text, personnel and strategy. He also develops herself further, likes to learn new things and, as a trained mediator, considers communication and freedom to be essential in editorial cooperation. After studying and training at the Indian Institute of Journalism & Mass Communication He accompanied an ambitious Internet portal into the Afterlife and was editor of the Scroll Lib Foundation. After that He did public relations for the MNC's in India. Email: amit.kumar (at) revyuh (dot) com ICE : 00 91 (0) 99580 61723

Astronomers have confirmed the slowdown and heating of the solar wind flow outside Pluto’s orbit, which are associated with the capture of interstellar neutrals. Data collected from the New Horizons interplanetary station provides more information about the outer region of the heliosphere.

The current magnetohydrodynamic models of the solar wind predict that, as the particle flux moves away from the Sun, it will more and more slow down and heat up due to interaction with neutral particles from the interstellar medium, which will be ionized and captured by the solar wind. This was partially confirmed by the data obtained by the Pioneer-10, Pioneer-11, and Voyager-2 probes, as well as by devices studying the Sun and the Earth’s magnetosphere. For example, Voyager 2 detected a decrease in the solar wind speed of six per cent at distances between 25 and 40 astronomical units from the Sun and ten per cent at a distance of about sixty astronomical units from the Sun. Comparison of these data with data obtained by the IMP-8 probe operating in near-Earth orbit showed a decrease in the solar wind speed by 10 per cent at a distance of 43 astronomical units from the Sun.

Currently, the New Horizons interplanetary station, equipped with the SWAP (Solar Wind Around Pluto) tool, is the only source of data on the behaviour of the solar wind and interstellar ions outside the orbit of Mars. The device moves in the ecliptic plane and the device’s capabilities allow you to directly compare the number of interstellar gas ions captured by the solar wind and the magnitude of the deceleration and heating of the solar plasma flow in the outer part of the heliosphere.

A team of astronomers led by Heather Elliott reported on the results of an analysis of data accumulated by the SWAP instrument when New Horizons was between 21 and 42 astronomical units from the sun, and their comparison with data from ACE and STEREO, which work at a distance of about one astronomical unit from a star.

It turned out that in the range of distances from 21 to 42 astronomical units from the Sun (outside the orbit of Pluto), the density of the solar wind gradually decreases, and the temperature rises, while it turns out to be higher than expected for the adiabatic profile of the dependence of temperature on distance. The decrease in the solar wind speed due to the capture of interstellar matter for distances of 30–43 astronomical units from the Sun is from 5 to 7 per cent of the original value. Scientists have also determined that the polytropic index for the solar wind decreases linearly with increasing distance from the Sun. 

The data obtained are consistent with the simulation results. It is worth noting that it is rather difficult to determine what contributes more to the increase in the temperature of the solar wind at such distances from the Sun – interstellar neutrals or an increase in the number of particles of the fast solar wind. New Horizons is expected to cross the boundary of the shock wave, where the speed of the solar wind ceases to be supersonic, in the middle of the next decade.

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