Jove
Visualize
Contact Us

Related Concept Videos

Magnetostatic Boundary Conditions01:28

Magnetostatic Boundary Conditions

1.0K
An electric field suffers a discontinuity at a surface charge. Similarly, a magnetic field is discontinuous at a surface current. The perpendicular component of a magnetic field is continuous across the interface of two magnetic mediums. In contrast, its parallel component, perpendicular to the current, is discontinuous by the amount equal to the product of the vacuum permeability and the surface current. Like the scalar potential in electrostatics, the vector potential is also continuous...
1.0K
Torque Free Motion01:15

Torque Free Motion

523
The torque-free motion refers to the movement of a rigid body in space when no external torques are acting upon it. This type of motion can be observed in environments where there are no external forces or frictions, like in outer space. For example, a rotation of Mars in space is a torque-free motion. Mars is an axisymmetric object, meaning it has an axis of symmetry along which it rotates, designated as the z-axis. The rotating frame of reference is defined such that the center of mass of...
523
Magnetism01:30

Magnetism

6.4K
Magnets are commonly found in everyday objects, such as toys, hangers, elevators, doorbells, and computer devices. Experimentation on these magnets shows that all magnets have two poles: one is labeled north (N) and the other south (S). Magnetic poles repel if they are alike and attract if unlike. Moreover, both poles of a magnet attract unmagnetized pieces of iron.
An individual magnetic pole cannot be isolated. No matter how small, every piece of a magnet contains a north pole and a south...
6.4K
Magnetic Field Lines01:19

Magnetic Field Lines

4.2K
The representation of magnetic fields by magnetic field lines is very useful in visualizing the strength and direction of the magnetic field. Each of the magnetic field lines forms a closed loop. The field lines emerge from the north pole (N), loop around to the south pole (S), and continue through the bar magnet back to the north pole.
Magnetic field lines follow several hard-and-fast rules:
4.2K
Potential Due to a Magnetized Object01:24

Potential Due to a Magnetized Object

323
Magnetic dipoles in magnetic materials are aligned when placed under an external magnetic field. For paramagnets and ferromagnets, dipole alignment occurs in the direction of the magnetic field. However, the dipoles align opposite to the field in the case of diamagnets. This state of magnetic polarization due to the external field is called magnetization. Magnetization is defined as the dipole moment per unit volume. It plays a similar role to polarization in electrostatics.
The vector...
323
Magnetic Force01:18

Magnetic Force

1.0K
In addition to the electric forces between electric charges, moving electric charges exert magnetic forces on each other. A magnetic field is created by a moving charge or a group of moving charges known as the electric current. A magnetic force is experienced by a second current or moving charge in response to this magnetic field. Fundamentally, interactions between moving electrons in the atoms of two bodies produce magnetic forces between them.
The magnetic force acting on a moving charge...
1.0K

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by
Same author

Anomalous transient enhancement of planetary ion escape at Mars.

Nature communications·2025
Same author

Jets Downstream of Collisionless Shocks: Recent Discoveries and Challenges.

Space science reviews·2024
Same author

Solar Wind Protons in the Diamagnetic Cavity at Comet 67P/Churyumov-Gerasimenko.

Journal of geophysical research. Space physics·2024
Same author

The Comet Interceptor Mission.

Space science reviews·2024
Same author

Observations of a Solar Energetic Particle Event From Inside and Outside the Coma of Comet 67P.

Journal of geophysical research. Space physics·2023
Same author

Mars' plasma system. Scientific potential of coordinated multipoint missions: "The next generation".

Experimental astronomy·2023
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Experiment Video

Updated: Jul 28, 2025

Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas
07:54

Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas

Published on: April 3, 2018

8.2K

Magnetosheath jets at Mars.

Herbert Gunell1, Maria Hamrin1, Sara Nesbit-Östman1

  • 1Department of Physics, Umeå University, 901 87 Umeå, Sweden.

Science Advances
|June 2, 2023
PubMed
Summary
This summary is machine-generated.

Magnetosheath jets, high-pressure plasma phenomena, are found at Mars, not just Earth. These jets influence planetary magnetic fields and space weather, impacting both Mars and Earth.

More Related Videos

A 100 KW Class Applied-field Magnetoplasmadynamic Thruster
11:47

A 100 KW Class Applied-field Magnetoplasmadynamic Thruster

Published on: December 22, 2018

9.1K
Cryogenic Liquid Jets for High Repetition Rate Discovery Science
08:34

Cryogenic Liquid Jets for High Repetition Rate Discovery Science

Published on: May 9, 2020

3.1K

Related Experiment Videos

Last Updated: Jul 28, 2025

Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas
07:54

Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas

Published on: April 3, 2018

8.2K
A 100 KW Class Applied-field Magnetoplasmadynamic Thruster
11:47

A 100 KW Class Applied-field Magnetoplasmadynamic Thruster

Published on: December 22, 2018

9.1K
Cryogenic Liquid Jets for High Repetition Rate Discovery Science
08:34

Cryogenic Liquid Jets for High Repetition Rate Discovery Science

Published on: May 9, 2020

3.1K

Area of Science:

  • Space Physics
  • Planetary Science
  • Plasma Physics

Background:

  • Magnetosheath jets are dynamic plasma entities observed near Earth.
  • These jets possess higher dynamic pressure than ambient plasma.
  • They are known to generate waves and facilitate energy transfer within the magnetosheath and magnetosphere.

Purpose of the Study:

  • To investigate the presence and characteristics of magnetosheath jets beyond Earth's magnetosphere.
  • To determine if similar phenomena occur at Mars.
  • To understand the implications of jets in different planetary environments.

Main Methods:

  • Utilizing data from the Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft.
  • Analyzing plasma and magnetic field measurements in the Martian magnetosheath.
  • Comparing observations with those from Earth's magnetosheath.

Main Results:

  • Magnetosheath jets were identified in the Martian magnetosheath.
  • These Martian jets are associated with increased magnetic field fluctuations.
  • Mars possesses a smaller bow shock compared to Earth, yet still forms these jets.

Conclusions:

  • Magnetosheath jets are not unique to Earth and occur at Mars.
  • Jets play a role in coupling large and small scales in magnetosheaths across the solar system.
  • These findings suggest jets may be common in astrophysical plasmas.