activity
20092023
most citedPerformance of centroiding algorithms at low light level conditions in adaptive optics

23 citations · 91 across the 17 of their papers we have counts for

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Showing astro-ph.IMShow all

14 papers · 1 filter

astro-ph.IM2022★ 4 cited

Data Pipeline Architecture and Development for VELC onboard Space Solar Mission AdityaL1

Jagdev Singh, B. Raghavendra Prasad, Chavali Sumana +4

ADITYA L-1 is India's first dedicated mission to study Sun and its atmosphere with Visible Emission Line Coronagraph (VELC), a major payload on ADITYA-L1. VELC has provision to mak…

astro-ph.IM2021★ 8 cited

Spectropolarimeter on-board the Aditya-L1: Polarization Modulation and Demodulation

K. Nagaraju, B. Raghavendra Prasad, Bhavana S. Hegde +5

One of the major science goals of the Visible Emission Line Coronagraph (VELC) payload aboard the Aditya-L1 mission is to map the coronal magnetic field topology and the quantitati…

astro-ph.IM2019★ 1 cited

Prospect for UV observations from the Moon. III. Assembly and ground calibration of Lunar Ultraviolet Cosmic Imager (LUCI)

Joice Mathew, B. G. Nair, Margarita Safonova +14

The Lunar Ultraviolet Cosmic Imager (LUCI) is a near-ultraviolet (NUV) telescope with all-spherical mirrors, designed and built to fly as a scientific payload on a lunar mission wi…

astro-ph.IM2010★ 3 cited

Extrapolating Zernike Moments to Predict Future Optical Wave-fronts in Adaptive Optics Using Real Time Data Mining

Akondi Vyas, M. B. Roopashree, B. Raghavendra Prasad

We present the details of predicting atmospheric turbulence by mining Zernike moment data obtained from simulations as well as experiments. Temporally correlated optical wave-front…

astro-ph.IM2010★ 23 cited

Performance of centroiding algorithms at low light level conditions in adaptive optics

Akondi Vyas, M. B. Roopashree, B. Raghavendra Prasad

The performance metrics of different centroiding algorithms at low light level conditions were optimized in the case of a Shack Hartmann Sensor (SHS) for efficient performance of t…

astro-ph.IM2009★ 2 cited

Prediction of wavefronts in adaptive optics to reduce servo lag errors using data mining

Akondi Vyas, M B Roopashree, B Raghavendra Prasad

Servo lag errors in adaptive optics lead to inaccurate compensation of wavefront distortions. An attempt has been made to predict future wavefronts using data mining on wavefronts…

astro-ph.IM2009★ 3 cited

Digital long focal length lenslet array using spatial light modulator

Akondi Vyas, M B Roopashree, B Raghavendra Prasad

Under a thin lens and paraxial approximation, the phase transformation function of a lens was simulated on a Liquid Crystal (LC) based Spatial Light Modulator (SLM). The properties…

astro-ph.IM2009★ 1 cited

Effective coherence length estimation of optical wavefronts

Akondi Vyas, M. B. Roopashree, B. Raghavendra Prasad

In adaptive optics, the measurement of spatial coherence length helps in deciding the optimum design parameters of a Shack Hartmann Sensor (SHS). Two methods of estimating the spat…

astro-ph.IM2009★ 1 cited

Performance analysis of Fourier and Vector Matrix Multiply methods for phase reconstruction from slope measurements

M B Roopashree, Akondi Vyas, B Raghavendra Prasad

The accuracy of wavefront reconstruction from discrete slope measurements depends on the sampling geometry, coherence length of the incoming wavefronts, wavefront sensor specificat…

astro-ph.IM2009★ 5 cited

Centroid Detection by Gaussian Pattern Matching in Adaptive Optics

Akondi Vyas, M B Roopashree, B Raghavendra Prasad

Shack Hartmann wavefront sensor is a two dimensional array of lenslets which is used to detect the incoming phase distorted wavefront through local tilt measurements made by record…

astro-ph.IM2009★ 1 cited

Spatial Light Modulator for wavefront correction

Akondi Vyas, M. B. Roopashree, Ravinder Kumar Banyal +1

We present a liquid crystal method of correcting the phase of an aberrated wavefront using a spatial light modulator. A simple and efficient lab model has been demonstrated for wav…

astro-ph.IM2009★ 4 cited

Progressive Prediction of Turbulence Using Wave-Front Sensor Data in Adaptive Optics Using Data Mining

Akondi Vyas, M B Roopashree, B Raghavendra Prasad

Nullifying the servo bandwidth errors improves the strehl ratio by a substantial quantity in adaptive optics systems. An effective method for predicting atmospheric turbulence to r…

astro-ph.IM2009★ 3 cited

Denoising Shack Hartmann Sensor spot pattern using Zernike Reconstructor

Akondi Vyas, M B Roopashree, B Raghavendra Prasad

Shack Hartmann Sensor (SHS) is inflicted with significant background noise that deteriorates the wave-front reconstruction accuracy. In this paper, a simple method to remove the ba…

astro-ph.IM2009★ 12 cited

Optimization of Existing Centroiding Algorithms for Shack Hartmann Sensor

Akondi Vyas, M B Roopashree, B R Prasad

Three centroiding techniques to estimate the position of the spots in a Shack Hartmann sensor: Normalized Centre of Gravity (CoG), Iteratively Weighted Centre of Gravity (IWCoG) an…