Communication performance of free space optical link using wavelength diversity in strong atmospheric turbulence
Abstract Atmospheric turbulence can be considered as one of the main problems facing FSO communication systems, which degrades the performance in terms of bit error rate. The objective of this paper is to examine the use of wavelength diversity in free-space optics to mitigate the effect of turbulen...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Kshatriya, Anil J. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2015 |
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| Schlagwörter: |
Free Space optical communication (FSO) |
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| Anmerkung: |
© The Optical Society of India 2015 |
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| Übergeordnetes Werk: |
Enthalten in: Journal of optics - [New Delhi] : Springer India, 1972, 44(2015), 3 vom: 05. Mai, Seite 215-219 |
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| Übergeordnetes Werk: |
volume:44 ; year:2015 ; number:3 ; day:05 ; month:05 ; pages:215-219 |
| Links: |
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| DOI / URN: |
10.1007/s12596-015-0248-7 |
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SPR026231557 |
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| 100 | 1 | |a Kshatriya, Anil J. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Communication performance of free space optical link using wavelength diversity in strong atmospheric turbulence |
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| 520 | |a Abstract Atmospheric turbulence can be considered as one of the main problems facing FSO communication systems, which degrades the performance in terms of bit error rate. The objective of this paper is to examine the use of wavelength diversity in free-space optics to mitigate the effect of turbulence on the received optical signal. As the refractive index variation will be different for different wavelengths, the fading is not same for different wavelength and different paths at the same time. The signals traveling through turbulent atmosphere undergo different amount of intensity fluctuations. The effect of atmospheric turbulence and scintillation cause intensity fluctuation of optical beam thus increasing the bit error rate (BER). In this paper wavelength diversity technique is proposed to reduce the fading under strong atmospheric turbulence condition. Mathematical expressions are derived for the estimation of the outage probability under strong atmospheric turbulence conditions and considerable improvement is found using wavelength diversity. | ||
| 650 | 4 | |a Free Space optical communication (FSO) |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Bit Error Rate (BER),Wavelength diversity |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Turbulence |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Acharya, Y. B. |4 aut | |
| 700 | 1 | |a Aggarwal, A. K. |4 aut | |
| 700 | 1 | |a Majumdar, A. K. |4 aut | |
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10.1007/s12596-015-0248-7 doi (DE-627)SPR026231557 (SPR)s12596-015-0248-7-e DE-627 ger DE-627 rakwb eng Kshatriya, Anil J. verfasserin aut Communication performance of free space optical link using wavelength diversity in strong atmospheric turbulence 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Optical Society of India 2015 Abstract Atmospheric turbulence can be considered as one of the main problems facing FSO communication systems, which degrades the performance in terms of bit error rate. The objective of this paper is to examine the use of wavelength diversity in free-space optics to mitigate the effect of turbulence on the received optical signal. As the refractive index variation will be different for different wavelengths, the fading is not same for different wavelength and different paths at the same time. The signals traveling through turbulent atmosphere undergo different amount of intensity fluctuations. The effect of atmospheric turbulence and scintillation cause intensity fluctuation of optical beam thus increasing the bit error rate (BER). In this paper wavelength diversity technique is proposed to reduce the fading under strong atmospheric turbulence condition. Mathematical expressions are derived for the estimation of the outage probability under strong atmospheric turbulence conditions and considerable improvement is found using wavelength diversity. Free Space optical communication (FSO) (dpeaa)DE-He213 Bit Error Rate (BER),Wavelength diversity (dpeaa)DE-He213 Turbulence (dpeaa)DE-He213 Acharya, Y. B. aut Aggarwal, A. K. aut Majumdar, A. K. aut Enthalten in Journal of optics [New Delhi] : Springer India, 1972 44(2015), 3 vom: 05. Mai, Seite 215-219 (DE-627)616732775 (DE-600)2533862-6 0974-6900 nnns volume:44 year:2015 number:3 day:05 month:05 pages:215-219 https://dx.doi.org/10.1007/s12596-015-0248-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 44 2015 3 05 05 215-219 |
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10.1007/s12596-015-0248-7 doi (DE-627)SPR026231557 (SPR)s12596-015-0248-7-e DE-627 ger DE-627 rakwb eng Kshatriya, Anil J. verfasserin aut Communication performance of free space optical link using wavelength diversity in strong atmospheric turbulence 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Optical Society of India 2015 Abstract Atmospheric turbulence can be considered as one of the main problems facing FSO communication systems, which degrades the performance in terms of bit error rate. The objective of this paper is to examine the use of wavelength diversity in free-space optics to mitigate the effect of turbulence on the received optical signal. As the refractive index variation will be different for different wavelengths, the fading is not same for different wavelength and different paths at the same time. The signals traveling through turbulent atmosphere undergo different amount of intensity fluctuations. The effect of atmospheric turbulence and scintillation cause intensity fluctuation of optical beam thus increasing the bit error rate (BER). In this paper wavelength diversity technique is proposed to reduce the fading under strong atmospheric turbulence condition. Mathematical expressions are derived for the estimation of the outage probability under strong atmospheric turbulence conditions and considerable improvement is found using wavelength diversity. Free Space optical communication (FSO) (dpeaa)DE-He213 Bit Error Rate (BER),Wavelength diversity (dpeaa)DE-He213 Turbulence (dpeaa)DE-He213 Acharya, Y. B. aut Aggarwal, A. K. aut Majumdar, A. K. aut Enthalten in Journal of optics [New Delhi] : Springer India, 1972 44(2015), 3 vom: 05. Mai, Seite 215-219 (DE-627)616732775 (DE-600)2533862-6 0974-6900 nnns volume:44 year:2015 number:3 day:05 month:05 pages:215-219 https://dx.doi.org/10.1007/s12596-015-0248-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 44 2015 3 05 05 215-219 |
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10.1007/s12596-015-0248-7 doi (DE-627)SPR026231557 (SPR)s12596-015-0248-7-e DE-627 ger DE-627 rakwb eng Kshatriya, Anil J. verfasserin aut Communication performance of free space optical link using wavelength diversity in strong atmospheric turbulence 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Optical Society of India 2015 Abstract Atmospheric turbulence can be considered as one of the main problems facing FSO communication systems, which degrades the performance in terms of bit error rate. The objective of this paper is to examine the use of wavelength diversity in free-space optics to mitigate the effect of turbulence on the received optical signal. As the refractive index variation will be different for different wavelengths, the fading is not same for different wavelength and different paths at the same time. The signals traveling through turbulent atmosphere undergo different amount of intensity fluctuations. The effect of atmospheric turbulence and scintillation cause intensity fluctuation of optical beam thus increasing the bit error rate (BER). In this paper wavelength diversity technique is proposed to reduce the fading under strong atmospheric turbulence condition. Mathematical expressions are derived for the estimation of the outage probability under strong atmospheric turbulence conditions and considerable improvement is found using wavelength diversity. Free Space optical communication (FSO) (dpeaa)DE-He213 Bit Error Rate (BER),Wavelength diversity (dpeaa)DE-He213 Turbulence (dpeaa)DE-He213 Acharya, Y. B. aut Aggarwal, A. K. aut Majumdar, A. K. aut Enthalten in Journal of optics [New Delhi] : Springer India, 1972 44(2015), 3 vom: 05. Mai, Seite 215-219 (DE-627)616732775 (DE-600)2533862-6 0974-6900 nnns volume:44 year:2015 number:3 day:05 month:05 pages:215-219 https://dx.doi.org/10.1007/s12596-015-0248-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 44 2015 3 05 05 215-219 |
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10.1007/s12596-015-0248-7 doi (DE-627)SPR026231557 (SPR)s12596-015-0248-7-e DE-627 ger DE-627 rakwb eng Kshatriya, Anil J. verfasserin aut Communication performance of free space optical link using wavelength diversity in strong atmospheric turbulence 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Optical Society of India 2015 Abstract Atmospheric turbulence can be considered as one of the main problems facing FSO communication systems, which degrades the performance in terms of bit error rate. The objective of this paper is to examine the use of wavelength diversity in free-space optics to mitigate the effect of turbulence on the received optical signal. As the refractive index variation will be different for different wavelengths, the fading is not same for different wavelength and different paths at the same time. The signals traveling through turbulent atmosphere undergo different amount of intensity fluctuations. The effect of atmospheric turbulence and scintillation cause intensity fluctuation of optical beam thus increasing the bit error rate (BER). In this paper wavelength diversity technique is proposed to reduce the fading under strong atmospheric turbulence condition. Mathematical expressions are derived for the estimation of the outage probability under strong atmospheric turbulence conditions and considerable improvement is found using wavelength diversity. Free Space optical communication (FSO) (dpeaa)DE-He213 Bit Error Rate (BER),Wavelength diversity (dpeaa)DE-He213 Turbulence (dpeaa)DE-He213 Acharya, Y. B. aut Aggarwal, A. K. aut Majumdar, A. K. aut Enthalten in Journal of optics [New Delhi] : Springer India, 1972 44(2015), 3 vom: 05. Mai, Seite 215-219 (DE-627)616732775 (DE-600)2533862-6 0974-6900 nnns volume:44 year:2015 number:3 day:05 month:05 pages:215-219 https://dx.doi.org/10.1007/s12596-015-0248-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 44 2015 3 05 05 215-219 |
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10.1007/s12596-015-0248-7 doi (DE-627)SPR026231557 (SPR)s12596-015-0248-7-e DE-627 ger DE-627 rakwb eng Kshatriya, Anil J. verfasserin aut Communication performance of free space optical link using wavelength diversity in strong atmospheric turbulence 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Optical Society of India 2015 Abstract Atmospheric turbulence can be considered as one of the main problems facing FSO communication systems, which degrades the performance in terms of bit error rate. The objective of this paper is to examine the use of wavelength diversity in free-space optics to mitigate the effect of turbulence on the received optical signal. As the refractive index variation will be different for different wavelengths, the fading is not same for different wavelength and different paths at the same time. The signals traveling through turbulent atmosphere undergo different amount of intensity fluctuations. The effect of atmospheric turbulence and scintillation cause intensity fluctuation of optical beam thus increasing the bit error rate (BER). In this paper wavelength diversity technique is proposed to reduce the fading under strong atmospheric turbulence condition. Mathematical expressions are derived for the estimation of the outage probability under strong atmospheric turbulence conditions and considerable improvement is found using wavelength diversity. Free Space optical communication (FSO) (dpeaa)DE-He213 Bit Error Rate (BER),Wavelength diversity (dpeaa)DE-He213 Turbulence (dpeaa)DE-He213 Acharya, Y. B. aut Aggarwal, A. K. aut Majumdar, A. K. aut Enthalten in Journal of optics [New Delhi] : Springer India, 1972 44(2015), 3 vom: 05. Mai, Seite 215-219 (DE-627)616732775 (DE-600)2533862-6 0974-6900 nnns volume:44 year:2015 number:3 day:05 month:05 pages:215-219 https://dx.doi.org/10.1007/s12596-015-0248-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 44 2015 3 05 05 215-219 |
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Kshatriya, Anil J. |
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Kshatriya, Anil J. misc Free Space optical communication (FSO) misc Bit Error Rate (BER),Wavelength diversity misc Turbulence Communication performance of free space optical link using wavelength diversity in strong atmospheric turbulence |
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Communication performance of free space optical link using wavelength diversity in strong atmospheric turbulence Free Space optical communication (FSO) (dpeaa)DE-He213 Bit Error Rate (BER),Wavelength diversity (dpeaa)DE-He213 Turbulence (dpeaa)DE-He213 |
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Kshatriya, Anil J. Acharya, Y. B. Aggarwal, A. K. Majumdar, A. K. |
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communication performance of free space optical link using wavelength diversity in strong atmospheric turbulence |
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Communication performance of free space optical link using wavelength diversity in strong atmospheric turbulence |
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Abstract Atmospheric turbulence can be considered as one of the main problems facing FSO communication systems, which degrades the performance in terms of bit error rate. The objective of this paper is to examine the use of wavelength diversity in free-space optics to mitigate the effect of turbulence on the received optical signal. As the refractive index variation will be different for different wavelengths, the fading is not same for different wavelength and different paths at the same time. The signals traveling through turbulent atmosphere undergo different amount of intensity fluctuations. The effect of atmospheric turbulence and scintillation cause intensity fluctuation of optical beam thus increasing the bit error rate (BER). In this paper wavelength diversity technique is proposed to reduce the fading under strong atmospheric turbulence condition. Mathematical expressions are derived for the estimation of the outage probability under strong atmospheric turbulence conditions and considerable improvement is found using wavelength diversity. © The Optical Society of India 2015 |
| abstractGer |
Abstract Atmospheric turbulence can be considered as one of the main problems facing FSO communication systems, which degrades the performance in terms of bit error rate. The objective of this paper is to examine the use of wavelength diversity in free-space optics to mitigate the effect of turbulence on the received optical signal. As the refractive index variation will be different for different wavelengths, the fading is not same for different wavelength and different paths at the same time. The signals traveling through turbulent atmosphere undergo different amount of intensity fluctuations. The effect of atmospheric turbulence and scintillation cause intensity fluctuation of optical beam thus increasing the bit error rate (BER). In this paper wavelength diversity technique is proposed to reduce the fading under strong atmospheric turbulence condition. Mathematical expressions are derived for the estimation of the outage probability under strong atmospheric turbulence conditions and considerable improvement is found using wavelength diversity. © The Optical Society of India 2015 |
| abstract_unstemmed |
Abstract Atmospheric turbulence can be considered as one of the main problems facing FSO communication systems, which degrades the performance in terms of bit error rate. The objective of this paper is to examine the use of wavelength diversity in free-space optics to mitigate the effect of turbulence on the received optical signal. As the refractive index variation will be different for different wavelengths, the fading is not same for different wavelength and different paths at the same time. The signals traveling through turbulent atmosphere undergo different amount of intensity fluctuations. The effect of atmospheric turbulence and scintillation cause intensity fluctuation of optical beam thus increasing the bit error rate (BER). In this paper wavelength diversity technique is proposed to reduce the fading under strong atmospheric turbulence condition. Mathematical expressions are derived for the estimation of the outage probability under strong atmospheric turbulence conditions and considerable improvement is found using wavelength diversity. © The Optical Society of India 2015 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">SPR026231557</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230331232730.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">201007s2015 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s12596-015-0248-7</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR026231557</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)s12596-015-0248-7-e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Kshatriya, Anil J.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Communication performance of free space optical link using wavelength diversity in strong atmospheric turbulence</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2015</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© The Optical Society of India 2015</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Atmospheric turbulence can be considered as one of the main problems facing FSO communication systems, which degrades the performance in terms of bit error rate. The objective of this paper is to examine the use of wavelength diversity in free-space optics to mitigate the effect of turbulence on the received optical signal. As the refractive index variation will be different for different wavelengths, the fading is not same for different wavelength and different paths at the same time. The signals traveling through turbulent atmosphere undergo different amount of intensity fluctuations. The effect of atmospheric turbulence and scintillation cause intensity fluctuation of optical beam thus increasing the bit error rate (BER). In this paper wavelength diversity technique is proposed to reduce the fading under strong atmospheric turbulence condition. Mathematical expressions are derived for the estimation of the outage probability under strong atmospheric turbulence conditions and considerable improvement is found using wavelength diversity.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Free Space optical communication (FSO)</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Bit Error Rate (BER),Wavelength diversity</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Turbulence</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Acharya, Y. B.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Aggarwal, A. K.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Majumdar, A. K.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Journal of optics</subfield><subfield code="d">[New Delhi] : Springer India, 1972</subfield><subfield code="g">44(2015), 3 vom: 05. Mai, Seite 215-219</subfield><subfield code="w">(DE-627)616732775</subfield><subfield code="w">(DE-600)2533862-6</subfield><subfield code="x">0974-6900</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:44</subfield><subfield code="g">year:2015</subfield><subfield code="g">number:3</subfield><subfield code="g">day:05</subfield><subfield code="g">month:05</subfield><subfield code="g">pages:215-219</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://dx.doi.org/10.1007/s12596-015-0248-7</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_SPRINGER</subfield></datafield><datafield tag="912" 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