UV Imaging Telescope - UVIT. The Ultra Violet Imaging Telescope onboard ASTROSAT. Some of the most interesting scientific aims of the proposed ASTROSAT. The UVIT is a part of Astrosat Mission. By Indian Space Research Organization. This website is maintained by the UVIT Payload Operations Centre at Indian Institute of Astrophysics.
http://uvit.iiap.res.in/
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UV Imaging Telescope - UVIT | UVIT | uvit.iiap.res.in Reviews
https://uvit.iiap.res.in
UV Imaging Telescope - UVIT. The Ultra Violet Imaging Telescope onboard ASTROSAT. Some of the most interesting scientific aims of the proposed ASTROSAT. The UVIT is a part of Astrosat Mission. By Indian Space Research Organization. This website is maintained by the UVIT Payload Operations Centre at Indian Institute of Astrophysics.
uvit.iiap.res.in
Science with UVIT | UVIT
http://uvit.iiap.res.in/Science
The UVIT telescopes offer unique capabilities, and are expected to be the most capable UV telescopes during their time in orbit. The primary strengths are:. Arc-second resolution over a wide (30') field of view. Time resolution as short as 600 Hz. A wide range of filters, along with gratings in FUV and NUV. Simultaneous observations in 3 bands - FUV, NUV and Visible. Simultaneous observations alongside X-ray timing and imaging telescopes onboard Astrosat. Science Highlights and Objectives.
Instrument | UVIT
http://uvit.iiap.res.in/Instrument
Ph counting, CCD. Twin Ritchie Chretian, 2 mirror system. The overall structure is shown below. Those parts of the telescopes which define locations of the optical elements are mostly made of Invar36, and the other parts are made of Aluminium alloy. The two telescopes are mounted on a cone-like structure of Titanium, which is attached to central cylinder of the S/C. There are three main contributors to the PSF: optics, detector, and drift of the aspect. Of these three the largest contribution is made...
Software | UVIT
http://uvit.iiap.res.in/Software
Bright Source Warning (Beta). Provides exposure time needed for different classes of objects for a given S/N or, alternatively, to calculate the S/N for a given exposure time. Usage Help and Documentation. Bright Source Warning Tool. Checks for bright stars in a given field of view and checks if the field is observable by UVIT. Usage Help and Documentation. Bright Source Warning Tool. The UVIT is a part of Astrosat Mission. By Indian Space Research Organization.
Intranet | UVIT
http://uvit.iiap.res.in/access
The UVIT is a part of Astrosat Mission. By Indian Space Research Organization. This website is maintained by the UVIT Payload Operations Centre at Indian Institute of Astrophysics.
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Scientific Objectives | aditya.iiap.res.in
http://aditya.iiap.res.in/science
Coronal waves as a source of coronal heating. Dynamics of coronal loops:formation and evolution. Temperaturediagnostics of the corona using line ratiotechiniques. Development, dynamics and origin of CMEs. Vital inputs to Space weather Prediction. Topology of magnetic fields. Important Properties of the Corona. Outer atmosphere of the sun is known as solar corona. Coronal intensities in the visible wavelength is million time fainter compared to the disk intensities. Density at the limb is about 10.
User account | aditya.iiap.res.in
http://aditya.iiap.res.in/user
Enter your aditya.iiap.res.in username. Enter the password that accompanies your username.
Optical Layout | aditya.iiap.res.in
http://aditya.iiap.res.in/optical-layout
Secondary Mirror to eject the disk light through a central hole and reflect the coronal light. Mirror to send out the disk light from the payload. Lyot Stop to cut of the Diffraction from the EA. Narrow Band Image Plane (Green Emission Line). Narrow Band Image Plane (Red Emission Line).
Science Working Group | aditya.iiap.res.in
http://aditya.iiap.res.in/scienceworkinggroup
Dipankar Banerjee (will be responsible for coordination between different groups and also participate in sub-group discussions and activities). The following sub-groups have been identified with specific science goals. Diagnostics of Coronal Loops,. Including heating and cooling. Durgesh Tripathi (lead),. B N Dwivedi,. Durgesh@ iucaa.ernet.in,. Bholadwivedi@ gmail.com, kpr@ iiap.res.in. P Venkatakrishnan (lead),. Pvk@ prl.res.in. Satya@ iiap.res.in. Transients (small and large scale). B Ravindra (lead),.
Events | aditya.iiap.res.in
http://aditya.iiap.res.in/node/42
Aditya Science Meet 2013.
Uniqueness of the Payload | aditya.iiap.res.in
http://aditya.iiap.res.in/payload
Uniqueness of the Payload. Simultaneous emission line images in the green and red emission lines allowing for temperature diagnostics. Very High Cadence(3-images per second). Simultaneous Polarization images in the continuum and line allowing for density diagnostics, magnetic topology, and 3D structure of CMEs. Observations close to the limb(better than 1.1 Rsun). Highly polished primary mirror - Micro roughness of the order of 1Å; an order better than the current technology.
Project Team | aditya.iiap.res.in
http://aditya.iiap.res.in/project-team
Deputy Project Directors :. Sanjay Gupta, ISAC. Abhijit Avinash Adoni, ISAC. Paratha Bandopadhyay, ISAC. GVP Bharatkumar, ISAC. NHemanth Kumar Reddy, ISAC. VVinu Viswanath, VSSC. DPD (DH and SSR). Sajjade Faisal Mustafa, ISAC. DPD (R and QA). DPD (ISTRAC,Ele.). ProfJagdev Singh,IIA,Bangalore. DrDipankar Banerjee,IIA,Bangalore. ProfP .Venkatakrishna,USO/PRL,Udalpur. ProfBRaghavendra Prasad,IIA,Bangalor. Shri R.Venkateswaran,LEOS,Bangalore. Shri Asit Patra,SAC,Ahmedabad. Programme Director, IRS and SSS.
Papers | aditya.iiap.res.in
http://aditya.iiap.res.in/papers
Proposed Visible Emission Line Space Solar Coronagraph.
Publications | kso.iiap.res.in
https://kso.iiap.res.in/publications
Listed below are the refereed publications that has utilized data and/or resources from Kodaikanal Observatory, obtained from NASA-ADS. Poljančić, I. Brajša, R. Hržina, D. Wöhl, H. Hanslmeier, A. Pötzi, W. Baranyi, T. Özgüç, A. Singh, J. Ruždjak, V. Differences in heliographic positions and rotation velocities of sunspot groups from various observatories. Hajra, R. Chakraborty, S. K. Dasgupta, A. Sivaraman, K. R. Sivaraman, H. Gupta, S. S. Howard, R. F. The Mount Wilson Ca ii K Plage Index Time Series.
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UV Imaging Telescope - UVIT | UVIT
UV Imaging Telescope - UVIT. The Ultra Violet Imaging Telescope onboard ASTROSAT. Some of the most interesting scientific aims of the proposed ASTROSAT. The UVIT is a part of Astrosat Mission. By Indian Space Research Organization. This website is maintained by the UVIT Payload Operations Centre at Indian Institute of Astrophysics.
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