太阳活动区域磁图图像数据集用于研究太空天气
Laura E Boucheron1, Ty Vincent2, Jeremy A Grajeda2
1Klipsch School of Electrical and Computer Engineering, New Mexico State University, Las Cruces, NM, 88003, USA. lboucher@nmsu.edu.
Scientific data
|November 24, 2023
概括
这个数据集提供了来自美国宇航局SDO的太阳光圈磁图,对于研究磁场和使用机器学习技术预测太阳耀斑至关重要.
科学领域:
- 太阳物理 太阳物理
- 天体物理学 天体物理学
- 太空物理学 太空物理学
背景情况:
- 太阳耀斑是源于有强磁流动的活跃区域的能量事件.
- 预测太阳耀斑对于太空天气预报和了解太阳动态至关重要.
- 现有的数据集可能缺乏用于机器学习应用的全面,一致格式化的磁力图数据.
研究的目的:
- 提供一套全面的视线太阳光圈磁图的数据集.
- 包括对应的太阳耀斑活动的标签.
- 为了促进太阳物理和自动太阳耀斑预测的研究.
主要方法:
- 使用来自美国宇航局太阳动力学天文台 (SDO) 地震和磁图像仪 (HMI) 的数据.
- 收集和处理太阳能活跃区域的视线磁图.
- 纳入与磁图相关的燃烧活动的标签.
主要成果:
- 一个精心策划的数据集,包含一致大小的太阳能活跃区域图像.
- 包括SDO HMI磁图和燃烧活动标签.
- 为用户配置提供最小处理的数据.
结论:
- 该数据集是太阳耀斑预测研究的宝贵资源.
- 为太阳物理学提供先进的图像分析和机器学习方法.
- 支持对磁性结构和喷发事件之间的关系的调查.
相关概念视频
Magnetostatic Boundary Conditions
964
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...
964
Magnetic Field Lines
4.1K
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:
4.1K
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...
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 Declination
47
Magnetic declination is the angle between true north, which aligns with the Earth's rotational axis, and magnetic north, which follows the direction of the Earth's magnetic field. This discrepancy exists because the magnetic poles do not coincide with the geographic poles. The value of magnetic declination depends on the observer's location on Earth and is subject to changes over time due to the dynamic nature of the Earth's magnetic field.The declination is called eastern when magnetic north...
47
Magnetic Field of a Solenoid
4.0K
A solenoid is a conducting wire coated with an insulating material, wound tightly in the form of a helical coil. The magnetic field due to a solenoid is the vector sum of the magnetic fields due to its individual turns. Therefore, for an ideal solenoid, the magnetic field within the solenoid is directly proportional to the number of turns per unit length and the current. Conversely, the magnetic field outside the solenoid is zero.
Consider a solenoid with 100 turns wrapped around a cylinder of...
Consider a solenoid with 100 turns wrapped around a cylinder of...
4.0K
Magnetic Field Of A Current Loop
4.6K
Consider a circular loop with a radius a, that carries a current I. The magnetic field due to the current at an arbitrary point P along the axis of the loop can be calculated using the Biot-Savart law.
4.6K


