FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1684687525> ?p ?o ?g. }

• W1684687525 endingPage "n/a" @default.
• W1684687525 startingPage "n/a" @default.
• W1684687525 abstract "[1] In order to learn more about the Martian polar caps, it is important to compare and contrast the behavior of both frozen H2O and CO2 in different parts of the electromagnetic spectrum. Because relatively little attention has been given, thus far, to observing the seasonal Martian polar caps in the thermal microwave part of the spectrum, in this experiment, a 35-GHz handheld radiometer was used to measure the microwave emission and scattering from layers of manufactured CO2 (dry ice). Compared to natural snow crystals, results for the dry ice layers exhibit lower microwave brightness temperatures for similar thicknesses, regardless of the incidence angle of the radiometer. For example, at 50° H (horizontal polarization) and with a covering 18 cm of dry ice, the brightness temperature was 76 K. When the total thickness of the dry ice was 27 cm, the brightness temperature was 86 K. The lower brightness temperatures are due to a combination of the lower physical temperature and the larger crystal sizes of the commercial CO2 crystals compared to the snow crystals. While little is known about the CO2 and water snowpacks on Mars, it is likely that the particles are in close contact with one another as is the case for ice sheets on Earth – the grains are interconnected. This would qualify as a dense media. In densely packed media, the particles do not scatter independently; rather, they interact with other particles. Dense media calculations compare very favorably with the observed values from the handheld radiometer. The calculated versus observed TBs are within 10% for each case with the exception of the 26 cm layer thickness and the 0.8 mm particle size (15%) and for the 14 cm layer thickness and the 2.0 mm particle size (16%). Thus, it appears that dense media transfer modeling (DMRT) will be useful for modeling the flow of energy emerging from frozen CO2 deposits. Because the dry ice used in this experiment was manufactured in the shape of cylindrical pellets, an effort was made to see what effect, if any, the shape of the crystal, for different particle sizes, has on microwave scattering. Results from a discrete dipole scattering (DDSCAT) model show that differently shaped crystals, having the same effective radius of a sphere, give very similar cross section/efficiencies." @default.
• W1684687525 created "2016-06-24" @default.
• W1684687525 creator A5004085387 @default.
• W1684687525 creator A5036216612 @default.
• W1684687525 creator A5038130056 @default.
• W1684687525 creator A5057975787 @default.
• W1684687525 creator A5068791839 @default.
• W1684687525 creator A5068877892 @default.
• W1684687525 creator A5090757725 @default.
• W1684687525 date "2003-04-01" @default.
• W1684687525 modified "2023-09-27" @default.
• W1684687525 title "Thirty-five-gigahertz measurements of CO2crystals" @default.
• W1684687525 cites W1609005775 @default.
• W1684687525 cites W1966528118 @default.
• W1684687525 cites W1969939749 @default.
• W1684687525 cites W197033098 @default.
• W1684687525 cites W1978524841 @default.
• W1684687525 cites W2012605152 @default.
• W1684687525 cites W2015934482 @default.
• W1684687525 cites W2027900982 @default.
• W1684687525 cites W2039425928 @default.
• W1684687525 cites W2069456590 @default.
• W1684687525 cites W2069474014 @default.
• W1684687525 cites W2072552058 @default.
• W1684687525 cites W2093361212 @default.
• W1684687525 cites W2101412430 @default.
• W1684687525 cites W2105744076 @default.
• W1684687525 cites W2118235452 @default.
• W1684687525 cites W2123701839 @default.
• W1684687525 cites W2133089566 @default.
• W1684687525 cites W2162246342 @default.
• W1684687525 cites W2176461124 @default.
• W1684687525 cites W4232772892 @default.
• W1684687525 cites W4234155321 @default.
• W1684687525 cites W4250740991 @default.
• W1684687525 cites W59078114 @default.
• W1684687525 doi "https://doi.org/10.1029/2001rs002478" @default.
• W1684687525 hasPublicationYear "2003" @default.
• W1684687525 type Work @default.
• W1684687525 sameAs 1684687525 @default.
• W1684687525 citedByCount "0" @default.
• W1684687525 crossrefType "journal-article" @default.
• W1684687525 hasAuthorship W1684687525A5004085387 @default.
• W1684687525 hasAuthorship W1684687525A5036216612 @default.
• W1684687525 hasAuthorship W1684687525A5038130056 @default.
• W1684687525 hasAuthorship W1684687525A5057975787 @default.
• W1684687525 hasAuthorship W1684687525A5068791839 @default.
• W1684687525 hasAuthorship W1684687525A5068877892 @default.
• W1684687525 hasAuthorship W1684687525A5090757725 @default.
• W1684687525 hasConcept C120189094 @default.
• W1684687525 hasConcept C120665830 @default.
• W1684687525 hasConcept C121332964 @default.
• W1684687525 hasConcept C125245961 @default.
• W1684687525 hasConcept C125388846 @default.
• W1684687525 hasConcept C1276947 @default.
• W1684687525 hasConcept C153294291 @default.
• W1684687525 hasConcept C191486275 @default.
• W1684687525 hasConcept C192562407 @default.
• W1684687525 hasConcept C197046000 @default.
• W1684687525 hasConcept C2778600265 @default.
• W1684687525 hasConcept C29705727 @default.
• W1684687525 hasConcept C39432304 @default.
• W1684687525 hasConcept C44838205 @default.
• W1684687525 hasConcept C53802167 @default.
• W1684687525 hasConcept C62520636 @default.
• W1684687525 hasConcept C83260615 @default.
• W1684687525 hasConcept C87355193 @default.
• W1684687525 hasConcept C91586092 @default.
• W1684687525 hasConcept C96960616 @default.
• W1684687525 hasConceptScore W1684687525C120189094 @default.
• W1684687525 hasConceptScore W1684687525C120665830 @default.
• W1684687525 hasConceptScore W1684687525C121332964 @default.
• W1684687525 hasConceptScore W1684687525C125245961 @default.
• W1684687525 hasConceptScore W1684687525C125388846 @default.
• W1684687525 hasConceptScore W1684687525C1276947 @default.
• W1684687525 hasConceptScore W1684687525C153294291 @default.
• W1684687525 hasConceptScore W1684687525C191486275 @default.
• W1684687525 hasConceptScore W1684687525C192562407 @default.
• W1684687525 hasConceptScore W1684687525C197046000 @default.
• W1684687525 hasConceptScore W1684687525C2778600265 @default.
• W1684687525 hasConceptScore W1684687525C29705727 @default.
• W1684687525 hasConceptScore W1684687525C39432304 @default.
• W1684687525 hasConceptScore W1684687525C44838205 @default.
• W1684687525 hasConceptScore W1684687525C53802167 @default.
• W1684687525 hasConceptScore W1684687525C62520636 @default.
• W1684687525 hasConceptScore W1684687525C83260615 @default.
• W1684687525 hasConceptScore W1684687525C87355193 @default.
• W1684687525 hasConceptScore W1684687525C91586092 @default.
• W1684687525 hasConceptScore W1684687525C96960616 @default.
• W1684687525 hasIssue "2" @default.
• W1684687525 hasLocation W16846875251 @default.
• W1684687525 hasOpenAccess W1684687525 @default.
• W1684687525 hasPrimaryLocation W16846875251 @default.
• W1684687525 hasRelatedWork W1135390322 @default.
• W1684687525 hasRelatedWork W1618392062 @default.
• W1684687525 hasRelatedWork W1969786533 @default.
• W1684687525 hasRelatedWork W1978485516 @default.
• W1684687525 hasRelatedWork W2011205060 @default.

• next