Jove
Visualize
お問い合わせ

関連する概念動画

Atomic Nuclei: Nuclear Magnetic Moment00:59

Atomic Nuclei: Nuclear Magnetic Moment

1.2K
All atomic nuclei are positively charged. When they have a nonzero spin, they behave like rotating charges. As a consequence of their charge and spin, these nuclei generate a magnetic field (B). This, in turn, gives rise to a magnetic moment (μ), which is randomly oriented in the absence of an external magnetic field. When an external magnetic field (B0) is applied, the magnetic moment vectors can align with the field or against it in 2 + 1 orientations. A hydrogen nucleus, which is just a...
1.2K
Potential Due to a Magnetized Object01:24

Potential Due to a Magnetized Object

324
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...
324
Atomic Nuclei: Nuclear Relaxation Processes01:23

Atomic Nuclei: Nuclear Relaxation Processes

690
In the absence of an external magnetic field, nuclear spin states are degenerate and randomly oriented. When a magnetic field is applied, the spins begin to precess and orient themselves along (lower energy) or against (higher energy) the direction of the field. At equilibrium, a slight excess population of spins exists in the lower energy state. Because the direction of the magnetic field is fixed as the z-axis,  the precessing magnetic moments are randomly oriented around the z-axis.
690
Atomic Nuclei: Nuclear Spin State Population Distribution01:14

Atomic Nuclei: Nuclear Spin State Population Distribution

1.0K
Near absolute zero temperatures, in the presence of a magnetic field, the majority of nuclei prefer the lower energy spin-up state to the higher energy spin-down state. As temperatures increase, the energy from thermal collisions distributes the spins more equally between the two states. The Boltzmann distribution equation gives the ratio of the number of spins predicted in the spin −½ (N−) and spin +½ (N+) states.
1.0K
Magnetic Field due to Moving Charges01:23

Magnetic Field due to Moving Charges

8.9K
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...
8.9K
Atomic Nuclei: Magnetic Resonance01:05

Atomic Nuclei: Magnetic Resonance

706
The number of nuclear spins aligned in the lower energy state is slightly greater than those in the higher energy state. In the presence of an external magnetic field, as the spins precess at the Larmor frequency, the excess population results in a net magnetization oriented along the z axis. When a pulse or a short burst of radio waves at the Larmor frequency is applied along the x axis, the coupling of frequencies causes resonance and flips the nuclear spins of the excess population from the...
706

こちらも読む

関連記事

共著者、ジャーナル、引用グラフによってこの研究に関連する記事。

並び替え
Same author

Retraction Note: Sub-second periodicity in a fast radio burst.

Nature·2026
Same author

A sudden change and recovery in the magnetic environment around a repeating fast radio burst.

Science (New York, N.Y.)·2026
Same author

A pulsar-like polarization angle swing from a nearby fast radio burst.

Nature·2025
Same author

Magnetospheric origin of a fast radio burst constrained using scintillation.

Nature·2025
Same author

A nebular origin for the persistent radio emission of fast radio bursts.

Nature·2024
Same author

A pulsar in a binary with a compact object in the mass gap between neutron stars and black holes.

Science (New York, N.Y.)·2024
Same journal

Family of magnetic field-boosted superconductors in rhombohedral graphene.

Nature·2026
Same journal

What's the human cost of US research turmoil? A new film finds out.

Nature·2026
Same journal

Daily briefing: Ovaries start a second job after menopause.

Nature·2026
Same journal

Audio long read: Is the peptide craze backed by science? The promise behind the hype.

Nature·2026
Same journal

Scientists fight back against far-right plans to restrict academic freedom in Germany.

Nature·2026
Same journal

How AI can crack open the 'hidden curriculum' for neurodivergent students.

Nature·2026
関連記事をすべて見る
JoVE
x logofacebook logolinkedin logoyoutube logo
JoVEについて
概要リーダーシップブログJoVEヘルプセンター
著者向け
出版プロセス編集委員会範囲と方針査読よくある質問投稿
図書館員向け
推薦の声購読アクセスリソース図書館諮問委員会よくある質問
研究
JoVE JournalMethods CollectionsJoVE Encyclopedia of Experimentsアーカイブ
教育
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab Manual教員リソースセンター教員サイト
利用規約
プライバシーポリシー
ポリシー

関連する実験動画

Updated: Jul 30, 2025

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

パルサー・バイナリ系の高度に磁気化された環境

Dongzi Li1, Anna Bilous2, Scott Ransom3

  • 1Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, CA, USA. dongzili@caltech.edu.

Nature
|May 17, 2023
PubMed
まとめ
この要約は機械生成です。

PSR B1744-24Aのようなクモパルサーは 磁気力が強い環境を示しています 証拠によると,これらの磁場はパルサーの放射に影響し,いくつかの高速ラジオバースト (FRB) に見られる条件に似ています.

さらに関連する動画

High-Temperature and High-Pressure In situ Magic Angle Spinning Nuclear Magnetic Resonance Spectroscopy
08:55

High-Temperature and High-Pressure In situ Magic Angle Spinning Nuclear Magnetic Resonance Spectroscopy

Published on: October 9, 2020

5.6K
Hyperpolarized Xenon for NMR and MRI Applications
16:20

Hyperpolarized Xenon for NMR and MRI Applications

Published on: September 6, 2012

19.6K

関連する実験動画

Last Updated: Jul 30, 2025

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
High-Temperature and High-Pressure In situ Magic Angle Spinning Nuclear Magnetic Resonance Spectroscopy
08:55

High-Temperature and High-Pressure In situ Magic Angle Spinning Nuclear Magnetic Resonance Spectroscopy

Published on: October 9, 2020

5.6K
Hyperpolarized Xenon for NMR and MRI Applications
16:20

Hyperpolarized Xenon for NMR and MRI Applications

Published on: September 6, 2012

19.6K

科学分野:

  • 天文学と天体物理学
  • パルサー物理学
  • バイナリー星系

背景:

  • スパイダーパルサーは,低質量伴星と密接な軌道にあるミリ秒パルサーです.
  • これらのシステムは プラズマの消去,時間遅延,パルサーの放射の蝕みなどの現象を呈しています
  • 伴星の磁場は,バイナリーシステムの進化と日食の性質に影響を及ぼすと仮定されています.

研究 の 目的:

  • スパイダーパルサーシステムPSR B1744-24Aの磁気環境を調査する
  • 磁場特性を理解するために 偏振と回転の変動を分析する.
  • スパイダーパルサーの行動と高速ラジオバースト (FRBs) の間の潜在的な接続を探求する.

主な方法:

  • PSR B1744-24Aにおける円形の偏化 (V) 変化の観測
  • 軌道の様々な段階における不規則で速い回転量 (RM) の分析.
  • 観測された偏振振動と既知のFRB特性との比較

主要な成果:

  • 半正規の円形の偏極化プロファイルの変化はファラデー変換を示し,コンパニオン磁場を> 10 Gに制限します.
  • 恒星風の磁場強度が10mG以上であることを示唆している.
  • 観測された偏極化行動は,繰り返し発生するFast Radio Bursts (FRB) と類似している.

結論:

  • PSR B1744-24Aは,伴星とその恒星の風の両方から重要な磁場を持つ高度に磁性化された環境を有しています.
  • ファラデーの変換とRMの変動を含む観測された現象は,これらの磁場に対する強力な証拠を提供します.
  • FRBとの類似性からすると,FRBの一部はスパイダーパルサーのようなバイナリ系から発生していると考えられる.