IIA Institutional Repository: Recent submissions

  • Joby, P. K (Indian Institute of Astrophysics, 2019-01)
    The Cosmic Microwave Background (CMB) is the oldest light in the Universe and gives us access to a picture of the Universe when it was only ≈ 300,000 years old. The CMB radiation consists of photons free streaming to us ...
  • Mathew, Joice (Indian Institute of Astrophysics, 2018-06)
    The Ultraviolet (UV) domain plays an important role in studying transient events, the atmosphere of stars and planets, characteristics of the interstellar medium, young stellar populations, physical properties of galaxies ...
  • Kishore, P (Indian Institute of Astrophysics, 2016-08)
    Energetic emission from the Sun can be divided into two broad categories, viz. gradual and impulsive. It is inferred from white-light observations that the first group is associated with mass ejections from the solar ...
  • Mageshwaran, T (Indian Institute of Astrophysics, 2017-11)
    A nearly self contained and detailed introduction to TDE physics with novel aspects and a summary of observations is provided. We have constructed a dynamical model of tidal disruption events (TDEs) that includes physical ...
  • Prasad, Avijeet (Indian Institute of Astrophysics, 2015-05)
    Magnetic fields are ubiquitous in the universe and play an important role in variety of astrophysical phenomenon. It is thus very important to understand the origin, structure and strength of these astrophysical magnetic ...
  • Manpreet Singh (Indian Institute of Astrophysics, 2015-04)
    The study of ultracold atoms is one of the frontier research areas of modern physics. The ability to control precisely the interactions between the ultracold atoms in optical lattices has led to the prediction and in ...
  • Mugundhan, V (Indian Institute of Astrophysics, 2018-10)
    Low frequency radio observations of the solar corona provide valuable information on the heliocentric distance range ≈ 1.1R - 3R , which is relatively difficult to observe from other wavelengths. These observations are ...
  • Narang, Nancy (Indian Institute of Astrophysics, 2019-07)
    The solar atmosphere is populated with various small-scale features which are observed to be very dynamic and highly structured. The advent of modern instruments with high spatial, spectral and temporal resolution, have ...
  • Nirmal, K (Indian Institute of Astrophysics, 2018-09)
    We describe the development of compact, lightweight payloads suitable for ground, space, and balloon-based observatories. The first instrument is a compact high resolution (≥ 20000) tunable spatial heterodyne spectrom- eter ...
  • Panini, Singam Srikanth (Indian Institute of Astrophysics, 2019-03)
    The recent progress in the development of multilayer mirrors has revolutionized the field of astronomical X-rays optics. A variety of multilayer mirrors are now being developed for several unique applications such as ...
  • Chitta, Lakshmi Pradeep (Indian Institute of Astrophysics, 2014-06)
    The surface of the Sun and solar-type stars is permeated by magnetic fields with a va- riety of spatial and temporal scales. The spatial scales range from sub-arcsec tangled fields that are yet to be observed (inaccessible ...
  • Mohan, Prashanth (Indian Institute of Astrophysics, 2013-09)
  • Priyanka Rani (Indian Institute of Astrophysics, 2019-02)
    Flux variability is one of the defining characteristics of active galactic nuclei (AGN). This has been known over the past six decades ever since the discov- ery of quasars in 1963. Since then AGN have been observed ...
  • Ramya, M. Anche (Indian Institute of Astrophysics, 2019-02)
    Polarimetric observations of celestial objects reveal information regarding magnetic field, scattered dust and planetary atmosphere. The degree of po- larization, which is of interest to astronomers, ranges from ...
  • Rubinur, K (Indian Institute of Astrophysics, 2019-04)
    This thesis is aimed at studying dual nuclei in galaxies using radio and UV observations. Dual nuclei are formed during galaxy mergers in our Universe. Since we know that almost all nearby galaxies host a super-massive ...
  • Sajal Kumar Dhara (Indian Institute of Astrophysics, 2015-08)
    The solar atmosphere is structured by the evolving magnetic fields. These structures occur on different spatial scales. On small scale - bright points with thin boundaries have been observed. On large spatial scale - ...
  • Sen, Samrat (Indian Institute of Astrophysics, 2020-01)
    The study of magnetic fluxtubes is a very important aspect as it plays an important role in several astrophysical phenomena in the solar atmosphere. Thus, it is very important to understand the properties and structures ...
  • Sarpotdar, Mayuresh N (Indian Institute of Astrophysics, 2018-10)
    At Indian Institute of Astrophysics, we conduct high altitude balloon ex- periments for atmospheric and astronomical observations in UV wavelength range. To carry out observations of astronomical sources, a fine pointing ...
  • Srivastav, S (Indian Institute of Astrophysics, 2017-02)
    Supernovae (SNe) are explosive transient events that mark the end stage of stellar evolution. This work presents a study of low redshift, hydrogen deficient (Type I) SNe, with emphasis on SNe of type Ia. The data were ...
  • Sindhu, N (Indian Institute of Astrophysics, 2019-08)
    The thesis focuses on understanding the single and binary stellar evolution in the old open clusters, M67 and NGC 188 using multiwavelength photometric data. We have used images from the Ultra-Violet Imaging Telescope ...

Search DSpace

Browse

My Account