Advanced Net Flux Radiometer for the Ice Giants
The design of an advanced Net Flux Radiometer (NFR), for inclusion as a payload on a future Ice Giants probe mission, is given. The Ice Giants NFR (IG-NFR) will measure the upward and downward radiation flux (hence net radiation flux), in seven spectral bands, spanning the range from solar to far in...
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| Veröffentlicht in: | Space science reviews 2020-02, Vol.216 (1), Article 11 |
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| creator | Aslam, S. Achterberg, R. K. Calcutt, S. B. Cottini, V. Gorius, N. J. Hewagama, T. Irwin, P. G. Nixon, C. A. Quilligan, G. Roos-Serote, M. Simon, A. A. Tran, D. Villanueva, G. |
| description | The design of an advanced Net Flux Radiometer (NFR), for inclusion as a payload on a future Ice Giants probe mission, is given. The Ice Giants NFR (IG-NFR) will measure the upward and downward radiation flux (hence net radiation flux), in seven spectral bands, spanning the range from solar to far infra-red wavelengths, each with a
5
∘
Field-Of-View (FOV) and in five sequential view angles (
±
80
∘
,
±
45
∘
, and
0
∘
) as a function of altitude. IG-NFR measurements within either Uranus or Neptune’s atmospheres, using dedicated spectral filter bands will help derive radiative heating and cooling profiles, and will significantly contribute to our understanding of the planet’s atmospheric heat balance and structure, tropospheric 3-D flow, and compositions and opacities of the cloud layers. The IG-NFR uses an array of non-imaging Winston cones integrated to a matched thermopile detector Focal Plane Assembly (FPA), with individual bandpass filters, housed in a diamond windowed vacuum micro-vessel. The FPA thermopile detector signals are read out in parallel mode, amplified and processed by a multi-channel digitizer application specific integrated circuit (MCD ASIC) under field programmable gate array (FPGA) control. The vacuum micro-vessel rotates providing chopping between FOV’s of upward and downward radiation fluxes. This unique design allows for small net flux measurements in the presence of large ambient fluxes and rapidly changing ambient temperatures during the probe descent to
≥
10
bar pressure. |
| doi_str_mv | 10.1007/s11214-019-0630-x |
| format | Article |
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5
∘
Field-Of-View (FOV) and in five sequential view angles (
±
80
∘
,
±
45
∘
, and
0
∘
) as a function of altitude. IG-NFR measurements within either Uranus or Neptune’s atmospheres, using dedicated spectral filter bands will help derive radiative heating and cooling profiles, and will significantly contribute to our understanding of the planet’s atmospheric heat balance and structure, tropospheric 3-D flow, and compositions and opacities of the cloud layers. The IG-NFR uses an array of non-imaging Winston cones integrated to a matched thermopile detector Focal Plane Assembly (FPA), with individual bandpass filters, housed in a diamond windowed vacuum micro-vessel. The FPA thermopile detector signals are read out in parallel mode, amplified and processed by a multi-channel digitizer application specific integrated circuit (MCD ASIC) under field programmable gate array (FPGA) control. The vacuum micro-vessel rotates providing chopping between FOV’s of upward and downward radiation fluxes. This unique design allows for small net flux measurements in the presence of large ambient fluxes and rapidly changing ambient temperatures during the probe descent to
≥
10
bar pressure.</description><identifier>ISSN: 0038-6308</identifier><identifier>EISSN: 1572-9672</identifier><identifier>DOI: 10.1007/s11214-019-0630-x</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Aerospace Technology and Astronautics ; Ambient temperature ; Application specific integrated circuits ; Astrophysics and Astroparticles ; Band spectra ; Bandpass filters ; Cones ; Cutting ; Diamonds ; Digitization ; Field of view ; Field programmable gate arrays ; Fluctuations ; Fluxes ; Focal plane ; Heat balance ; Heating and cooling ; Ice giant planets ; In Situ Exploration of the Ice Giants: Science and Technology ; Integrated circuits ; Neptune ; Net radiation ; Physics ; Physics and Astronomy ; Planetology ; Radiation ; Radiation flux ; Radiative heating ; Signal processing ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Spectral bands ; Thermopiles ; Three dimensional flow ; Uranus atmosphere ; Vessels ; Wavelengths</subject><ispartof>Space science reviews, 2020-02, Vol.216 (1), Article 11</ispartof><rights>This is a U.S. government work and not under copyright protection in the U.S.; foreign copyright protection may apply 2020</rights><rights>Space Science Reviews is a copyright of Springer, (2020). All Rights Reserved.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c359t-721bf33942856b3b77d97d00d5622bd9a53e296537956e8d50641fba74c7123b3</citedby><cites>FETCH-LOGICAL-c359t-721bf33942856b3b77d97d00d5622bd9a53e296537956e8d50641fba74c7123b3</cites><orcidid>0000-0002-9581-647X</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s11214-019-0630-x$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s11214-019-0630-x$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,41488,42557,51319</link.rule.ids></links><search><creatorcontrib>Aslam, S.</creatorcontrib><creatorcontrib>Achterberg, R. K.</creatorcontrib><creatorcontrib>Calcutt, S. B.</creatorcontrib><creatorcontrib>Cottini, V.</creatorcontrib><creatorcontrib>Gorius, N. J.</creatorcontrib><creatorcontrib>Hewagama, T.</creatorcontrib><creatorcontrib>Irwin, P. G.</creatorcontrib><creatorcontrib>Nixon, C. A.</creatorcontrib><creatorcontrib>Quilligan, G.</creatorcontrib><creatorcontrib>Roos-Serote, M.</creatorcontrib><creatorcontrib>Simon, A. A.</creatorcontrib><creatorcontrib>Tran, D.</creatorcontrib><creatorcontrib>Villanueva, G.</creatorcontrib><title>Advanced Net Flux Radiometer for the Ice Giants</title><title>Space science reviews</title><addtitle>Space Sci Rev</addtitle><description>The design of an advanced Net Flux Radiometer (NFR), for inclusion as a payload on a future Ice Giants probe mission, is given. The Ice Giants NFR (IG-NFR) will measure the upward and downward radiation flux (hence net radiation flux), in seven spectral bands, spanning the range from solar to far infra-red wavelengths, each with a
5
∘
Field-Of-View (FOV) and in five sequential view angles (
±
80
∘
,
±
45
∘
, and
0
∘
) as a function of altitude. IG-NFR measurements within either Uranus or Neptune’s atmospheres, using dedicated spectral filter bands will help derive radiative heating and cooling profiles, and will significantly contribute to our understanding of the planet’s atmospheric heat balance and structure, tropospheric 3-D flow, and compositions and opacities of the cloud layers. The IG-NFR uses an array of non-imaging Winston cones integrated to a matched thermopile detector Focal Plane Assembly (FPA), with individual bandpass filters, housed in a diamond windowed vacuum micro-vessel. The FPA thermopile detector signals are read out in parallel mode, amplified and processed by a multi-channel digitizer application specific integrated circuit (MCD ASIC) under field programmable gate array (FPGA) control. The vacuum micro-vessel rotates providing chopping between FOV’s of upward and downward radiation fluxes. This unique design allows for small net flux measurements in the presence of large ambient fluxes and rapidly changing ambient temperatures during the probe descent to
≥
10
bar pressure.</description><subject>Aerospace Technology and Astronautics</subject><subject>Ambient temperature</subject><subject>Application specific integrated circuits</subject><subject>Astrophysics and Astroparticles</subject><subject>Band spectra</subject><subject>Bandpass filters</subject><subject>Cones</subject><subject>Cutting</subject><subject>Diamonds</subject><subject>Digitization</subject><subject>Field of view</subject><subject>Field programmable gate arrays</subject><subject>Fluctuations</subject><subject>Fluxes</subject><subject>Focal plane</subject><subject>Heat balance</subject><subject>Heating and cooling</subject><subject>Ice giant planets</subject><subject>In Situ Exploration of the Ice Giants: Science and Technology</subject><subject>Integrated circuits</subject><subject>Neptune</subject><subject>Net radiation</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Planetology</subject><subject>Radiation</subject><subject>Radiation flux</subject><subject>Radiative heating</subject><subject>Signal processing</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Spectral bands</subject><subject>Thermopiles</subject><subject>Three dimensional flow</subject><subject>Uranus atmosphere</subject><subject>Vessels</subject><subject>Wavelengths</subject><issn>0038-6308</issn><issn>1572-9672</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><recordid>eNp1kMFKAzEQhoMouFYfwFvAc-xMskk2x1JsLRQF0XPIbrK6pd2tyVbq27tlBU-e5jD_9w_zEXKLcI8AepoQOeYM0DBQAtjxjGQoNWdGaX5OMgBRsGFRXJKrlDYAJ0pnZDrzX66tgqdPoaeL7eFIX5xvul3oQ6R1F2n_EeiqCnTZuLZP1-SidtsUbn7nhLwtHl7nj2z9vFzNZ2tWCWl6pjmWtRAm54VUpSi19kZ7AC8V56U3TorAjZJCG6lC4SWoHOvS6bzSyEUpJuRu7N3H7vMQUm833SG2w0nLRZ4jCMRiSOGYqmKXUgy13cdm5-K3RbCnD-3oxQ5e7MmLPQ4MH5k0ZNv3EP-a_4d-ANgNYok</recordid><startdate>20200201</startdate><enddate>20200201</enddate><creator>Aslam, S.</creator><creator>Achterberg, R. 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K.</creatorcontrib><creatorcontrib>Calcutt, S. B.</creatorcontrib><creatorcontrib>Cottini, V.</creatorcontrib><creatorcontrib>Gorius, N. J.</creatorcontrib><creatorcontrib>Hewagama, T.</creatorcontrib><creatorcontrib>Irwin, P. G.</creatorcontrib><creatorcontrib>Nixon, C. A.</creatorcontrib><creatorcontrib>Quilligan, G.</creatorcontrib><creatorcontrib>Roos-Serote, M.</creatorcontrib><creatorcontrib>Simon, A. A.</creatorcontrib><creatorcontrib>Tran, D.</creatorcontrib><creatorcontrib>Villanueva, G.</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ProQuest Central Student</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Science Database</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central Basic</collection><jtitle>Space science reviews</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Aslam, S.</au><au>Achterberg, R. K.</au><au>Calcutt, S. B.</au><au>Cottini, V.</au><au>Gorius, N. J.</au><au>Hewagama, T.</au><au>Irwin, P. G.</au><au>Nixon, C. A.</au><au>Quilligan, G.</au><au>Roos-Serote, M.</au><au>Simon, A. A.</au><au>Tran, D.</au><au>Villanueva, G.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Advanced Net Flux Radiometer for the Ice Giants</atitle><jtitle>Space science reviews</jtitle><stitle>Space Sci Rev</stitle><date>2020-02-01</date><risdate>2020</risdate><volume>216</volume><issue>1</issue><artnum>11</artnum><issn>0038-6308</issn><eissn>1572-9672</eissn><abstract>The design of an advanced Net Flux Radiometer (NFR), for inclusion as a payload on a future Ice Giants probe mission, is given. The Ice Giants NFR (IG-NFR) will measure the upward and downward radiation flux (hence net radiation flux), in seven spectral bands, spanning the range from solar to far infra-red wavelengths, each with a
5
∘
Field-Of-View (FOV) and in five sequential view angles (
±
80
∘
,
±
45
∘
, and
0
∘
) as a function of altitude. IG-NFR measurements within either Uranus or Neptune’s atmospheres, using dedicated spectral filter bands will help derive radiative heating and cooling profiles, and will significantly contribute to our understanding of the planet’s atmospheric heat balance and structure, tropospheric 3-D flow, and compositions and opacities of the cloud layers. The IG-NFR uses an array of non-imaging Winston cones integrated to a matched thermopile detector Focal Plane Assembly (FPA), with individual bandpass filters, housed in a diamond windowed vacuum micro-vessel. The FPA thermopile detector signals are read out in parallel mode, amplified and processed by a multi-channel digitizer application specific integrated circuit (MCD ASIC) under field programmable gate array (FPGA) control. The vacuum micro-vessel rotates providing chopping between FOV’s of upward and downward radiation fluxes. This unique design allows for small net flux measurements in the presence of large ambient fluxes and rapidly changing ambient temperatures during the probe descent to
≥
10
bar pressure.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s11214-019-0630-x</doi><orcidid>https://orcid.org/0000-0002-9581-647X</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
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| ispartof | Space science reviews, 2020-02, Vol.216 (1), Article 11 |
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| language | eng |
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| source | SpringerLink Journals - AutoHoldings |
| subjects | Aerospace Technology and Astronautics Ambient temperature Application specific integrated circuits Astrophysics and Astroparticles Band spectra Bandpass filters Cones Cutting Diamonds Digitization Field of view Field programmable gate arrays Fluctuations Fluxes Focal plane Heat balance Heating and cooling Ice giant planets In Situ Exploration of the Ice Giants: Science and Technology Integrated circuits Neptune Net radiation Physics Physics and Astronomy Planetology Radiation Radiation flux Radiative heating Signal processing Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Spectral bands Thermopiles Three dimensional flow Uranus atmosphere Vessels Wavelengths |
| title | Advanced Net Flux Radiometer for the Ice Giants |
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