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Optical properties of Titan and early Earth haze laboratory analogs in the mid-visible
Scattering and absorption of sunlight by aerosols are integral to understanding the radiative balance of any planetary atmosphere covered in a haze, such as Titan and possibly the early Earth. One key optical parameter of an aerosol is its refractive index. We have simulated both Titan and early Ear...
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Published in: | Icarus (New York, N.Y. 1962) N.Y. 1962), 2010-06, Vol.207 (2), p.903-913 |
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container_end_page | 913 |
container_issue | 2 |
container_start_page | 903 |
container_title | Icarus (New York, N.Y. 1962) |
container_volume | 207 |
creator | Hasenkopf, Christa A. Beaver, Melinda R. Trainer, Melissa G. Langley Dewitt, H. Freedman, Miriam A. Toon, Owen B. McKay, Christopher P. Tolbert, Margaret A. |
description | Scattering and absorption of sunlight by aerosols are integral to understanding the radiative balance of any planetary atmosphere covered in a haze, such as Titan and possibly the early Earth. One key optical parameter of an aerosol is its refractive index. We have simulated both Titan and early Earth organic haze aerosols in the laboratory and measured the real and imaginary portion of their refractive index at
λ
=
532
nm using cavity ringdown aerosol extinction spectroscopy. This novel technique allows analysis on freely-floating particles minutes after formation. For our Titan analog particles, we find a real refractive index of
n
=
1.35
±
0.01 and an imaginary refractive index
k
=
0.023
±
0.007, and for the early Earth analog particles we find
n
=
1.81
±
0.02 and
k
=
0.055
±
0.020. The Titan analog refractive index has a smaller real and similar imaginary refractive index compared to most previous laboratory measurements of Titan analog films, including values from Khare et al. (Khare, B.N., Sagan, C., Arakawa, E.T., Suits, F., Callcott, T.A., Williams, M.W. [1984]. Icarus 60, 127–137). These newly measured Titan analog values have implications for spacecraft retrievals of aerosol properties on Titan. The early Earth analog has a significantly higher real and imaginary refractive index than Titan analogs reported in the literature. These differences suggest that, for a given amount of aerosol, the early Earth analog would act as a stronger anti-greenhouse agent than the Titan analog. |
doi_str_mv | 10.1016/j.icarus.2009.12.015 |
format | article |
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λ
=
532
nm using cavity ringdown aerosol extinction spectroscopy. This novel technique allows analysis on freely-floating particles minutes after formation. For our Titan analog particles, we find a real refractive index of
n
=
1.35
±
0.01 and an imaginary refractive index
k
=
0.023
±
0.007, and for the early Earth analog particles we find
n
=
1.81
±
0.02 and
k
=
0.055
±
0.020. The Titan analog refractive index has a smaller real and similar imaginary refractive index compared to most previous laboratory measurements of Titan analog films, including values from Khare et al. (Khare, B.N., Sagan, C., Arakawa, E.T., Suits, F., Callcott, T.A., Williams, M.W. [1984]. Icarus 60, 127–137). These newly measured Titan analog values have implications for spacecraft retrievals of aerosol properties on Titan. The early Earth analog has a significantly higher real and imaginary refractive index than Titan analogs reported in the literature. These differences suggest that, for a given amount of aerosol, the early Earth analog would act as a stronger anti-greenhouse agent than the Titan analog.</description><identifier>ISSN: 0019-1035</identifier><identifier>EISSN: 1090-2643</identifier><identifier>DOI: 10.1016/j.icarus.2009.12.015</identifier><identifier>CODEN: ICRSA5</identifier><language>eng</language><publisher>Amsterdam: Elsevier Inc</publisher><subject>Aerosols ; Analogs ; Astronomy ; Earth ; Earth, ocean, space ; Exact sciences and technology ; Experimental techniques ; Haze ; Photochemistry ; Planetary atmospheres ; Refractive index ; Refractivity ; Retrieval ; Solar system ; Spectroscopy ; Sunlight ; Titan</subject><ispartof>Icarus (New York, N.Y. 1962), 2010-06, Vol.207 (2), p.903-913</ispartof><rights>2010 Elsevier Inc.</rights><rights>2015 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c467t-805f7ffbedb702ee1e588f3c5f417d3c2d5f6b2a6ef76a811d13a3df48ee3ae63</citedby><cites>FETCH-LOGICAL-c467t-805f7ffbedb702ee1e588f3c5f417d3c2d5f6b2a6ef76a811d13a3df48ee3ae63</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27901,27902</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=22806448$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Hasenkopf, Christa A.</creatorcontrib><creatorcontrib>Beaver, Melinda R.</creatorcontrib><creatorcontrib>Trainer, Melissa G.</creatorcontrib><creatorcontrib>Langley Dewitt, H.</creatorcontrib><creatorcontrib>Freedman, Miriam A.</creatorcontrib><creatorcontrib>Toon, Owen B.</creatorcontrib><creatorcontrib>McKay, Christopher P.</creatorcontrib><creatorcontrib>Tolbert, Margaret A.</creatorcontrib><title>Optical properties of Titan and early Earth haze laboratory analogs in the mid-visible</title><title>Icarus (New York, N.Y. 1962)</title><description>Scattering and absorption of sunlight by aerosols are integral to understanding the radiative balance of any planetary atmosphere covered in a haze, such as Titan and possibly the early Earth. One key optical parameter of an aerosol is its refractive index. We have simulated both Titan and early Earth organic haze aerosols in the laboratory and measured the real and imaginary portion of their refractive index at
λ
=
532
nm using cavity ringdown aerosol extinction spectroscopy. This novel technique allows analysis on freely-floating particles minutes after formation. For our Titan analog particles, we find a real refractive index of
n
=
1.35
±
0.01 and an imaginary refractive index
k
=
0.023
±
0.007, and for the early Earth analog particles we find
n
=
1.81
±
0.02 and
k
=
0.055
±
0.020. The Titan analog refractive index has a smaller real and similar imaginary refractive index compared to most previous laboratory measurements of Titan analog films, including values from Khare et al. (Khare, B.N., Sagan, C., Arakawa, E.T., Suits, F., Callcott, T.A., Williams, M.W. [1984]. Icarus 60, 127–137). These newly measured Titan analog values have implications for spacecraft retrievals of aerosol properties on Titan. The early Earth analog has a significantly higher real and imaginary refractive index than Titan analogs reported in the literature. These differences suggest that, for a given amount of aerosol, the early Earth analog would act as a stronger anti-greenhouse agent than the Titan analog.</description><subject>Aerosols</subject><subject>Analogs</subject><subject>Astronomy</subject><subject>Earth</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Experimental techniques</subject><subject>Haze</subject><subject>Photochemistry</subject><subject>Planetary atmospheres</subject><subject>Refractive index</subject><subject>Refractivity</subject><subject>Retrieval</subject><subject>Solar system</subject><subject>Spectroscopy</subject><subject>Sunlight</subject><subject>Titan</subject><issn>0019-1035</issn><issn>1090-2643</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNp9kLFqHDEQhhcTQy5O3iCFmpA0u9FIWmmvCQTjxAaDGzutmJVGPh17uxdJZzg_fWTOpHQ1xXz__MPXNJ-Bd8BBf9920WE65E5wvu5AdBz6s2YFfM1boZV816w4h3ULXPbvmw85bznn_bCWq-bP3b7U8MT2adlTKpEyWwK7jwVnhrNnhGk6sitMZcM2-ExswnFJWJZ0rHuclsfM4szKhtgu-vYp5jhO9LE5Dzhl-vQ6L5qHX1f3l9ft7d3vm8uft61T2pR24H0wIYzkR8MFEVA_DEG6PigwXjrh-6BHgZqC0TgAeJAofVADkUTS8qL5erpb3_97oFzsLmZH04QzLYdsjRZCGyVFJb-9SYI2IIQyYCqqTqhLS86Jgt2nuMN0tMDti3C7tSfh9kW4BWGr8Br78tqAuRoNCWcX8_-sEAPXSg2V-3HiqIp5ipRsdpFmRz4mcsX6Jb5d9A-QIpkb</recordid><startdate>20100601</startdate><enddate>20100601</enddate><creator>Hasenkopf, Christa A.</creator><creator>Beaver, Melinda R.</creator><creator>Trainer, Melissa G.</creator><creator>Langley Dewitt, H.</creator><creator>Freedman, Miriam A.</creator><creator>Toon, Owen B.</creator><creator>McKay, Christopher P.</creator><creator>Tolbert, Margaret A.</creator><general>Elsevier Inc</general><general>Elsevier</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20100601</creationdate><title>Optical properties of Titan and early Earth haze laboratory analogs in the mid-visible</title><author>Hasenkopf, Christa A. ; Beaver, Melinda R. ; Trainer, Melissa G. ; Langley Dewitt, H. ; Freedman, Miriam A. ; Toon, Owen B. ; McKay, Christopher P. ; Tolbert, Margaret A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c467t-805f7ffbedb702ee1e588f3c5f417d3c2d5f6b2a6ef76a811d13a3df48ee3ae63</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Aerosols</topic><topic>Analogs</topic><topic>Astronomy</topic><topic>Earth</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Experimental techniques</topic><topic>Haze</topic><topic>Photochemistry</topic><topic>Planetary atmospheres</topic><topic>Refractive index</topic><topic>Refractivity</topic><topic>Retrieval</topic><topic>Solar system</topic><topic>Spectroscopy</topic><topic>Sunlight</topic><topic>Titan</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hasenkopf, Christa A.</creatorcontrib><creatorcontrib>Beaver, Melinda R.</creatorcontrib><creatorcontrib>Trainer, Melissa G.</creatorcontrib><creatorcontrib>Langley Dewitt, H.</creatorcontrib><creatorcontrib>Freedman, Miriam A.</creatorcontrib><creatorcontrib>Toon, Owen B.</creatorcontrib><creatorcontrib>McKay, Christopher P.</creatorcontrib><creatorcontrib>Tolbert, Margaret A.</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>Icarus (New York, N.Y. 1962)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hasenkopf, Christa A.</au><au>Beaver, Melinda R.</au><au>Trainer, Melissa G.</au><au>Langley Dewitt, H.</au><au>Freedman, Miriam A.</au><au>Toon, Owen B.</au><au>McKay, Christopher P.</au><au>Tolbert, Margaret A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Optical properties of Titan and early Earth haze laboratory analogs in the mid-visible</atitle><jtitle>Icarus (New York, N.Y. 1962)</jtitle><date>2010-06-01</date><risdate>2010</risdate><volume>207</volume><issue>2</issue><spage>903</spage><epage>913</epage><pages>903-913</pages><issn>0019-1035</issn><eissn>1090-2643</eissn><coden>ICRSA5</coden><abstract>Scattering and absorption of sunlight by aerosols are integral to understanding the radiative balance of any planetary atmosphere covered in a haze, such as Titan and possibly the early Earth. One key optical parameter of an aerosol is its refractive index. We have simulated both Titan and early Earth organic haze aerosols in the laboratory and measured the real and imaginary portion of their refractive index at
λ
=
532
nm using cavity ringdown aerosol extinction spectroscopy. This novel technique allows analysis on freely-floating particles minutes after formation. For our Titan analog particles, we find a real refractive index of
n
=
1.35
±
0.01 and an imaginary refractive index
k
=
0.023
±
0.007, and for the early Earth analog particles we find
n
=
1.81
±
0.02 and
k
=
0.055
±
0.020. The Titan analog refractive index has a smaller real and similar imaginary refractive index compared to most previous laboratory measurements of Titan analog films, including values from Khare et al. (Khare, B.N., Sagan, C., Arakawa, E.T., Suits, F., Callcott, T.A., Williams, M.W. [1984]. Icarus 60, 127–137). These newly measured Titan analog values have implications for spacecraft retrievals of aerosol properties on Titan. The early Earth analog has a significantly higher real and imaginary refractive index than Titan analogs reported in the literature. These differences suggest that, for a given amount of aerosol, the early Earth analog would act as a stronger anti-greenhouse agent than the Titan analog.</abstract><cop>Amsterdam</cop><pub>Elsevier Inc</pub><doi>10.1016/j.icarus.2009.12.015</doi><tpages>11</tpages></addata></record> |
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subjects | Aerosols Analogs Astronomy Earth Earth, ocean, space Exact sciences and technology Experimental techniques Haze Photochemistry Planetary atmospheres Refractive index Refractivity Retrieval Solar system Spectroscopy Sunlight Titan |
title | Optical properties of Titan and early Earth haze laboratory analogs in the mid-visible |
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