Matches in SemOpenAlex for { <https://semopenalex.org/work/W2902292188> ?p ?o ?g. }
- W2902292188 endingPage "20" @default.
- W2902292188 startingPage "10" @default.
- W2902292188 abstract "Although a substantial ice cover has been identified within the mid-latitudes of Mars, there is uncertainty regarding the formation, current and former volume, and dynamic evolution of these ice masses. Here, we present the first comprehensive ice volume estimate of martian glacier-like forms (GLFs) from systematic population scale mapping and volumetric analysis. The outlines of 1243 GLFs were manually delineated from 6 m per pixel Context Camera (CTX) images and the volume of each determined using a volume–area scaling approach. Our results show that GLFs cover a surface area of 11344 ± 393 km2 and have a total volume of 1744 ± 441 km3. Using two end-member scenarios for ice concentration by volume of 30% (pore ice) and 90% (debris-covered glacier ice), we calculate the volume of ice contained within GLFs to be between 523 ± 132 km3 (480 ± 121 Gt) and 1570 ± 397 km3 (1439 ± 364 Gt), equivalent to a mean global water layer 3 to 10 mm thick. We investigate the local topographic setting of each GLF by reference to the Mars Orbiter Laser Altimeter (MOLA) digital elevation model. Our analysis reveals that globally GLFs are on average larger in latitudes >36° and on slopes between 2 and 8°. In the northern hemisphere GLFs between 500 and 2500 m in elevation and in the southern hemisphere GLFs with a northern aspect are also larger on average. The observed spatial patterns of GLF landform and volume distribution suggests that regional to local meteorological and topographical conditions play an important role in GLF ice accumulation and/or preservation. Assuming a net accumulation rate of 10 mm a−1 typical of climatic excursions with high obliquity, we estimate a period of at least 13 ka is required to yield the average calculated GLF ice thickness of ∼130 m. Such a period is well within the timeframe of a high obliquity cycle (20–40 ka), suggesting that the current GLF volume could have formed during a single climate excursion." @default.
- W2902292188 created "2018-12-11" @default.
- W2902292188 creator A5031102264 @default.
- W2902292188 creator A5032634179 @default.
- W2902292188 creator A5079554586 @default.
- W2902292188 date "2019-02-01" @default.
- W2902292188 modified "2023-09-26" @default.
- W2902292188 title "Area and volume of mid-latitude glacier-like forms on Mars" @default.
- W2902292188 cites W1498786100 @default.
- W2902292188 cites W1502127694 @default.
- W2902292188 cites W1865568237 @default.
- W2902292188 cites W1901583545 @default.
- W2902292188 cites W1960598803 @default.
- W2902292188 cites W1967750735 @default.
- W2902292188 cites W1973822498 @default.
- W2902292188 cites W1982531131 @default.
- W2902292188 cites W1982776499 @default.
- W2902292188 cites W1983550241 @default.
- W2902292188 cites W1986618533 @default.
- W2902292188 cites W1992145662 @default.
- W2902292188 cites W1997213796 @default.
- W2902292188 cites W1998780374 @default.
- W2902292188 cites W2011515733 @default.
- W2902292188 cites W2028924837 @default.
- W2902292188 cites W2032600327 @default.
- W2902292188 cites W2042405928 @default.
- W2902292188 cites W2045323482 @default.
- W2902292188 cites W2056216751 @default.
- W2902292188 cites W2059288596 @default.
- W2902292188 cites W2060984454 @default.
- W2902292188 cites W2063530398 @default.
- W2902292188 cites W2068619219 @default.
- W2902292188 cites W2070529447 @default.
- W2902292188 cites W2083596540 @default.
- W2902292188 cites W2094459693 @default.
- W2902292188 cites W2100957654 @default.
- W2902292188 cites W2107462639 @default.
- W2902292188 cites W2109258549 @default.
- W2902292188 cites W2120077698 @default.
- W2902292188 cites W2124919065 @default.
- W2902292188 cites W2127408714 @default.
- W2902292188 cites W2131803542 @default.
- W2902292188 cites W2139407666 @default.
- W2902292188 cites W2142755971 @default.
- W2902292188 cites W2146528866 @default.
- W2902292188 cites W2151346430 @default.
- W2902292188 cites W2152597400 @default.
- W2902292188 cites W2166364033 @default.
- W2902292188 cites W2166808849 @default.
- W2902292188 cites W2168601869 @default.
- W2902292188 cites W2273628640 @default.
- W2902292188 cites W2301318036 @default.
- W2902292188 cites W2332696172 @default.
- W2902292188 cites W2334239165 @default.
- W2902292188 cites W2341582552 @default.
- W2902292188 cites W2557438774 @default.
- W2902292188 cites W2586443905 @default.
- W2902292188 cites W4377077305 @default.
- W2902292188 doi "https://doi.org/10.1016/j.epsl.2018.11.031" @default.
- W2902292188 hasPublicationYear "2019" @default.
- W2902292188 type Work @default.
- W2902292188 sameAs 2902292188 @default.
- W2902292188 citedByCount "15" @default.
- W2902292188 countsByYear W29022921882020 @default.
- W2902292188 countsByYear W29022921882021 @default.
- W2902292188 countsByYear W29022921882022 @default.
- W2902292188 countsByYear W29022921882023 @default.
- W2902292188 crossrefType "journal-article" @default.
- W2902292188 hasAuthorship W2902292188A5031102264 @default.
- W2902292188 hasAuthorship W2902292188A5032634179 @default.
- W2902292188 hasAuthorship W2902292188A5079554586 @default.
- W2902292188 hasBestOaLocation W29022921882 @default.
- W2902292188 hasConcept C100834320 @default.
- W2902292188 hasConcept C100970517 @default.
- W2902292188 hasConcept C114793014 @default.
- W2902292188 hasConcept C121332964 @default.
- W2902292188 hasConcept C122523270 @default.
- W2902292188 hasConcept C127313418 @default.
- W2902292188 hasConcept C1276947 @default.
- W2902292188 hasConcept C13280743 @default.
- W2902292188 hasConcept C181843262 @default.
- W2902292188 hasConcept C20556612 @default.
- W2902292188 hasConcept C205649164 @default.
- W2902292188 hasConcept C2524010 @default.
- W2902292188 hasConcept C2778835443 @default.
- W2902292188 hasConcept C33923547 @default.
- W2902292188 hasConcept C37054046 @default.
- W2902292188 hasConcept C39432304 @default.
- W2902292188 hasConcept C49204034 @default.
- W2902292188 hasConcept C62520636 @default.
- W2902292188 hasConcept C62649853 @default.
- W2902292188 hasConcept C83260615 @default.
- W2902292188 hasConceptScore W2902292188C100834320 @default.
- W2902292188 hasConceptScore W2902292188C100970517 @default.
- W2902292188 hasConceptScore W2902292188C114793014 @default.
- W2902292188 hasConceptScore W2902292188C121332964 @default.
- W2902292188 hasConceptScore W2902292188C122523270 @default.
- W2902292188 hasConceptScore W2902292188C127313418 @default.