Feasibility of Cosmic Object Detection Using a Solar FSR System

Hristo Kabakchiev; Vera Behar; Ivan Garvanov; Dorina Kabakchieva; Avgust Kabakchiev; Panayot Daskalov; Herman Rohling; Mark Bentum; Jorge Fernandes

doi:10.1109/SPS.2019.8882062

Feasibility of Cosmic Object Detection Using a Solar FSR System

Hristo Kabakchiev
, Vera Behar
, Ivan Garvanov
, Dorina Kabakchieva
, Avgust Kabakchiev
, Panayot Daskalov
, Herman Rohling
, Mark Bentum
, Jorge Fernandes

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Academic › peer-review

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Abstract

The article analyses the possibility of the forward scatter radar method for detecting large-sized cosmic objects when using emission of the Sun as probing signals. The method of the forward scatter radar is based on the phenomenon of a significant increase the bistatic target radar cross section when the probe signal is scattered forward, i.e. along direction of the principal beam of locator pattern.

Original language	English
Title of host publication	2019 Signal Processing Symposium (SPSympo)
Place of Publication	USA
Publisher	IEEE
Pages	57-60
Number of pages	4
ISBN (Electronic)	978-1-7281-1715-7
ISBN (Print)	978-1-7281-1716-4
DOIs	https://doi.org/10.1109/SPS.2019.8882062
Publication status	Published - 24 Oct 2019
Event	Signal Processing Symposium, SPSympo 2019 - Krakow, Poland Duration: 17 Sept 2019 → 19 Sept 2019

Conference

Conference	Signal Processing Symposium, SPSympo 2019
Abbreviated title	SPSympo 2019
Country/Territory	Poland
City	Krakow
Period	17/09/19 → 19/09/19

Keywords

diffraction
forward scatter effect
radar

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10.1109/SPS.2019.8882062

Cite this

@inproceedings{39caf47a57a64afaa2f764aa7f57ffb4,

title = "Feasibility of Cosmic Object Detection Using a Solar FSR System",

abstract = "The article analyses the possibility of the forward scatter radar method for detecting large-sized cosmic objects when using emission of the Sun as probing signals. The method of the forward scatter radar is based on the phenomenon of a significant increase the bistatic target radar cross section when the probe signal is scattered forward, i.e. along direction of the principal beam of locator pattern.",

keywords = "diffraction, forward scatter effect, radar",

author = "Hristo Kabakchiev and Vera Behar and Ivan Garvanov and Dorina Kabakchieva and Avgust Kabakchiev and Panayot Daskalov and Herman Rohling and Mark Bentum and Jorge Fernandes",

year = "2019",

month = oct,

day = "24",

doi = "10.1109/SPS.2019.8882062",

language = "English",

isbn = "978-1-7281-1716-4",

pages = "57--60",

booktitle = "2019 Signal Processing Symposium (SPSympo)",

publisher = "IEEE",

address = "United States",

note = "Signal Processing Symposium, SPSympo 2019, SPSympo 2019 ; Conference date: 17-09-2019 Through 19-09-2019",

}

Kabakchiev, H, Behar, V, Garvanov, I, Kabakchieva, D, Kabakchiev, A, Daskalov, P, Rohling, H, Bentum, M & Fernandes, J 2019, Feasibility of Cosmic Object Detection Using a Solar FSR System. in 2019 Signal Processing Symposium (SPSympo)., 8882062, IEEE, USA, pp. 57-60, Signal Processing Symposium, SPSympo 2019, Krakow, Poland, 17/09/19. https://doi.org/10.1109/SPS.2019.8882062

TY - GEN

T1 - Feasibility of Cosmic Object Detection Using a Solar FSR System

AU - Kabakchiev, Hristo

AU - Behar, Vera

AU - Garvanov, Ivan

AU - Kabakchieva, Dorina

AU - Kabakchiev, Avgust

AU - Daskalov, Panayot

AU - Rohling, Herman

AU - Bentum, Mark

AU - Fernandes, Jorge

PY - 2019/10/24

Y1 - 2019/10/24

N2 - The article analyses the possibility of the forward scatter radar method for detecting large-sized cosmic objects when using emission of the Sun as probing signals. The method of the forward scatter radar is based on the phenomenon of a significant increase the bistatic target radar cross section when the probe signal is scattered forward, i.e. along direction of the principal beam of locator pattern.

AB - The article analyses the possibility of the forward scatter radar method for detecting large-sized cosmic objects when using emission of the Sun as probing signals. The method of the forward scatter radar is based on the phenomenon of a significant increase the bistatic target radar cross section when the probe signal is scattered forward, i.e. along direction of the principal beam of locator pattern.

KW - diffraction

KW - forward scatter effect

KW - radar

UR - https://www.scopus.com/pages/publications/85074902525

U2 - 10.1109/SPS.2019.8882062

DO - 10.1109/SPS.2019.8882062

M3 - Conference contribution

SN - 978-1-7281-1716-4

SP - 57

EP - 60

BT - 2019 Signal Processing Symposium (SPSympo)

PB - IEEE

CY - USA

T2 - Signal Processing Symposium, SPSympo 2019

Y2 - 17 September 2019 through 19 September 2019

ER -

Feasibility of Cosmic Object Detection Using a Solar FSR System

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