相关实验视频
Updated: Jun 26, 2025

09:27
Wind Tunnel Experiments to Study Chaparral Crown Fires
Published on: November 14, 2017
9.7K
我看到了'烟雾'的标志,然后它消失在空气中
Lyle Suh1, Ajit S Puri2, Jasmeet Singh2
1University of Massachusetts Chan Medical School, Worcester, MA, USA.
Clinical imaging
|May 17, 2024
概括
莫亚莫亚是一种罕见的脑血管疾病,导致大脑中的动脉狭窄. 它通过脑血管学上的独特的"烟雾"外观来识别,这表明了渐进式狭窄.
科学领域:
- 神经学 神经学
- 血管医学 血管医学
- 放射学 放射学是一门学科.
背景情况:
- 莫亚莫亚病是一种渐进的,非动脉样硬化,非炎症性血管病变.
- 它会影响内内动脉和威利斯圆.
- 莫亚莫亚可以是特异性 (疾病) 或继发于其他疾病 (综合征).
研究的目的:
- 为了描述Moyamoya的关键特征.
- 为了突出诊断成像的发现.
- 为了区分Moyamoya病与Moyamoya综合征.
主要方法:
- 对Moyamoya.com的现有文献进行了审查.
- 对Moyamoya的诊断标准的分析.
- 专注于脑血管造影的发现.
主要成果:
- 莫亚莫亚涉及主要大脑动脉的渐进性狭窄.
- 在脑血管造影中观察到一种特有的"烟雾"标志.
- 这种情况可以是主要的或与其他综合征相关.
结论:
- 莫亚莫亚是一种独特的血管病变,具有特定的血管学特征.
- 脑血管造影对于诊断莫亚莫亚的诊断至关重要.
- 了解潜在的原因 (疾病与综合症) 对于患者的管理很重要.
相关概念视频
Vaporization
34.6K
The physical form of a substance changes by changing its temperature. For example, raising the temperature of a liquid causes the liquid to vaporize (convert into vapor). The process is called vaporization—a surface phenomenon. For vaporization to occur, kinetic energy must be greater than the intermolecular forces that keep molecules bonded. The amount of energy needed to vaporize a quantity of liquid at a given pressure and a constant temperature is called the heat of vaporization. When...
34.6K
Significance of Displacement Current
4.5K
A displacement current is analogous to a real current in Ampère's law, participating in Ampère's law the same way as the usual conduction current. However, it is produced by a changing electric field. Displacement current is defined in terms of a time-varying electric field, and also has an associated displacement current density. By adding a term accounting for displacement current, Maxwell modified the existing Ampère's law, which is now called generalized Ampère's law.
4.5K
Pulmonary Cycle: Exhalation
1.6K
In terms of human respiration, the act of expelling air, known as exhalation (or expiration), operates on the principle of pressure gradients. During expiration, the pressure within the lungs exceeds that of the surrounding atmosphere. Under normal conditions, quiet breathing involves passive exhalation and is free of muscular contractions. This is because the exhalation process is driven by the natural elastic recoil of the lungs and chest wall, both of which have an inherent tendency to...
1.6K
Flame Photometry: Overview
564
Flame photometry, also known as flame emission spectrometry, is a technique used for the qualitative and quantitative analysis of elements present in a sample using a flame as the source of excitation energy. The concept of flame photometry was realized in the early 1860s by Kirchhoff and Bunsen, who discovered that specific elements emit characteristic radiation when excited in flames. The first instrument developed for this purpose was used to measure sodium (Na) in plant ash using a Bunsen...
564
Tip-of-the-Tongue Phenomenon
141
The tip-of-the-tongue (TOT) phenomenon is a cognitive experience characterized by a temporary inability to retrieve specific information from memory despite having a strong feeling of knowing the information. Although individuals cannot access the target word or detail, they frequently recall related elements, such as its initial letter, syllable count, or context. This partial retrieval often causes frustration, as one might recognize a familiar face or know that a name starts with a specific...
141
Detection of Black Holes
2.2K
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...
2.2K

