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Record #173446:

Evolution of the Martian climate: effects of the ice sheets / Takasumi Kurahashi-Nakamura, Eiicha Tajika.

Title: Evolution of the Martian climate: effects of the ice sheets / Takasumi Kurahashi-Nakamura, Eiicha Tajika.
Author(s): Kurahashi-Nakamura, Takasumi.
Tajika, Eiicha.
Date: 2005.
Language: Japanese.
In: Seppyo : Journal of the Japanese Society of Snow and Ice. (2005.), Vol. 67(2) (2005)
Abstract: Presents numerical study suggesting permanent CO₂ ice caps played important role in evolution of Mars from warm climate with dense CO₂ atmosphere to present cold climate. Suggests instability of CO₂ system, triggered by impact erosion and/or sputtering of atmosphere, caused runaway condensation of dense CO₂ atmosphere to form large polar caps. Investigation with ice sheet model suggests temperature at bottom of CO₂ ice caps would exceed melting point due to geothermal heat flux. Gaseous or liquid CO₂ produced by basal melting might have permeated and diffused into subsurface through Martian crust. CO₂ removed from surface may presently exist in Martian subsurface as clathrate, carbonate, and/or liquid and gaseous phases.
Notes:

Seppyo : Journal of the Japanese Society of Snow and Ice. Vol. 67(2) :133-145 (2005).

English abstract.

Keywords: 551.32 -- Glaciology.
551.58 -- Climatology.
523.43 -- Mars.
52 -- Astronomy.
551.582 -- Climatology of particular places.
546.264-31 -- Carbon dioxide.
551.324.24 -- Ice sheets and caps.
551.510.4 -- Atmosphere, composition.
536 -- Heat.
548.736.65 -- Clathrate hydrates.
536.421.1 -- Melting.
551.336 -- Ice ages.
519.673 -- Modelling.
E13 -- Glaciology: glacioastronomy.
SPRI record no.: 173446

MARCXML

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100 1# ‡aKurahashi-Nakamura, Takasumi.
245 10 ‡aEvolution of the Martian climate :‡beffects of the ice sheets /‡cTakasumi Kurahashi-Nakamura, Eiicha Tajika.
260 ## ‡a[S.l.] :‡b[s.n.],‡c2005.
300 ## ‡ap. 133-145 :‡bill., diags.
500 ## ‡aSeppyo : Journal of the Japanese Society of Snow and Ice. Vol. 67(2) :133-145 (2005).
500 ## ‡aEnglish abstract.
520 3# ‡aPresents numerical study suggesting permanent CO₂ ice caps played important role in evolution of Mars from warm climate with dense CO₂ atmosphere to present cold climate. Suggests instability of CO₂ system, triggered by impact erosion and/or sputtering of atmosphere, caused runaway condensation of dense CO₂ atmosphere to form large polar caps. Investigation with ice sheet model suggests temperature at bottom of CO₂ ice caps would exceed melting point due to geothermal heat flux. Gaseous or liquid CO₂ produced by basal melting might have permeated and diffused into subsurface through Martian crust. CO₂ removed from surface may presently exist in Martian subsurface as clathrate, carbonate, and/or liquid and gaseous phases.
546 ## ‡aIn Japanese.
650 07 ‡a551.32 -- Glaciology.‡2udc
650 07 ‡a551.58 -- Climatology.‡2udc
650 07 ‡a523.43 -- Mars.‡2udc
650 07 ‡a52 -- Astronomy.‡2udc
650 07 ‡a551.582 -- Climatology of particular places.‡2udc
650 07 ‡a546.264-31 -- Carbon dioxide.‡2udc
650 07 ‡a551.324.24 -- Ice sheets and caps.‡2udc
650 07 ‡a551.510.4 -- Atmosphere, composition.‡2udc
650 07 ‡a536 -- Heat.‡2udc
650 07 ‡a548.736.65 -- Clathrate hydrates.‡2udc
650 07 ‡a536.421.1 -- Melting.‡2udc
650 07 ‡a551.336 -- Ice ages.‡2udc
650 07 ‡a519.673 -- Modelling.‡2udc
650 07 ‡aE13 -- Glaciology: glacioastronomy.‡2local
700 1# ‡aTajika, Eiicha.
773 0# ‡7nnas ‡tSeppyo : Journal of the Japanese Society of Snow and Ice. ‡gVol. 67(2) (2005) ‡wSPRI-17791
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917 ## ‡aUnenhanced record from Muscat, imported 2019
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