Since it launched last year, NASA’s Parker Solar Probe has made three dives toward the sun as it reached the fastest speed ever clocked by a human-built vehicle. Scientists released the mission’s first batch of findings on Wednesday, revealing that the dynamics of our star are even weirder than once imagined.

Four papers published in the journal Nature describe what the spacecraft observed during its first two flybys, as it passed within about 15 million miles of the surface of the sun. That is about half the distance that the planet Mercury orbits the sun.

“All of this brand-new information about how the way our star works is going to help us understand how the sun drives change in the space environment throughout our solar system,” said Nicola Fox, director of the heliophysics division at NASA, during a telephone news conference on Wednesday.

The information could help scientists develop ways to provide advance warning of solar storms that could knock out satellites and electrical grids or endanger the health of astronauts in orbit.

Blazing Hot Bubble

The sun is essentially a big ball of hydrogen and helium, and for something that we see every day, it remains a complex ball of mystery.

One puzzle that scientists have been pondering for decades: Why is the solar atmosphere superhot?

The surface of the sun — what we see as a yellow disk in the sky — is about 10,000 degrees Fahrenheit. That is toasty, but cool compared with what lies above, in the thin atmosphere known as the corona.

There, the temperatures jump by a factor of 300 or more, to millions of degrees. The corona also accelerates the solar wind — the million-miles-per-hour stream of particles that fly outward from the sun.

Justin C. Kasper, a professor of space sciences and engineering at the University of Michigan and the principal investigator of one of the solar probe’s four instruments, said scientists said they had a hunch that the vibrating of the sun’s magnetic fields — like the plucking of a guitar string — was critical to heating the corona. So they were curious about what the vibrations would look like closer to the sun.

As expected, the vibrations did get stronger. But the instrument also picked up additional, powerful waves. “Kind of like rogue waves in the ocean,” Dr. Kasper said.

As one of the big waves swept the spacecraft, the speed of the solar wind would, within seconds, rise by 300,000 miles per hour. Each wave would last seconds to minutes. “Just as quickly, in seconds, it goes past us, and we’re back in the normal solar wind,” Dr. Kasper said.

The waves were so strong that they could flip the direction of the magnetic field, producing S-shape twists that the scientists called “switchbacks,” like the twisty paths carved in the side of a steep mountain.

“These are very large and energetic events,” Dr. Kasper said. “We’re really excited about this, because we think it tells us a possible path to understanding how energy is getting from the sun into the atmosphere and heating it.”

Where the Wind Blows

With the closer view of the sun, scientists also now have a better idea of where the solar wind originates.

Most of the solar wind measurements to date have been in the neighborhood of Earth, more than 90 million miles from the sun.

Stuart Bale, a physicist at the University of California, Berkeley, who leads an instrument that measures the electric and magnetic fields in the solar wind, said trying to study solar winds from Earth is like observing the waterfall halfway down.

“The water is always flowing past us,” he said. “It is very turbulent, chaotic, unstructured. And we want to know what is the source of the waterfall, what’s at the top. Is there an iceberg melting up there? Is there a sprinkler system? A lake?”

By the time the solar wind reaches Earth, clues about its origin have been jumbled and become difficult to discern.

“We want to know the source of the water, what’s at the top,” Dr. Bale said.

He said that data from the Parker Solar Probe now shows that the so-called slow solar wind, moving at relatively slow speeds of less than a million miles per hour, emerges from what are known as coronal holes — locations associated with sunspots and where hydrogen and helium are colder and less dense — near the sun’s Equator. (Faster solar winds traveling more than a million miles per hour were known to originate from coronal holes near the poles.)

Star Dust

The spacecraft has also been putting together a picture of the cloud of dust surrounding the sun and the corona — bits shed from comets and asteroids that have passed. The dust was thinner closer to the sun, matching the expectations for a long-theorized dust-free zone around the star.

As the Parker Solar Probe gets closer — repeated flybys of Venus in the coming years will eventually nudge it to a trajectory that will take it within four million miles of the sun — it is likely to confirm that observation and reveal new mysteries.

“It’s a bit early to say whether these discoveries actually overturn existing models,” Daniel Verscharen, a space scientist at University College London who wrote a commentary accompanying the Nature papers, said in an email. “They definitely show that there is a lot more happening close to the sun and that it’s absolutely worth going there to explore further.”

A European Space Agency mission, Solar Orbiter, is set to launch in February. While it will not get as close to the sun as the Parker Solar Probe, it will carry instruments that will provide different views and provide more clues on solving the mystery of the solar wind.

Eugene N. Parker, a retired University of Chicago astrophysicist whom the spacecraft is named after, predicted the existence of the solar wind in 1958. “It was humbling to see the probe’s launch and watch it disappear into the night sky,” Dr. Parker, now 92, said in a statement provided by the university. “But now that data is finally coming in and being analyzed, things are getting really exciting.”