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MUSES02
IC AUDIO 2 CIRCUIT 8DIP
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- 資料表 MUSES02 DataSheet
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規格
| Part Status | Not For New Designs |
| Amplifier Type | Audio |
| Number of Circuits | 2 |
| Slew Rate | 5V/µs |
| Gain Bandwidth Product | 11 MHz |
| Current - Input Bias | 100 nA |
| Voltage - Input Offset | 300 µV |
| Current - Supply | 8mA |
| Current - Output / Channel | 50 mA |
| Voltage - Supply Span (Min) | 7 V |
| Voltage - Supply Span (Max) | 32 V |
| Operating Temperature | -40°C ~ 85°C |
| Mounting Type | Through Hole |
| Package / Case | 8-DIP (0.300", 7.62mm) |
| Supplier Device Package | 8-DIP |
概述
Description
MUSES02 (Multi-Unit Spectroscopic Explorer for the Solar System) is a space mission concept designed to study celestial bodies in our solar system using advanced spectroscopic techniques. The primary aim is to analyze the composition and physical properties of objects like asteroids, comets, and moons, providing insights into their formation and evolution.
MUSES02 employs a multi-channel spectrometer capable of capturing data across various wavelengths, enhancing our understanding of surface materials and atmospheric compositions. By targeting specific celestial events and objects, the mission seeks to unravel the history of our solar system and its constituent bodies.
The mission also emphasizes technology development, aiming to improve spectroscopic instruments for future exploration. MUSES02 is part of a broader initiative to foster international collaboration in planetary science, and its findings could have implications for understanding planetary processes, resource exploration, and the potential for life beyond Earth.
MUSES02 employs a multi-channel spectrometer capable of capturing data across various wavelengths, enhancing our understanding of surface materials and atmospheric compositions. By targeting specific celestial events and objects, the mission seeks to unravel the history of our solar system and its constituent bodies.
The mission also emphasizes technology development, aiming to improve spectroscopic instruments for future exploration. MUSES02 is part of a broader initiative to foster international collaboration in planetary science, and its findings could have implications for understanding planetary processes, resource exploration, and the potential for life beyond Earth.
Features
MUSES02 is a high-resolution space-based spectroscopic mission designed to enhance our understanding of the universe. Key features include:
1. Spectroscopic Capability: MUSES02 employs advanced spectrometers to analyze light from celestial objects across various wavelengths, enabling detailed composition studies.
2. High Resolution: The mission offers high spectral resolution, allowing for precise measurements of chemical elements and compounds in astronomical sources.
3. Wide Field of View: It is capable of observing a broad range of astronomical phenomena simultaneously, which is crucial for comprehensive surveys.
4. Multi-Wavelength Observations: MUSES02 operates across different wavelengths (e.g., ultraviolet, optical, infrared), facilitating diverse astrophysical investigations.
5. Data Collection: It gathers extensive data on exoplanets, star formation, and galaxy evolution, contributing to our knowledge of cosmic processes.
6. Collaboration: MUSES02 collaborates with ground-based telescopes and other space missions for enhanced observational synergy.
These features position MUSES02 as a vital tool for advancing astrophysical research and understanding the universe's complexities.
1. Spectroscopic Capability: MUSES02 employs advanced spectrometers to analyze light from celestial objects across various wavelengths, enabling detailed composition studies.
2. High Resolution: The mission offers high spectral resolution, allowing for precise measurements of chemical elements and compounds in astronomical sources.
3. Wide Field of View: It is capable of observing a broad range of astronomical phenomena simultaneously, which is crucial for comprehensive surveys.
4. Multi-Wavelength Observations: MUSES02 operates across different wavelengths (e.g., ultraviolet, optical, infrared), facilitating diverse astrophysical investigations.
5. Data Collection: It gathers extensive data on exoplanets, star formation, and galaxy evolution, contributing to our knowledge of cosmic processes.
6. Collaboration: MUSES02 collaborates with ground-based telescopes and other space missions for enhanced observational synergy.
These features position MUSES02 as a vital tool for advancing astrophysical research and understanding the universe's complexities.
Package
MUSES02 is available in a small, compact package type known as the WLCSP (Wafer Level Chip Scale Package). This packaging allows for a reduced footprint, making it suitable for space-constrained applications while maintaining performance and functionality.
Pinout
The MUSES02 is a high-performance operational amplifier with a pin count of 8. It is designed for audio applications, offering low distortion and high fidelity.
The pin functions are as follows:
1. Pin 1 (Offset Null): Used for offset adjustment.
2. Pin 2 (Inverting Input): The negative input for the operational amplifier.
3. Pin 3 (Non-inverting Input): The positive input for the operational amplifier.
4. Pin 4 (V- or GND): Negative power supply or ground connection.
5. Pin 5 (Offset Null): Another pin for offset adjustment, often tied to pin 1.
6. Pin 6 (Output): The output of the operational amplifier.
7. Pin 7 (V+ or Vcc): Positive power supply connection.
8. Pin 8 (NC): No connection (not used).
The MUSES02 is favored in high-fidelity audio equipment due to its low noise and high slew rate.
The pin functions are as follows:
1. Pin 1 (Offset Null): Used for offset adjustment.
2. Pin 2 (Inverting Input): The negative input for the operational amplifier.
3. Pin 3 (Non-inverting Input): The positive input for the operational amplifier.
4. Pin 4 (V- or GND): Negative power supply or ground connection.
5. Pin 5 (Offset Null): Another pin for offset adjustment, often tied to pin 1.
6. Pin 6 (Output): The output of the operational amplifier.
7. Pin 7 (V+ or Vcc): Positive power supply connection.
8. Pin 8 (NC): No connection (not used).
The MUSES02 is favored in high-fidelity audio equipment due to its low noise and high slew rate.
Manufacturer
The MUSES02 is manufactured by MUSES, a brand under Nippon Chemi-Con Corporation. Nippon Chemi-Con is a Japanese company known for producing high-quality capacitors and audio components, primarily focusing on the audio and electronics markets. The MUSES brand specifically specializes in high-performance audio operational amplifiers designed for audiophiles and professional audio applications. Their products are recognized for their sound quality and precision, catering to the needs of high-end audio equipment manufacturers and enthusiasts.
Application
MUSES02 is primarily applied in the fields of modeling and understanding complex systems. Key application areas include environmental monitoring, climate modeling, urban planning, disaster management, and resource allocation. It is also utilized in decision support systems, healthcare analytics, and optimizing supply chain logistics, leveraging its capabilities to simulate scenarios and analyze data effectively.
Equivalent
Equivalent products to the MUSES02 chip include the MUSES03, MUSES01, and various op-amps from different manufacturers such as the OPA2134 from Texas Instruments, AD823 from Analog Devices, and the LM4562 from Texas Instruments. These alternatives typically offer similar performance characteristics in audio applications.
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