一个5000fps,4兆像素,耐辐射,晶圆尺度CMOS图像传感器,用于直接检测电子和光子
Andrew Scott1, Claus Bauzà1, Adrià Bofill-Petit1
1IMASENIC S.L., C. Torrassa 77, Sant Adrià de Besòs, 08930 Barcelona, Spain.
Sensors (Basel, Switzerland)
|January 28, 2026
概括
这项研究详细介绍了一种4.2兆像素晶圆尺度CMOS图像传感器,其可处理每秒5000多的图像. 该传感器优化为高速电子检测,非常适用于先进的成像应用.
科学领域:
- * 固态物理 固态物理
- * 电气工程 电气工程
- * 光电子学 * 光电子学
背景情况:
- *CMOS图像传感器技术的进步对于高性能成像系统至关重要.
- * 对能够实现极高率和大格式成像的传感器的需求日益增长.
研究的目的:
- * 介绍一个新的晶圆尺度CMOS图像传感器的设计和特征.
- * 通过分辨率,速度和检测能力来评估其性能.
主要方法:
- *设计和制造一个4.2兆像素的CMOS传感器,在200毫米晶圆上有58微米像素.
- * 实现双面读取与柱平行可编程增益放大器 (PGAs) 和模拟数字转换器 (ADCs) 的实现.
- *利用了216个LVDS子车道进行高速数据传输 (1Gbps DDR) 和串行外围接口 (SPI) 进行编程.
主要成果:
- * 在4.2兆像素的完整分辨率下,每秒拍摄超过5000.
- * 传感器阵列包括2052个列和2064个行,有24624个ADC.
- * 已证明对直接电子检测的优化,具有对光子检测的能力.
结论:
- *开发的晶圆尺度CMOS图像传感器满足高速成像要求.
- *其大格式和高率使其适合于像波传感等苛刻的应用.
- * 传感器的双重检测能力 (电子和光子) 提高了它的多功能性.
相关概念视频
Biological Effects of Radiation
17.8K
All radioactive nuclides emit high-energy particles or electromagnetic waves. When this radiation encounters living cells, it can cause heating, break chemical bonds, or ionize molecules. The most serious biological damage results when these radioactive emissions fragment or ionize molecules. For example, α and β particles emitted from nuclear decay reactions possess much higher energies than ordinary chemical bond energies. When these particles strike and penetrate matter, they...
17.8K
pH Scale
79.5K
Hydronium and hydroxide ions are present both in pure water and in all aqueous solutions, and their concentrations are inversely proportional as determined by the ion product of water (Kw). The concentrations of these ions in a solution are often critical determinants of the solution’s properties and the chemical behaviors of its other solutes. Two different solutions can differ in their hydronium or hydroxide ion concentrations by a million, billion, or even trillion times. A common means of...
79.5K
Radiation: Applications
1.8K
The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
The average...
1.8K
Absorption of Radiation
1.3K
The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
1.3K
Electron Configuration of Multielectron Atoms
64.9K
The alkali metal sodium (atomic number 11) has one more electron than the neon atom. This electron must go into the lowest-energy subshell available, the 3s orbital, giving a 1s22s22p63s1 configuration. The electrons occupying the outermost shell orbital(s) (highest value of n) are called valence electrons, and those occupying the inner shell orbitals are called core electrons. Since the core electron shells correspond to noble gas electron configurations, we can abbreviate electron...
64.9K
Electron Carriers
91.7K
Electron carriers can be thought of as electron shuttles. These compounds can easily accept electrons (i.e., be reduced) or lose them (i.e., be oxidized). They play an essential role in energy production because cellular respiration is contingent on the flow of electrons.
Over the many stages of cellular respiration, glucose breaks down into carbon dioxide and water. Electron carriers pick up electrons lost by glucose in these reactions, temporarily storing and releasing them into the electron...
Over the many stages of cellular respiration, glucose breaks down into carbon dioxide and water. Electron carriers pick up electrons lost by glucose in these reactions, temporarily storing and releasing them into the electron...
91.7K


