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The ESA's Solar Orbiter will work with Parker. In order to get its orbit close to the Sun, both the Solar Orbiter and Parker will use the gravity from Venus. The Solar Orbiter will collect contextual information to help us understand the in situ measurements Parker gives.

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Solar Wind Electrons Alphas and Protons Investigation

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Solar Wind Electrons Alphas and Protons Investigation

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SWEAP will count protons, helium ions, and electrons and measure their density, velocity, and temperature.

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The WISPR experiment is a group of telescopes that will take pictures of solar wind, the inner heliosphere, shocks, the Sun’s corona, and other things when they pass the Parker Solar Probe.

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Integrated Science Investigation of the Sun

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Integrated Science Investigation of the Sun

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The IS☉IS observes heavy ions, energetic electrons, and protons and associates them with coronal structures and solar wind.

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The FIELDS experiment will measure the waves and fields of electricity and magnetism, Poynting flux, electron temperature, density of plasma, radio emissions, density fluctuations, and the potential of floating spacecraft.

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Both solar wind and energetic particles affect space weather. Space weather influences the lifetime and orbit of a satellite and the electronics that are on them.

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Energetic particles are particles with high energy that are dangerous to both satellites and astronauts.

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How Can Parker Solar Probe Get So Close to the Sun?

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The goal of the Parker Solar Probe is to study how heat and energy move through the Sun's corona and what stimulates energetic particles and solar wind. The spacecraft will also take pictures of solar wind.

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There's a wind that emanates from the Sun, and it blows not like a soft whistle but like a hurricane's scream. Made of electrons, protons and heavier ions, the solar wind courses through the solar system at roughly 1 million mph (1.6 million kph), barreling over everything in its path.

Yet through the wind's roar, NASA's Parker Solar Probe hears the small chirps, squeaks and rustles that hint at the origin of this mysterious and ever-present wind. And now the Parker Solar Probe team is getting their first chance to hear them, too.

"We are looking at the young solar wind, being born around the Sun," said mission Project Scientist Nour Raouafi, from the Johns Hopkins Applied Physics Laboratory (APL), in Laurel, Maryland. "And it's completely different from what we see here near Earth."

Scientists have studied the solar wind for more than 60 years, but they're still puzzled over some of its behaviors. While they know it comes from the Sun's million-degree upper atmosphere called the corona, the solar wind, for example, doesn't slow down as it leaves the Sun - it speeds up, and it has a sort of internal heater that keeps it from cooling as it zips through space. With growing concern about the solar wind's ability to interfere with GPS satellites and disrupt power grids on the ground, it's become imperative to better understand it.

Just 17 months since launch, and after three orbits around the Sun, Parker Solar Probe - designed, built and now operated by Johns Hopkins APL for NASA - has not disappointed.

" What we're actually seeing is beyond anything anybody imagined."

"We expected to make big discoveries because we're going into uncharted territory," Raouafi said. "What we're actually seeing is beyond anything anybody imagined."

Researchers suspected that plasma waves within the solar wind could be responsible for some of the wind's odd characteristics. Just as fluctuations in air pressure cause winds that force rolling waves on the ocean, fluctuations in electric and magnetic fields can cause waves that roll through the clouds of electrons, protons and other charged particles that make up the plasma racing away from the Sun. Particles can ride these plasma waves much like the way a surfer rides an ocean wave, propelling them to higher speeds.

"Plasma waves certainly play a part in heating and accelerating the particles," Raouafi said. Scientists just don't know how much of a part.

That's where Parker Solar Probe comes in. The spacecraft's FIELDS instrument can eavesdrop on the electric and magnetic fluctuations caused by plasma waves. And it can "hear" when the waves and particles interact with one another, recording frequency and amplitude information about these plasma waves that scientists could then play as sound waves. And it results in some striking sounds.

Take, for example, whistler-mode waves. These are caused by energetic electrons bursting out of the Sun's corona. These electrons follow magnetic field lines that stretch from the Sun out to the solar system's farthest edge, spinning around them like they're riding a carousel. When a plasma wave's frequency matches how frequently those electrons are spinning, they amplify one another. And it sounds like a scene out of "Star Wars."

" Nobody knows what causes these chirping waves or what they do to heat and accelerate the solar wind."

"Some theories suggest that part of the solar wind's acceleration is due to these escaping electrons," said David Malaspina, a member of the FIELDS team and an assistant professor at the University of Colorado, Boulder, and the Laboratory for Atmospheric and Space Physics. They could also be a critical clue to understanding one process that heats the solar wind.

"We can use observations of these waves to work our way backward and probe the source of these electrons in the corona," Malaspina said.

Another example are dispersive waves. These plasma waves quickly shift from one frequency to another as they move through the solar wind. These shifts create a sort of "chirp" that sounds like wind rushing over a microphone.

"These waves haven't been detected in the solar wind before, at least not in any large numbers," Malaspina explained. They're rare near the Earth, so researchers thought they were unimportant. But closer to the Sun, these waves are everywhere.

"Nobody knows what causes these chirping waves or what they do to heat and accelerate the solar wind. That's what we're going to be determining," Malaspina said. "I think it's incredibly exciting."

Raouafi commented that seeing all of this wave activity very close to the Sun is why this mission is so critical. "We are seeing new, early behaviors of solar plasma we couldn't observe here at Earth, and we're seeing that the energy carried by the waves is being dissipated somewhere along the way, to heat and accelerate the plasma."

Sounds of the Solar Wind

Listen to Dispersive Chirping Waves 1:
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Listen to Dispersive Chirping Waves 2:
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Listen to Langmuir Waves:
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Listen to Whistler Mode Waves 1:
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Listen to Whistler Mode Waves 2:
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But it wasn't just plasma waves that Parker Solar Probe heard. While barreling through a cloud of microscopic dust, the spacecraft's instruments also captured a sound resembling old TV static. That static-like sound is actually hundreds of microscopic impacts happening every day as dust from asteroids torn apart by the Sun's gravity and solar heating and particles stripped from comets as they graze the star strike the spacecraft at speeds close to a quarter of a million miles per hour.

As Parker Solar Probe cruised through this dust cloud, the spacecraft didn't just crash into these particles - it obliterated them. Each grain's atoms burst apart into electrons, protons and other ions in a mini puff of plasma that the FIELDS instrument can "hear."

Each collision, however, also chips away a tiny bit of the spacecraft.

"It was well understood that this would happen," Malaspina explained. "What was not understood was how much dust was going to be there." APL engineers used models and remote observations to estimate how bad the situation might be well before the spacecraft launched. But in this uncharted territory, the number was bound to have some margin of error.

James Kinnison, the Parker Solar Probe mission system engineer at APL, said this discrepancy in dust density is just one more reason why Parker being close to the Sun is so useful. "We protected almost everything from the dust," Kinnison said. And although the dust is denser than expected, nothing right now points to dust impacts being a concern for the mission, he added.

Parker Solar Probe is scheduled to make another 21 orbits around the Sun, using five Venus flybys to draw itself increasingly closer. That will allow researchers to even better understand how these waves change their behavior closer to the Sun and allow scientists to build a more complete evolutionary picture of the solar wind.

Media contact: Justyna.Surowiec@jhuapl.edu, 240-228-8103, Justyna.Surowiec@jhuapl.edu

The Applied Physics Laboratory, a not-for-profit division of The Johns Hopkins University, meets critical national challenges through the innovative application of science and technology. For more information, visit www.jhuapl.edu.

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Parker Solar Probe Team Hears First Whispers of the Solar Wind's Birth

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There's a wind that emanates from the Sun, and it blows not like a soft whistle but like a hurricane's scream. Made of electrons, protons and heavier ions, the solar wind courses through the solar system at roughly 1 million mph (1.6 million kph), barreling over everything in its path.

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Solar wind is the constant outflow of the Sun’s magnetic field and particles. A change in solar wind can shake the magnetic field of the Earth.