Tag Archive for 'Magnetic field'

Parker Solar Probe has flown through the solar corona and sampled particles and magnetic fields there. Image credit: NASA’s Goddard Space Flight Center.

Parker Solar Probe Identifies Mechanism Driving Fast Solar Wind

Jun 12, 2023 by News Staff

NASA’s Parker Solar Probe has flown close enough to the Sun to detect the fine structure of the solar wind close to where it is generated at the solar...

The highly variable magnetic field around the source of FRB 20190520B. Image credit: Di Li / ScienceApe / CAS.

Astronomers Detect Highly Variable Magnetic Field around Source of Repeating Fast Radio Burst

May 12, 2023 by News Staff

Fast radio bursts (FRBs) are brief flashes of radio waves from distant galaxies that are probably emitted by neutron stars. Some FRBs repeat, which enables...

The most recognizable feature of graphene’s electronic spectrum is its Dirac point, around which interesting phenomena tend to cluster. At low temperatures, the intrinsic behavior in this regime is often obscured by charge inhomogeneity, but thermal excitations can overcome the disorder at elevated temperatures and create an electron-hole plasma of Dirac fermions. The Dirac plasma has been found to exhibit unusual properties, including quantum-critical scattering and hydrodynamic flow. However, little is known about the plasma’s behavior in magnetic fields. Xin et al. report magnetotransport in this quantum-critical regime. Image credit: University of Manchester.

Physicists Discover Giant Magnetoresistance in Graphene

Apr 12, 2023 by News Staff

Record-high magnetoresistance appears in graphene under ambient conditions, according to new research led by the University of Manchester. The most recognizable...

This image of the Crab Nebula combines data from IXPE in magenta and NASA’s Chandra X-ray Observatory in dark purple. Image credit: IXPE / NASA / Chandra / CXC / SAO / K. Arcand / L. Frattare.

IXPE Observes Crab Nebula and Its Pulsar

Apr 11, 2023 by News Staff

Located 6,500 light-years away in the constellation of Taurus, the Crab Nebula and its pulsar formed in a supernova whose light reached Earth in July 1054. This...

An artist’s conceptual rendering of interactions between a prospective exoplanet and its star. Image credit: NSF / Alice Kitterman.

Astronomers Detect Radio Emission Associated with Magnetic Field of Nearby Exoplanet

Apr 4, 2023 by News Staff

Observing magnetic star-planet interactions offers promise for determining the magnetic fields of exoplanets. Models of star-planet interactions predict...

This image shows the Vela pulsar wind nebula: light blue represents X-ray polarization data from IXPE; pink and purple colors correspond to data from NASA’s Chandra X-ray observatory; the NASA/ESA Hubble Space Telescope contributed the stars in the background. Image credit: IXPE / NASA / MSFC / Fei Xie / CXC / SAO / STScI / Hubble / Chandra / Judy Schmidt / Kimberly Arcand / Nancy Wolk.

Polarized X-ray Detection Sheds New Light on Vela Pulsar Wind Nebula

Mar 8, 2023 by News Staff

Astronomers using the Imaging X-ray Polarimetry Explorer (IXPE) — a collaboration between NASA and the Italian Space Agency — have observed...

The climbing capabilities of living creatures such as geckos, tree frogs, and inchworms provide a promising platform for exploiting biomimetic soft climbing robots. Image credit: Sun et al., doi: 10.1016/j.xcrp.2022.101241.

GeiwBot: Gecko- and Inchworm-Inspired Robot Can Climb Walls and Ceilings

Feb 28, 2023 by News Staff

GeiwBot can climb on walls and ceilings of different textures including glass, polyimide, and aluminum; its climbing behavior is based on dynamic attachment...

Drosophila melanogaster and other non-migrating animals can sense external magnetic fields. Image credit: University of Manchester.

Animals’ Ability to Sense Magnetic Field May Be More Widespread than Previously Thought

Feb 23, 2023 by News Staff

New research led by University of Leicester and University of Manchester scientists shows that a molecule present in all living cells called flavin adenine...

The 200-m-wide crater at the Domaine du Météore-vineyard in France. Image credit: Frank Brenker, Goethe University Frankfurt.

Ancient Impact Crater Discovered in France

Feb 22, 2023 by Enrico de Lazaro

The ancient crater, formally known as ‘le Clot,’ is about 220 m in diameter and 30 m in depth, and is located in the ground of the Domaine du Meteore-vineyard...

An artist’s impression of a magnetar eruption. Image credit: NASA’s Goddard Space Flight Center.

Astronomers Detect Spin-Down Glitch in Distant Magnetar

Jan 27, 2023 by News Staff

Magnetars are a special subset of the isolated neutron star family, with X-ray and radio emission mainly powered by the decay of their immense magnetic...

Schematic and applications of the liquid-solid phase transition of MPTM. Image credit: Wang et al., doi: 10.1016/j.matt.2022.12.003.

Shape-Shifting Robot Can Turn into Liquid and Escape Cage

Jan 26, 2023 by News Staff

Researchers from the Shenzhen Campus of Sun Yat-sen University, Carnegie Mellon University, the Chinese University of Hong Kong and Zhejiang University...

This artist’s conception shows a zoomed in view of MWC 349A and its surrounding disk of gas and dust that are being shaped by the winds and high-speed jet. Image credit: ALMA / ESO / NAOJ / NRAO / M. Weiss, NRAO, AUI & NSF.

ALMA Spots Hidden Jet from Oddball Star MWC 349A

Jan 9, 2023 by News Staff

The jet observed by the Atacama Large Millimeter/submillimeter Array (ALMA) is ejecting material away from MWC 349A at a blistering 500 km per second (311...

This composite image shows one of the studied clusters, NGC 3293, which is 11 million years old and is located about 8,300 light-years from Earth in the constellation of Carina. The image contains X-rays from Chandra (purple) as well as infrared data from ESA’s Herschel Space Observatory (red), longer-wavelength infrared data from NASA’s retired Spitzer Space Telescope (blue and white), and optical data from the MPG/ESO 2.2-m telescope at ESO’s La Silla Observatory appearing as red, white and blue. Image credit: NASA / CXC / Penn State University / Getman et al. / ESA / JPL-Caltech / Herschel Space Observatory / IPAC / SSC / Spitzer Space Telescope / MPG / ESO / G. Beccar.

Astronomers Trace Evolution of X-Ray Activity in Young Sun-Like Stars

Dec 27, 2022 by News Staff

Astronomers using NASA’s Chandra X-ray Observatory and ESA’s Gaia satellite have studied a sample of 6,003 stars in 10 different open clusters with...

An artist’s impression of a magnetar. Image credit: NASA’s Goddard Space Flight Center / S. Wiessinger.

Distant Magnetar Has Solid Surface with No Atmosphere

Nov 4, 2022 by News Staff

Magnetars are neutron stars with ultra-strong magnetic fields, which can be observed in X-rays. Polarization measurements could provide information on...

This composite image shows the supernova remnant Cassiopeia A, a structure resulting from the explosion of a star in the constellation of Cassiopeia. The blues represent data from NASA’s Chandra X-ray Observatory, the turquoise is from IXPE, and the gold is courtesy of the NASA/ESA Hubble Space Telescope. Image credit: NASA / CXC / SAO / NASA / MSFC / Vink et al. / STScI.

IXPE Maps Polarized X-Rays from Cassiopeia A

Oct 18, 2022 by News Staff

Cassiopeia A is a remnant that blew up as a supernova approximately 11,000 years ago. This composite image shows the supernova remnant Cassiopeia A, a...

This artist’s illustration indicates where the modeling of the ALMA data predicts the hot spot to be and its orbit around Sagittarius A*. Image credit: ESO / M. Kornmesser / M. Wielgus / Event Horizon Collaboration.

ALMA Spots Bubble of Hot Gas in Orbit around Milky Way’s Central Black Hole

Sep 22, 2022 by News Staff

Sagittarius A*, the 4.3-million-solar-mass black hole at the center of our Milky Way Galaxy, was observed with the Atacama Large Millimeter/submillimeter...

This image, obtained with the Metis instrument onboard ESA’s Solar Orbiter on March 25, 2022, shows the solar corona. Image credit: Telloni et al., doi: 10.3847/2041-8213/ac8104.

ESA’s Solar Orbiter Observes Magnetic Switchback in Sun’s Corona

Sep 12, 2022 by Natali Anderson

Solar switchbacks are sudden, large radial deflections of the solar wind magnetic field, previously revealed in interplanetary space by NASA spacecraft. This...

Top left: a giant blue star, much more massive than our Sun, has consumed, through nuclear fusion at its center, all its hydrogen, helium, and heavier elements up to iron. It now has a small iron core (red dot) at its center. Unlike the earlier stages of fusion, the fusion of iron atoms absorbs, rather than releases, energy. The fusion-released energy that has held up the star against its own weight now is gone, and the star will quickly collapse, triggering a supernova explosion. Top right: the collapse has begun, producing a superdense neutron star with a strong magnetic field at its center (inset). The neutron star, though containing about 1.5 times the mass of the Sun, is only about the size of Manhattan. Bottom left: the supernova explosion has ejected a fast-moving shell of debris outward into interstellar space. At this stage, the debris shell is dense enough to shroud from view any radio waves coming from the region of the neutron star. Bottom right: As the shell of explosion debris expands over a few decades, it becomes less dense and eventually becomes thin enough that radio waves from inside can escape. This allowed observations by the VLA Sky Survey to detect bright radio emission created as the rapidly spinning neutron star’s powerful magnetic field sweeps through the surrounding space, accelerating charged particles. This phenomenon is called a pulsar wind nebula. Image credit: Melissa Weiss, NRAO / AUI / NSF.

Astronomers Spot Pulsar Wind Nebula in Distant Dwarf Galaxy

Jun 15, 2022 by News Staff

A pulsar wind nebula is created when the powerful magnetic field of a rapidly spinning neutron star accelerates surrounding charged particles to nearly...

MeerKAT image of the PSR J0901-4046 region at 1.28 GHz. Image credit: Caleb et al., doi: 10.1038/s41550-022-01688-x.

Astronomers Discover Unusual Radio-Emitting Neutron Star

May 31, 2022 by News Staff

Radio-emitting neutron stars are objects with spin periods ranging from milliseconds to tens of seconds; as they age and spin more slowly, their radio...

https://cdn.sci.news/images/2022/04/image_10734-Micronova.jpg

New Type of Nova Discovered: Micronova

Apr 21, 2022 by News Staff

A micronova is a thermonuclear blast that happens on the surface of certain stars and lasts for just a few hours making them extremely difficult to observe. This...

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