1- Detection of radio waves from the Universe- Tools & Techniques

Auriel3003
Auriel3003
|
Published on 30 Jul 2022
#ARTICLE#Multi-Spectral-Astronomy

Lecture Notes on Radio Astronomy and GMRT by Yashwant Gupta

1. Introduction to Radio Astronomy

- Definition and Importance:

- Radio astronomy involves studying celestial objects through the radio frequencies of the electromagnetic spectrum.

- It provides a unique window into the universe, allowing observations of phenomena that are not visible in optical wavelengths.

- Role of GMRT:

- The Giant Meterwave Radio Telescope (GMRT) is one of the most significant facilities in radio astronomy, designed to enhance our understanding of various astronomical phenomena.

2. Overview of the Receiver System

- Key Components:

- Feed Elements: Located at the antenna focus, these elements capture incoming radio waves.

- Front-end Electronics: Responsible for amplifying the weak signals received from the feed elements.

- Optical Fiber Transmission: Converts analog signals to optical signals for transmission to the central station, reducing losses.

- Analog and Digital Processing Chains: Essential for analyzing the signals received, with appropriate controls for frequency settings.

- Bandwidth Significance:

- The original GMRT system had a bandwidth of 32 MHz. A larger bandwidth allows for the collection of more signal data, increasing sensitivity and improving observations of sources that emit over a broader frequency range.

3. Capabilities of the GMRT

- Historical Context:

- Constructed in the 1990s, GMRT began regular observations in 2002 and serves as an international facility for astronomers worldwide.

- Observational Demand:

- The facility is highly oversubscribed, with demand for observing time often two to three times higher than available scheduling.

- Research Areas:

- Studies range from solar radio emissions to searching for extra-solar planets, pulsars, supernova remnants, and cosmic magnetism.

4. Scientific Applications of GMRT

- Diverse Research Topics:

- Radio emission from the Sun

- Cosmic magnetism

- Galactic structures and dynamics

- All-sky surveys, such as the TGSS at 150 MHz, providing critical data on the distribution and characteristics of celestial sources.

- Significant Findings:

- GMRT has contributed to numerous research publications and groundbreaking discoveries in radio astronomy.

5. Recent Upgrades to GMRT

- Major Enhancements:

- The upgraded GMRT features seamless frequency coverage from 120 to 1450 MHz, with plans to extend down to 50 MHz.

- Instantaneous bandwidth has increased to 400 MHz, significantly improving sensitivity and versatility.

- Noise Rejection:

- Improved receiver quality allows for better rejection of man-made radio noise, enhancing the overall quality of observations.

- Performance Improvement:

- The upgraded system demonstrates a sensitivity improvement by a factor of three compared to the legacy GMRT, allowing for better-quality imaging and data analysis.

6. Introduction to the Square Kilometer Array (SKA)

- Project Overview:

- The SKA is the most ambitious radio astronomy project, aiming for a sensitivity improvement of over 10 times compared to existing facilities.

- It will feature a total collecting area of one square kilometer and will utilize many smaller antennas spread across continents.

- Technological Innovations:

- The project requires cutting-edge technology in areas like antenna design, electronics, and data processing.

- Signal transport will involve optical fibers, with network traffic exceeding current global internet traffic.

- Global Collaboration:

- The SKA involves participation from multiple countries, showcasing international cooperation in advancing radio astronomy.

7. Future Prospects in Radio Astronomy

- Research Opportunities:

- The SKA is expected to enable groundbreaking research on topics such as the early universe, dark energy, and the evolution of galaxies.

- New techniques will facilitate studies of transient sources and the search for extraterrestrial intelligence (SETI).

- Timeline for Development:

- Design work for the SKA is currently ongoing, with expectations for construction to begin in 2020 and operational readiness by around 2024.

8. Conclusion

- Summary of Key Points:

- Radio astronomy provides invaluable insights into the universe through the study of electromagnetic signals.

- The GMRT has been a pivotal facility in this field, with recent upgrades enhancing its capabilities.

- The SKA promises revolutionary advancements in radio astronomy, marking a new era in our understanding of the cosmos.

Powered by wisp

Related Posts
IUCAA Science Day: ASRT (Affordable Small Radio Telescope)

IUCAA Science Day: ASRT (Affordable Small Radio Telescope)

This report provides an overview of the Affordable Small Radio Telescope (ASRT) demonstration conducted during the National Science Day open house at the Inter-University Center for Astronomy and Astrophysics (IUCAA) on February 28, 2024. The ASRT operates within the Ku-band (12-16 GHz) of the radio spectrum and is designed to be cost-effective and easily replicable using off-the-shelf components. The primary objective of the ASRT is to observe solar emissions, leveraging the sun as a nearby star that emits radiation across all wavelengths of the electromagnetic spectrum. The report discusses the architecture and working principles of the ASRT, detailing its components such as the satellite dish antenna, satellite finder, mechanical mount, and electrical connections. The demonstration showcased the telescope's capability to conduct solar drift scans, providing valuable data about solar activity. The report emphasizes the potential of affordable radio telescopes like the ASRT to broaden access to advanced scientific research and highlights the contributions of various Indian institutes in solar observations.

Read Full Article
5- X-Ray Astronomy

5- X-Ray Astronomy

X-ray astronomy, emerging in the 1960s, studies celestial objects through their X-ray emissions, providing insights into high-energy phenomena like black holes and supernovae. The Astrosat mission enhances this field with multi-wavelength observations using instruments such as the Soft X-ray Telescope and Cadmium Zinc Telluride Imager. Key findings include variability in active galactic nuclei and the detection of gamma-ray bursts. Over the past 50 years, advancements in technology have propelled X-ray astronomy forward, contributing significantly to cosmology and our understanding of the universe. The analogy of the blind men and the elephant illustrates the need for multi-wavelength approaches in this research.

Read Full Article
An Overview of Radio Astronomy

An Overview of Radio Astronomy

Gautam Kulkarni delivered an engaging internal talk on "An Overview of Radio Astronomy" at VIIT's EnTC Department, attended by 22 students. The presentation covered the historical milestones in radio astronomy, key radiation sources such as the 21 cm hydrogen line and pulsars, and various antenna types. Kulkarni explained collaborative observations through interferometry and introduced the Giant Metrewave Radio Telescope (GMRT). The session fostered active audience engagement, including a Q&A, and inspired students to explore careers in astronomy. The Antariksh Club thanks Kulkarni for his valuable insights and the attendees for their participation.

Read Full Article
Radio Antennas: our ears in Radio Realm...

Radio Antennas: our ears in Radio Realm...

This report summarizes a presentation on antennas and their crucial role in radio astronomy, delivered during the IUCAA Science Day. It begins with an overview of the electromagnetic spectrum, emphasizing the characteristics of electromagnetic waves and their significance in detecting radio waves from Earth. The report details the fundamentals of antenna technology, exploring various types, including monopole, dipole, folded dipole, Yagi-Uda, log periodic, patch, and parabolic antennas, along with their operational principles and applications. The presentation culminates in an experimental demonstration of antenna transmission and reception, showcasing practical insights into optimizing antenna performance across different frequencies. Additionally, the report highlights contributions from prominent Indian institutes engaged in antenna research and development, underscoring their role in advancing radio astronomy and communication technologies.

Read Full Article
© Antariksh 2025