Arun kumar Singh

Mr. Arun kumar Singh

orcid

Research Focus & Metrics

Academic Career Length

8Years (2019-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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1 December 2020 in Acta Astronautica
Verified
Journal Article
Closed access
KRKanaka Durga Reddybattula
Kanaka Durga Reddybattula
SPSampad Kumar Panda
Sampad Kumar Panda
SSSunil Kumar Sharma
Sunil Kumar Sharma
ASArun kumar Singh
Arun kumar Singh
KKKasmira Kurnala
Kasmira Kurnala
SWSamyuktha Wuyyuru
Samyuktha Wuyyuru

1 September 2020 in Acta Astronautica
Verified
Journal Article
Closed access
SSSunil Kumar Sharma
Sunil Kumar Sharma
ASArun kumar Singh
Arun kumar Singh
SPSampad Kumar Panda
Sampad Kumar Panda
Kutubuddin AnsariKutubuddin Ansari
Kutubuddin Ansari

30 March 2021 in Journal of Geophysical Research: Space Physics
Verified
Journal Article
Open access
PDF file
ASArun kumar Singh
Arun kumar Singh
HHHaris Haralambous
Haris Haralambous
COChristina Oikonomou
Christina Oikonomou
We examine systematic differences between topside electron density measurements and different topside model formulations including α‐Chapman, NeQuick, and an improved NeQuick (NeQuick‐corr) topside formulation, recently proposed. The global topside electron density data set used, was extracted from Radio Occultation (RO) topside electron density profiles on board Low‐Earth Orbit satellites from the COSMIC/FORMOSAT‐3 (Constellation Observing System for Meteorology, Ionosphere, and Climate and Formosa Satellite) mission. By using RO topside electron density measurements collocated with digisonde stations, we ensure that our investigation is based on two independent data sets (RO and digisondes). A subset of these profiles, with matched (within 5%) peak RO‐digisonde characteristics (foF2 and hmF2) is also exploited. This subset is exploited to extend the investigation on the basis of a higher quality validation data set. The comparison demonstrates that α‐Chapman and NeQuick‐corr underestimate, whereas NeQuick overestimates COSMIC topside electron density observations. The main outcome of this study is the significant NeQuick topside representation improvement that can be achieved near the F region peak, if the key parameter g, which controls the change of scale height with respect to altitude, is optimized to a value of 0.15 (compared to a currently adopted value of 0.125). The NeQuick‐corr topside formulation using the optimized g value of 0.15 outperforms all other topside formulations.

28 May 2021 in Atmosphere
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Journal Article
Open access
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HHHaris Haralambous
Haris Haralambous
TLTheodoros Leontiou
Theodoros Leontiou
VPVasilis Petrou
Vasilis Petrou
ASArun kumar Singh
Arun kumar Singh
MCMarios Charalambides
Marios Charalambides
AAAgis Agisilaou
Agis Agisilaou
The objective of this article is to present a concept for single-frequency Global Navigation Satellite System (GNSS) positioning local ionospheric mitigation over a certain area. This concept is based on input parameters driving the NeQuick-G algorithm (the ionospheric single-frequency GNSS correction algorithm adopted by Galileo GNSS system), estimated on a local as opposed to a global scale, from ionospheric characteristics measured by a digital ionosonde and a collocated dual-frequency Total Electron Content (TEC) monitor. This approach facilitates the local adjustment of Committee Consultative for Ionospheric Radiowave propagation (CCIR) files and the Az ionization level, which control the ionospheric electron density profile in NeQuick-G, therefore enabling better estimation of positioning errors under quiet geomagnetic conditions. This novel concept for local ionospheric positioning error mitigation may be adopted at any location where ionospheric characteristics foF2 and M(3000)F2 can be measured, as a means to enhance the accuracy of single-frequency positioning applications based on the NeQuick-G algorithm.


1 June 2019 in Advances In Space Research
Verified
Journal Article
Closed access
ASArun kumar Singh
Arun kumar Singh
RDRupesh M. Das
Rupesh M. Das
SSShailendra Saini
Shailendra Saini