相关实验视频
Updated: Apr 14, 2026

11:47
A 100 KW Class Applied-field Magnetoplasmadynamic Thruster
Published on: December 22, 2018
9.8K
活跃的星系. 活动的星系. 一个超大质量黑洞喷射基中的强磁场
Ivan Martí-Vidal1, Sébastien Muller2, Wouter Vlemmings2
1Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, SE-43992, Onsala, Sweden. mivan@chalmers.se.
概括
研究人员使用阿塔卡马大毫米/亚毫米阵列 (ALMA) 检测到活跃银河系核 (AGN) 喷射基底的强磁场. 这一发现为这些强大的宇宙喷气如何形成和引导提供了新的见解.
科学领域:
- 天体物理学 天体物理学
- 宇宙磁场是宇宙的磁场.
- 活跃的银河系核心 (AGN)
背景情况:
- 活跃的银河系核 (AGN) 是由物质积聚到超大质量黑洞的力量驱动的.
- 来自AGN的外流喷气是能量现象,但它们的形成和引导机制是不确定的.
- 假设磁场在AGN喷气形成和聚合中起着关键作用.
研究的目的:
- 研究磁场在AGN喷气的形成和结合中的作用.
- 为了检测和描述AGN喷气机底部的磁场.
主要方法:
- 使用阿塔卡马大毫米/亚毫米阵列 (ALMA) 观测遥远的AGN PKS 1830-211.
- 检测到一个极化信号,特别是法拉第旋转,表明磁场存在.
- 测量了旋转量,它与沿视线的磁场强度和电子密度的积分成比例.
主要成果:
- 在AGN PKS 1830-211的喷气基地检测到一个显著的极化信号 (法拉第旋转).
- 推导出高旋转度的测量,表明存在强磁场.
- 在距离黑洞大约光日 (0.01 帕塞克) 的尺度上,推断的磁场强度至少为几十个高斯.
结论:
- 在AGN喷气的底部存在强大的磁场.
- 这些磁场可能在形成和引导从活跃的银河系核中观察到的强大的喷气中发挥着至关重要的作用.
- 这些发现提供了直接的证据,支持AGN喷气的磁性起源.
相关概念视频
Detection of Black Holes
2.6K
Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
2.6K
Schwarzschild Radius and Event Horizon
3.0K
No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...
3.0K
Magnetic Field Lines
6.6K
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:
Magnetic field lines follow several hard-and-fast rules:
6.6K
Magnetic Fields
8.0K
A moving charge or a current creates a magnetic field in the surrounding space, in addition to its electric field. The magnetic field exerts a force on any other moving charge or current that is present in the field. Like an electric field, the magnetic field is also a vector field. At any position, the direction of the magnetic field is defined as the direction in which the north pole of a compass needle points.
A magnetic field is defined by the force that a charged particle experiences...
A magnetic field is defined by the force that a charged particle experiences...
8.0K
Magnetic Field due to Moving Charges
12.6K
A stationary charge creates and interacts with the electric field, while a moving charge creates a magnetic field.
Consider a point charge moving with a constant velocity. Like the electric field, the magnetic field at any point is directly proportional to the magnitude of the charge and inversely proportional to the square of the distance between the source point and the field point. However, unlike the electric field, the magnetic field is always perpendicular to the plane containing the line...
Consider a point charge moving with a constant velocity. Like the electric field, the magnetic field at any point is directly proportional to the magnitude of the charge and inversely proportional to the square of the distance between the source point and the field point. However, unlike the electric field, the magnetic field is always perpendicular to the plane containing the line...
12.6K
Energy In A Magnetic Field
3.0K
If a magnetic field is sustained, there must be a current in a closed circuit or loop, implying some energy has been spent in creating the field. If this energy is not dissipated via the circuit's resistance, it is stored in the field.
Take an ideal inductor with zero resistance. Although it's practically impossible, assume that the coil's resistance is so small that it is practically negligible. The loss of the field's energy to dissipate thermal energy (or heat) is thus...
Take an ideal inductor with zero resistance. Although it's practically impossible, assume that the coil's resistance is so small that it is practically negligible. The loss of the field's energy to dissipate thermal energy (or heat) is thus...
3.0K

