the global martian volcanic evolutionary history abstract viking mission image data revealed the total spatial extent of preserved volcanic surface on mars one of the dominating surface expressions is olympus mons and the surrounding volcanic province tharsis earlier studies of the global volcanic sequence of events based on stratigraphic relationships and crater count statistics were limited to the image resolution of the viking orbiter camera here a global investigation based on high resolution image data gathered by the high resolution stereo camera hrsc during the first years of mars express orbiting around mars is presented additionally mars orbiter camera moc and thermal emission imaging system themis images were used for more detailed and complementary information the results reveal global volcanism during the noachian period 3 7 ga followed by more focused vent volcanism in three tharsis elysium and circum hellas and later two tharsis and elysium volcanic provinces finally the volcanic activity became localized to the tharsis region about 1 6 ga ago where volcanism was active until very recently 200 100 ma these age results were expected from radiometric dating of martian meteorites but now verified for extended geological units mainly found in the tharsis montes surroundings showing prolonged volcanism for more than 3 5 billions years the volcanic activity on mars appears episodic but decaying in intensity and localizing in space the spatial and temporal extent of martian volcanism based on crater count statistics now provides a much better database for modelling the thermodynamic evolution of mars

further evidence for a mass movement origin of the olympus mons aureole analysis of the ridge graben and fracture patterns on the aureole material surrounding olympus mons lends further support to an origin by gravity sliding of the outer flanks of the shield the patterns provide evidence of the nature of sliding especially in the last stages of emplacement no part of the slide need have traveled the whole extent of the aureole for the slides to occur on a shallow slope reduction of shear strength of the materials involved is required possibly by melting of ground ice triggering mechanisms could be volcanically related marsquakes and possibly stresses induced on the surrounding area by the growing olympus mons volcano

planetary waves and variability of the semidiurnal tide in the mesosphere and lower thermosphere over esrange 68 n 21 e during winter 1 the main features of the planetary waves and the variability of the semidiurnal tide with planetary wave periods observed by meteor radar over esrange 68 n 21 e have been investigated the interval of 39 months covering continuous measurements from october 1999 to december 2002 has been examined the planetary waves most frequently observed by meteor radar measurements in the mesosphere and lower thermosphere 80 100 km over esrange are 5 8 to 10 16 and 23 day waves the quasi 2 day wave is excluded in this study they are strongly amplified in the winter some differences between high and middle latitude planetary waves notwithstanding the 5 10 and 16 day waves are most probably related to the well known normal mode there are some reasons to believe that the vertically upward propagating 23 day wave could be generated by solar forcing the variability of the semidiurnal tide with periods of planetary waves has been thoroughly studied as well it is found that in the winter when the planetary waves are significantly amplified a very strong periodic variability of the semidiurnal tide is observed as well this result indicates that the most probable mechanism responsible for the periodic tidal variability during winter is in situ nonlinear coupling between tides and planetary waves two winter periods have been examined 1999 2000 and 2001 2002 in order to find strong evidence supporting this suggestion the validity of the frequency phase and vertical wavenumber wavelength relationship between the prime the planetary wave and semidiurnal tide and secondary waves has been established the novel aspect of this work is that we show for the first time that the calculated vertical structures vertical wavelengths of the sum and difference secondary waves which have very close periods are actually very different

the acheron dorsum on mars a novel interpretation of its linear depressions and a model for its evolution abstract the acheron dorsum north of olympus mons on mars is a unique 800 km long arcuate ridge apparently unrelated to other adjacent morphologies acheron dorsum is crossed by deep and wide fractures fossae here referred to also as linear depressions or lds commonly interpreted as grabens formed by local lithosphere stress in response to endogenous mantle upwelling we suggest an alternate view that the linear depressions may result from gravitational self adjustment of a loose deposit similar to the deep seated gravitational slope deformations dsgsd or sackung a kind of slow mass movement well documented on earth numerical simulations based on a finite difference numerical model devised for terrestrial dsgsds reproduce the timing and position of lds reasonably well provided that the viscosity of the viscoplastic layer is between 7 10 15 and 10 17 pa s while rock masses typically exhibit much higher values based on comparison with glacial examples we find that these viscosities could be compatible to a rock ice mixture this leads to the hypothesis that the rock underneath acheron dorsum may be highly fragmented and that ice might have been involved in its deformation our hypothesis could shed light on the puzzling stress pattern on acheron dorsum which follows approximately the ridge without requiring the presence of hypothetical small scale endogenous currents

the influence of closed brine pockets and permeable brine channels on the thermo elastic properties of saline ice a model of the thermo elastic behaviour of saline ice is formulated and model solutions describing thermo elastic waves tew propagating into a half space of the ice are investigated the model is based on a proposal that saline ice is a matrix which encompasses both closed brine pockets and permeable channels filled with brine experiments on the thermal expansion of saline ice samples and on tew in saline ice have been performed in the cold laboratories of the university centre in svalbard and in university college london the experimental data are compared with theoretical conclusions the experimental data support our hypothesis that the brine in saline ice is divided between closed pockets and open permeable channels this article is part of the themed issue microdynamics of ice

variabilities of low latitude migrating and nonmigrating tides in gps tec and timed saber temperature during the sudden stratospheric warming event of 2013 the global positioning system gps deduced total electron content tec data at 15 n geomagnetic which is the crest region of equatorial ionization anomaly are used to study tidal variabilities during the 2013 sudden stratospheric warming ssw event the results from space time spectral analysis reveal that the amplitudes of migrating diurnal dw1 and semi diurnal sw2 tides are larger than those of non migrating tides after the ssw onset the amplitudes of dw1 sw2 sw1 and ds0 increase moreover they show 16 day variations similar to the periodicity of the high latitude stratospheric planetary wave pw suggesting that the non migrating tides sw1 and ds0 are possibly generated due to non linear interaction of migrating tides with pw similar spectral analysis on temperature at 10 n obtained from the sounding of atmosphere by broadband emission radiometry saber shows that the sw2 enhances at stratospheric heights and the sw2 is more dominant at 80 90 km but its amplitude decreases around 100 km the amplitudes of non migrating tides become comparable to those of sw2 around 100 km and their contribution become increasingly important at higher heights this suggests that the non linear interaction between migrating tides and pw occur at low latitude upper mesospheric heights as sw2 exhibits 16 day periodicity in saber temperature at 100 km as observed in tec besides it is observed that the eastward propagating tides are less dominant than westward propagating tides in both tec and saber temperature

topography of the shield volcano olympus mons on mars olympus mons one of the largest known shield volcanoes in the solar system covers an area of 3 2 105 km2and has a diameter of 600 km excluding its vast aureole deposits the structure is five times larger than the largest shield volcano on the earth it is situated on the north west flank of the tharsis volcanic region a broad topographic rise on the martian surface the volcano has three physical subdivisions the summit caldera the terraced upper flanks and the lower flanks which terminate in a scarp 2 10 km high that nearly surrounds the structure a large block of images of the tharsis region including olympus mons was obtained by the viking mission1 here we present a topographic map of olympus mons compiled using various combinations of stereo pairs of these images together with stereoscopic perspective views generated by image processing techniques

thermo mechanical loads of confined sea ice on structures records of the ice pressures on the joggle skirt of the coal quay in spitsbergen were performed over winter seasons in 2013 and 2015 the ice thickness below the quay was above 2m ice temperature

tank study of physico chemical controls on gas content and composition during growth of young sea ice during an ice tank experiment samples were taken to study the processes of acquisition and alteration of the gas properties in young first year sea ice during a complete growth warming cooling cycle the goal was to obtain reference levels for total gas content and concentrations of atmospheric gases o2 n2 co2 in the absence of significant biological activity the range of total gas content values obtained 3 5 to 18 ml of gas per kilo of ice was similar to previous measurements or estimates however major differences occurred between the current and quiet basins showing the role of water dynamics at the ice water interface in controlling bubble nucleation processes extremely high co2 concentrations were observed in all the experiments up to 57 in volume parts it is argued that these could have resulted from two unexpected biases in the experimental settings concentrations of bubbles nucleated at the interface are controlled by diffusion both from the ice water interface towards the well mixed reservoir and between the interface water and the bubble itself this double kinetic effect results in a transition of the gas composition in the bubbles from values close to solubility in sea water towards values close to atmospheric as the ice cover builds up

high latitude mesospheric mean winds a comparison between tromso 69 n and svalbard 78 n 1 daily mean winds in the upper mesosphere regions above tromso 69 n 19 e and svalbard 78 n 16 e are presented these having been obtained from 6 years operation of the middle frequency radar at tromso and almost 2 years operation of the svalbard meteor radar the findings depart somewhat from the predictions of current modeling particularly in that outflow from the pole occurs almost all year round this picture is in accordance with a ferrell cell circulation in summer but not in winter gravity wave drag parameterized by the rayleigh drag coefficient is suggested as a likely cause of the widespread ageostrophic motion characterizing the winter dynamics

equations for determining the gas and brine volumes in sea ice samples on a etabli des equations utilisables pour determiner le taux de gaz inclus dans la glace de mer a partir de mesures de densite de salinite et de temperature dans des gammes de temperatures entre 2 c et 30 c inversement ces relations peuvent etre utilisees pour calculer la densite de la glace de mer en fonction de la temperature et de la salinite en prenant en compte a la fois la presence de gaz et de cristaux de sel dans la glace on donne aussi des equations qui permettent le calcul du volume de gaz et d eau salee dans la glace a des temperatures autres que celle pour laquelle la densite a ete determinee

the 8 hour tide in the arctic mesosphere and lower thermosphere an all sky vhf meteor radar at esrange 68 n 21 e near kiruna in northern sweden has been used to investigate the 8 hour tide in the arctic mesosphere and lower thermosphere we present a climatology of the 8 hour tide over the period october 1999 to april 2001 the tide appears to be a persistent feature of the arctic atmosphere although a large day to day variability of the tidal amplitude is observed at times the 8 hour tide reaches amplitudes over 30 m s 1 the amplitude of the tide increases with height across the observed height range of 80 100 km monthly mean tidal amplitudes range from 2 m s 1 to values as large as 10 m s 1 a clear seasonal behavior is apparent with maximum amplitudes observed in the autumn vertical wavelengths are shortest in winter and spring 25 35 km and longest in summer and autumn 50 90 km at least on some occasions the vertical wave number relationships between the 8 12 and 24 hour tides suggest that the 8 hour tide is being generated by nonlinear interaction between the 12 and 24 hour tides

mean winds and tides in the arctic mesosphere and lower thermosphere 1 a new meteor radar has been deployed at esrange 68 n 21 e near kiruna in sweden the radar has been used to measure winds and tides in the arctic mesosphere lower thermosphere region over the interval august 1999 to july 2000 conspicuous features of the measured mean winds include a strong shear of up to 5 m s 1 km 1 in the summer zonal flow resulting in eastward flows of in excess of 30 m s 1 at the upper heights observed 97 km an equatorward meridional flow is observed in summer and winter which reaches maximum values of 13 m s 1 in a summer jet poleward flow in comparison is weak and only occurs at the equinoxes the monthly mean and seasonal mean behaviors of the amplitudes and phases of the 12 and 24 hour tides are examined and compared to the global scale wave model 98 the observations are generally very close to the model predictions for the 24 hour tide and for the 12 hour tide in winter in other seasons particularly summer the observed 12 hour tidal amplitudes are significantly larger than those predicted in spring and summer the wavelength of the 12 hour tide is significantly larger than that predicted

modeling the salinity profile of undeformed arctic sea ice the salinity of sea ice affects its physical and ecological properties here a multilayer one dimensional halo thermodynamic sea ice model is used to simulate the vertical salinity profile of undeformed arctic sea ice the model successfully reproduces the desalination pattern observed in first year fy and multi year my ice the model can also be integrated with a prescribed time independent salinity profile substantial differences in the simulated mass balance and ice ocean salt flux arise depending on the salinity after 10 years into the simulation the annual mean ice thickness is 2 85 m with the interactive halodynamic component compared to 2 53 m 2 29 m with a prescribed time independent vertically varying constant salinity profile modelling sea ice salinity is especially important when sea ice is transitioning from a my to fy ice regime thus including a halodynamic component in sea ice models would significantly improve simulations of future climate

observations of brine drainage networks and microstructure of first year sea ice brine drainage networks and the microstructure of first year sea ice have been examined at two locations near barrow northern alaska a method for obtaining full depth sections of ice sheets up to 1 8 m thick is presented and shown to provide information on the spatial distribution and geometry of brine drainage networks on a scale of meters a number of such sections from the two test sites are presented which reveal a greater variety of main channel and side branch configurations than is typically observed in ice grown in the laboratory vertical and horizontal micrographs and thin section photographs were obtained in november 1993 and march and may 1994 at a test site in the relatively protected elson lagoon the resulting time series of photographic records provide detailed information on the size shape and spatial distribution of the brine and gas filled inclusions and a means to quantify their size and shape changes with time an example of the changes with time in inclusion sizes and aspect ratios in the vertical and horizontal directions for a depth of 0 2 m with a given thermal history is also presented

nonmigrating semidiurnal tide over the arctic determined from timed doppler interferometer wind observations received 25 june 2009 revised 30 october 2009 accepted 5 november 2009 published 30 march 2010 1 the timed doppler interferometer tidi on the nasa thermosphere ionosphere mesosphere energetics and dynamics timed satellite has been measuring horizontal winds in the mesosphere and lower thermosphere mlt since 2002 because of the high inclination of the timed orbit tidi measures the horizontal winds from pole to pole every orbit this paper presents the first assessment of the spatial structure and temporal evolution of the nonmigrating semidiurnal tides over the arctic determined from the tidi wind measurements and a comparison of the structure of the nonmigrating semidiurnal tide between the arctic and antarctic the nonmigrating semidiurnal tides were determined as a 60 day average based on the yaw cycles of the spacecraft the nonmigrating semidiurnal tidal wind field over the arctic comprises mainly the westward propagating zonal wave numbers1 w1 and3 w3 andstandingzonalwavenumber0 s0 modes thew1modeis the most prominent maximizing above 90 km poleward of 60 n during the yaw interval ranging from mid march to mid may while this mode exhibits a slight amplitude increase toward the north pole during this interval its phase is nearly constant with latitude the s0 mode is enhanced over two yaw intervals ranging from mid january to mid may but its amplitude decreases toward the north pole compared to the w1 semidiurnal tide over the antarctic that over the arctic is smaller in amplitude of less extended duration achieves maximum amplitudes at higher altitudes by 10 km and exhibits a weaker amplitude increase toward the pole these differences likely result from differences in excitation mechanisms and efficiency and or in propagation conditions in the two responses for the nonmigrating semidiurnal tides between the arctic and antarctic

chronology eruption duration and atmospheric contribution of the martian volcano apollinaris patera geologic mapping thermal inertia measurements and an analysis of the color visual wavelengths of the martian volcano apollinaris patera indicate the existence of two different surface materials comprising an early easily eroded edifice and a more recent competent fan on the southern flank a chronology of six major events that is consistent with the present morphology of the volcano has been identified we propose that large scale explosive activity occurred during the formation of the main edifice and that the distinctive fan on the southern flank appears to have been formed by lavas of low eruptive rate similar to those that form compound pahoehoe flow fields on earth a basal escarpment typically 500 m in relief and morphologically similar to the one surrounding olympus mons was produced between the formation of the main edifice and the fan indicating multistage eruptions over a protracted period of time contact relations between the volcanic units and the adjacent chaotic material indicate that formation of the chaotic material occurred over an extended period of time and may be related to the volcanic activity that formed apollinaris patera stereophotogrammetric measurements permit the volume of the volcano to be estimated at 105 km3 from this volume measurement and an inferred eruption rate 1 5 10 2 km3 yr 1 we estimate the total eruption duration for the main edifice to be 107 yrs plausible estimates of the exsolved volatile content of the parent magma imply that greater than 1015 kg of water vapor was released into the atmosphere as a consequence of this activity this large amount of water vapor as well as other exsolved gases must have had a significant impact on local and possibly global climatic conditions

fault propagation folds induced by gravitational failure and slumping of the central costa rica volcanic range implications for large terrestrial and martian volcanic edifices long sublinear ridges and related scarps located at the base of large volcanic structures are frequently interpreted as normal faults associated with extensional regional stress in contrast the ridges bordering the central costa rica volcanic range ccrvr are the topographic expression of hanging wall asymmetric angular anticlines overlying low angle thrust faults at the base of the range these faults formed by gravitational failure and slumping of the flanks of the range due to the weight of the volcanic edifices and were perhaps triggered by the intrusion of magma over the past 20 000 years the thrust fault underlying alajuela ridge rises from a depth of 700 m at a dip of 15 over a distance of a few kilometers it ramps up at 600 m depth on a 40 slope and terminates in the axis of the forward syncline 400 m below the surface the hanging wall of this fault has been thrusted about 200 m away from the volcanic range axis thrusting on the lower flanks of the ccrvr is compensated by extension on the range axis with formation of summit grabens shallow seismicity in the volcanic range suggests that thrusting is still active we postulate that at kilauea volcano hawaii the gravity and magma induced slumping of the southern flank on low angle thrust faults generates hanging wall anticlines similar to those observed in costa rica these anticlines are hypothesized to occur along the base of the volcano where the thrust faults ramp up toward the sea bottom ridges and scarps between 2000 and 5000 m below sea level are interpreted as the topographic expression of these folds we further suggest that the scarps of the ccrvr and kilauea are valid scaled terrestrial analogs of the perimeter scarp of the martian volcano olympus mons we suggest that the crust below olympus mons has failed under the load of the volcano triggering the radial slumping of the flanks of the volcano on basal thrusts the thrusting would have in turn formed the anticlinal ridges and scarps that surround the edifice the thrusting seems to be preferential toward the northwest and southeast and a northeast southwest rift zone seems to have developed perpendicular to the regional topographic gradient the thrust faults may extend all the way to the base of the martian crust about 40 km and they may have been active until almost the end of the volcanic activity we suggest that gravitational failure and slumping of the flanks of volcanoes is a process common to most large volcanic edifices in the ccrvr and at kilauea this slumping of the flanks is a slow intermittent process but it could evolve to rapid massive avalanching leading to catastrophic eruptions thus monitoring of uplift and displacement of the folds related to the slump tectonics could become an additional effective method for mitigating volcanic hazards

a link between variability of the semidiurnal tide and planetary waves in the opposite hemisphere 1 horizontal wind observations over four years from the meteor radar at esrange 68 n 21 e are analyzed to determine the variability of the semidiurnal tide simultaneous global observations of temperature and geopotential from the saber satellite instrument are used to construct time series of planetary wave amplitudes and geostrophic mean zonal wind during northern hemisphere summer and fall the temporal variability of the semidiurnal tide at esrange is found to be well correlated with the amplitude of planetary wavenumber 1 in the stratosphere in high southern latitudes i e in the opposite hemisphere the correlations indicate that a significant part of the tidal variation at esrange is due to dynamical interactions in the southern hemisphere a corresponding robust correlation pattern for the esrange tides is not apparent at other times of the multiple years analyzed

the character of polar tidal signatures in the extended canadian middle atmosphere model the characteristics of the diurnal semidiurnal and terdiurnal tides zonal wave numbers 5 to 5 in temperature and zonal wind in the polar mesosphere and lower thermosphere region as simulated by the extended canadian middle atmosphere model are examined the most significant diurnal semidiurnal and terdiurnal tides in the polar regions are ds0 dw1 and de1 sw3 sw2 sw1 ss0 se1 and se2 and tw3 ts0 and tw1 respectively and their latitudinal structures seasonal variations and hemispheric asymmetries noted of these components ds0 tw1 ts0 and tw3 exhibit a seasonally symmetric variation with both hemispheres strengthening simultaneously on the other hand dw1 strengthens asymmetrically so that when one hemisphere is strong the other is weak the remainder show no seasonal tendency but vacillate on shorter than seasonal time scales in a symmetric or antisymmetric manner at different times of the year global scale correlations of the amplitudes of the migrating tides dw1 sw2 and the stationary planetary wave 1 and the assumed child nonmigrating tides are also examined the results indicate that the correlations are highly time scale dependent and the significant correlations seen with the original time series are mainly due to longer term variations 18 days there are no consistent global correlations associated with the short term variations 18 days among these waves

large scale waves in the mesosphere and lower thermosphere observed by saber observations made by the sounding of the atmosphere using broadband emission radiometry saber instrument on board nasa s thermosphere ionosphere mesosphere energetics and dynamics timed satellite have been processed using salby s fast fourier synoptic mapping ffsm algorithm the mapped data provide a first synoptic look at the mean structure and traveling waves of the mesosphere and lower thermosphere mlt since the launch of the timed satellite in december 2001 the results show the presence of various wave modes in the mlt which reach largest amplitude above the mesopause and include kelvin and rossby gravity waves eastward propagating diurnal oscillations non sunsynchronous tides and a set of quasi normal modes associated with the so called 2 day wave the latter exhibits marked seasonal variability attaining large amplitudes during the solstices and all but disappearing at the equinoxes saber data also show a strong quasi stationary rossby wave signal throughout the middle atmosphere of the winter hemisphere the signal extends into the tropics and even into the summer hemisphere in the mlt suggesting ducting by westerly background zonal winds at certain times of the year the 5 day rossby normal mode and the 4 day wave associated with instability of the polar night jet are also prominent in saber data

lithospheric flexure and gravity spreading of olympus mons volcano mars the structural architecture of large volcanoes is governed substantially by gravity driven deformation that is manifest as distinct processes such as basement flexure or volcanic spreading temporal effects and the mutual interplay of these processes have been investigated only to a limited extent and so we present novel numerical models of the time dependent deformation associated with them the models simulate the combined effects of lithospheric flexure and volcanic spreading during growth increments of an elastoplastic volcanic cone different spreading scenarios are considered by a variable coupling decoupling behavior at the interface between volcano and basement we apply our models to olympus mons on mars which is characterized by upper to middle flank terraces on the shield is encircled by a basal scarp that has an average slope of 30 and is surrounded by distant deposits that resemble large scale slumping features on earth our results are consistent with the interpretation that terraces on olympus mons flanks form by thrust faulting that results from lithospheric flexure the presence and expression of terraces depend on the coupling of volcano and basement on the time of volcano growth relative to mantle relaxation and on the cohesion of the edifice the encircling scarp may be related to a very low friction detachment at the edifice base which leads to a normal fault regime on the lowermost flanks with time and volcano growth predicted stress and faulting regimes migrate only slightly indicating that the structural architecture of volcanoes is largely set in the very early stages of formation

diurnal variation of gravity wave momentum flux and its forcing on the diurnal tide 1 the diurnal variation of gravity wave gw momentum flux is derived from the 5 years of meteor radar wind measurements at maui hawaii the amplitude and phase relationships between the gw forcing and the diurnal tide are analyzed by calculating their equivalent rayleigh frictions the results show that the gw momentum flux is clearly modulated by the diurnal tide the forcing from the momentum flux convergence has strong effects on both the amplitude and phase of the diurnal tide they can reach 80 ms 1 day 1 for the amplitude and 15 h day 1 for the phase the gw forcing tends to increase the diurnal tide amplitude above 90 km but has a small damping effect below 90 km it tends to increase the phase of the diurnal tide throughout all altitudes seasonal variations of the gw forcing exist which result in differences in their effects on the diurnal tide the magnitudes of the forcing are in agreement with recent results from satellite observations but are much larger than values used in general circulation models this work also demonstrates that meteor radar measurements can provide a valuable data set for the study of gw tide interactions

thermal evolution of permeability and microstructure in sea ice 1 the fluid permeability k of sea ice constrains a broad range of processes such as the growth and decay of seasonal ice the evolution of summer ice albedo and biomass build up such processes are critical to how sea ice and associated ecosystems respond to climate change however studies of k and its dependence on brine porosity and microstructure are sparse here we present a multifaceted theory for k which closely captures laboratory and field data x ray computed tomography provides an unprecedented look at the brine phase and its connectivity we find that sea ice displays universal transport properties remarkably similar to crustal rocks yet over a much narrower temperature range our results yield simple parameterizations for fluid transport in terms of temperature and salinity and permit more realistic representations of sea ice in global climate and biological models

the pristine shape of olympus mons on mars and the subaqueous origin of its aureole deposits abstract the tallest volcano in the solar system olympus mons on mars is bordered by at least ten enormous sub circular hummocky deposits forming a welded halo termed the aureole the aureole units or simply aureoles which are the deposits of landslides from olympus mons have dramatically transformed the pristine size and shape of the volcanic edifice topographic data are used to determine the amount of collapsed material and so reconstruct the original outline of olympus mons before the landslides took place under the assumption that the edifice did not start failing until it had reached this maximum size due to post aureole deposition on the eastern and southern flanks and to the uncertainty of the slippage level on the northern side the reconstruction is sufficiently precise along the western and north western olympus mons flank it is more uncertain for the northern flank while it is not feasible around the rest of the volcano it appears that the radius along the western and north western olympus mons before the collapse of the aureole landslides was approximately 200 km longer or more the results show that the volume of the aureoles even if enormous is insufficient to fill the ideal conical edifice which would be obtained prolonging the olympus mons flanks with present slope angles thus an overhang remains in the pre aureole reconstructed olympus mons which would also explain the onset of instability that led to the aureole collapse further a drape deposit blanketing the southern acheron fossae ridge just at the front of the western w aureole landslide deposit and a fan channel system carved on the same w aureole are investigated and it is suggested that these morphologies have been emplaced in subaqueous setting while the drape may indicate a landslide thrust water splash akin to a tsunami deposit caused by the fast travelling w aureole landslide the fan channel system is similar to certain morphologies in the terrestrial oceans a numerical model of the collapse of the western aureole unit in water shows final runouts on both acheron ridge and amazonis planitia compatible with observations provided that the friction angle is extremely small of the order of a tenth of degree simulations indicate that the w aureole could have reached acheron fossae ridge with velocities in excess of 100 m s which would explain the several tens of km long distance reached by the landslide thrust tsunami deposit in short morphological and numerical lines of evidence would indicate a subaqueous origin for the largest w aureole landslide

a network model for fluid transport through sea ice the flow of liquid through porous sea ice is a fundamental process affecting problems in polar biology oceanography and geophysics the geometry and connectedness of the pore microstructure of sea ice determine its fluid permeability which depends strongly on temperature here we analyze a simple pipe network as a basis for modeling fluid flow through the complex porous microstructure and for numerical approximations of the fluid permeability of sea ice as a function of temperature for slow flow the fluid system is equivalent to an electrical resistor network and the network is solved using a fast multi grid method the radii of the pipes in the network are chosen randomly from distributions describing measured cross sectional areas of brine inclusions in sea ice at this stage the model reflects only the most general features of brine microstructure and its evolution with temperature preliminary results for a basic implementation in two dimensions are presented they are consistent with theoretical bounds on the vertical fluid permeability of sea ice found recently moreover the results agree roughly with laboratory data for higher porosities for lower porosities and colder temperatures the fully connected network of pipes in the model albeit with smaller radii overestimates observed values this finding provides evidence that the brine network becomes more disconnected with lower temperatures which is consistent with transitional behavior near a percolation threshold

aureole deposits of the martian volcano olympus mons the aureole of grooved terrain that surrounds the large shield volcano olympus mons consists of several overlapping roughly circular sheets each 0 5 to 1 5 km thick the surfaces of these materials bear abundant curvilinear ridges and troughs 10 to 100 km long and 1 to 5 km wide which form anastomosing patterns that vary in length and width over the aureole the aureole is asymmetric to olympus mons extending almost 1000 km northwest from the center of the volcano but only 600 km southeast the lobate form of the deposits the pressure ridges on their surfaces and the deflection of aureole material around barriers indicate that the deposits were emplaced as viscous flows high resolution viking orbiter pictures show the aureole material to be unstratified and it is inferred to contain randomly distributed large dark blocks whose weathering products form dark streaks in the talus on the flanks of ridges a pyroclastic origin is proposed for the aureole the following sequence is suggested at least six great pyroclastic eruptions occurred prior to the construction olympus mons they formed very fluid ash flows that became viscous during late stages of emplacement and pressure ridges formed on the surfaces of the deposits before they finally came to rest the oldest and most extensive aureole deposit finely grooved terrain was considerably modified by erosion prior to being partly covered by later eruptions a positive gravity anomaly over the olympus mons area may define the site of a near surface magma chamber that was the source of the pyroclastic eruptions

winter temperature tides from 30 to 110 km at mcmurdo 77 8 s 166 7 e antarctica lidar observations and comparisons with wam we provide the first characterization of diurnal and semidiurnal thermal tides in temperature from 30 to 110 km in the winter season may through august at mcmurdo 77 8 s 166 7 e antarctica the observations were made with an fe boltzmann temperature lidar in 2011 and 2012 over 330 h of winter data are compiled into a composite day of temperature perturbations that significantly reduce the incoherent wave effects while preserving the coherent tidal signatures both diurnal and semidiurnal tides have small amplitudes less than 3 k below 100 km with vertical wavelengths of 29 and 23 km respectively a new finding of this study is the fast growth of diurnal and semidiurnal tidal amplitudes above 100 km to at least 15 k near 110 km exceeding that of the freely propagating tides originating from the lower atmosphere such fast growth exists for all kp index cases and diurnal amplitude increases to 15 30 k at 110 km with larger kp indices corresponding to larger tidal amplitudes and faster growth rates the slopes of diurnal tidal phases become steeper above 100 km and the tidal phases barely change with altitude from 100 to 106 km the tidal growth behavior is reproduced in the whole atmosphere model wam with phases comparable to the observations but magnitudes significantly underestimated wam compares reasonably well with the observations below 100 km the observed significant amplitude increases and phase structure changes suggest additional tidal sources near or above 100 km which deserve future investigation

mars stratigraphy and gravimetry of olympus mons and its aureole olympus mons and its surroundings have been investigated using impact crater statistics crater retention ages of all major geological units show that their emplacement occurred during three time intervals the underlying fractured plains are part of the northern plains in general n 1 4 10 3 km 2 this time is followed by the time interval represented by crater retention ages n 1 8 10 4 to 3 10 3 km 2 some lava flows in the fractured plains the smooth plains and the aureole materials were emplaced during this time the aureole probably developed by some sort of collapse of the outer parts of an ancient volcano proto olympus mons underlying the present shield its remnants may show in the scarp and small parts of the shield not covered by younger lava flows the third interval covers crater retention ages n 1 5 10 5 to 3 10 4 km 2 this volcanic activity followed a period of dormancy a series of lava flows forming caldera and present shield surface and flooding a depression around the shield are distinguishable the regional stratigraphy is discussed as part of the global geological history the question of the genesis of the aureole material is addressed by gravity models the topographic mass of olympus mons contributes about 80 to the aureole gravity high northwest of the mountain the gravity high of the entire aureole can be explained by a density model consisting of the topographic masses of olympus mons and the aureole materials it does not require additional high density materials underneath the aureole thus aureole materials of an allochthonous origin by collapse are in agreement with the gravity data however the gravity data do not preclude an autochthonous and volcanic origin of the aureole materials in the latter case possible subsurface intrusions should have no density contrasts with the surroundings

source regions for antarctic mlt non migrating semidiurnal tides 1 source regions for the westward propagating zonal wavenumber one and three components of the semidiurnal tide observed in the summer mesosphere and lower thermosphere over antarctica are identified by correlating local tidal variations with global planetary wave one activity in the stratosphere and lower mesosphere the advantages of using zonal wavenumber resolved tidal amplitudes for such a study are described the results support the prediction of a source region in the northern hemisphere

mars paleostratigraphic restoration of buried surfaces in tharsis montes volcanism in the tharsis province of mars occurred in several different areas and was generally continuous without large time intervals between eruptive episodes major lava flow units are numerous and extensive but relatively thin in many places impact craters on buried surfaces project above younger flows that overlie them a new application of crater dating methods has been developed to aid in the identification of these buried surfaces and to determine their lateral extent the technique is especially adaptable to the tharsis region where the stratigraphic succession of major flow units has been established by detailed geologic mapping knowledge of the overall stratigraphy allows correlations to be made between known and unknown surfaces by comparing their crater frequencies at diameters large enough to insure their recognition on the buried unit the method has been applied to aid in the restoration of buried rock units and to construct a series of paleostratigraphic maps showing the sequence of major eruptive events in the tharsis region

thermal expansion coefficients for sea ice coefficients of thermal linear expansion were determined for sea ice using a michelson interferometer over a temperature range of 4 to 15 c the coefficients varied from 45 10 6 to 54 10 6 c 1 for ice with a salinity of 2 ppt and from 33 10 6 to 53 10 6 c 1 for ice with a salinity of 4 ppt initially warming the sea ice resulted in coefficients that were the same as those for fresh water ice within the limits of experimental error subsequent sea ice cooling resulted in coefficients that were initially lower than those for fresh water ice but that asymptotically approached the coefficient values for fresh water ice at colder temperatures on the second warming and cooling cycle the coefficients of thermal linear expansion exhibited hysteresis and a decrease in magnitudes we have also shown that pettersson s 1883 and malmgren s 1927 measurements of the thermal volume expansion of sea ice were the result of phase transitions that caused brine expulsion when air free sea ice was cooled and internal porosity increases when sea ice was warmed our results indicate that petterson s 1883 and malmgren s 1927 measurements of the thermal volume expansion of sea ice are in error consequently theoretical descriptions based on their results are incorrect anderson 1960 zubov and savelyev given in doronin and kheisin 1977 doronin and kheisin 1977 our results for the initial sea ice warming cycle do agree with cox s 1983 analysis

microdynamics of ice understanding the dynamic behaviour of ice in glaciers polar ice caps sea ice and the icy planets of the solar system is a major challenge especially in a time of changing climate amplified at the poles and exciting new space exploration this theme issue of the philosophical transactions of the

tides in the mesopause region over antarctica comparison of whole atmosphere model simulations with ground based observations almost a quarter century ago first optical and radar observations from the south pole revealed rich dynamics unexpected from classical tidal theory a strong semidiurnal wind oscillation was detected near the mesopause implying substantial deviations from the classical view that the semidiurnal variation is dominated by the migrating tide subsequent systematic observations exhibited large seasonal variations of both the diurnal and semidiurnal tide with dramatic reduction in amplitude from summer to winter first numerical simulations with a realistic general circulation model extending into the lower thermosphere indicated the presence of nonmigrating tides with substantial amplitudes in the polar regions however direct model data comparisons have been limited to idealized linear models here whole atmosphere model wam simulations for january and july are compared with available wind climatologies based on multiyear radar observations at different locations in antarctica as well as with first summertime lidar measurements of temperature the diurnal tide simulation agrees well with most of the independent radar and satellite wind observations in both seasons the strong semidiurnal tide comprised of migrating and nonmigrating components is well reproduced in summer while in winter the model tends to overestimate the amplitudes over the continental edge besides model validation a self consistent numerical solution also enables cross validation of observations made with different instruments at different locales

tidal oscillations of the arctic upper mesosphere and lower thermosphere in winter the upper mesosphere and lower thermosphere of the northern polar cap was investigated using fabry perot interferometer measurements of the horizontal wind velocity in the lower thermosphere meridian scanning photometer observations of atomic oxygen green line brightness in the lower thermosphere and michelson interferometer records of the infrared meinel oh bands brightness and rotational temperature in the upper mesosphere tidal airglow oscillations in the absence of local solar heating were studied using a superposed epoch analysis of observations obtained around three new moon intervals november 9 22 1993 december 7 20 1993 and january 4 17 1994 in eureka 80 n tidal harmonics were uncovered with an iterated least chi squared fit and their existence in the data tested using a goodness of fit probability against a null hypothesis of no oscillations no single dominant tide was found at all times and altitudes of the winter arctic upper mesosphere and lower thermosphere the horizontal wind velocity of the lower thermosphere exhibited all the first three harmonics of the tide with the largest amplitude oscillations shown by the diurnal component of the meridional wave speed the atmospheric layer near the mesopause that contributes to the oh airglow emission experienced terdiurnal oscillations throughout the winter season theoretical polarization relations for evanescent tides considerations of energy density propagation with altitude and a day by day analysis of the zonal and meridional wind speed and temperature all indicate that the terdiurnal tide observed on november was an evanescent zonally symmetric tide other data indicate propagating tides migrating tides or a mixture of both

evidence for nonlinear coupling of planetary waves and tides in the antarctic mesopause analyses of hourly mean meridional and zonal winds near 95 km observed with the meteor radar system at molodezhnaya station 68 s 45 e during 1990 reveal the presence of long period 2 18 day waves with dominant periods corresponding to those of rossby normal modes modified by mean zonal winds time varying analyses indicate that although significant contributions at planetary wave periods persist with nearly constant periods for intervals of days to weeks temporal variability of these periods is observed over longer intervals tidal motions which mainly consist of the semidiurnal and the diurnal periods demonstrate considerable modulation of their amplitudes that vary with time the observed tidal amplitude modulations are investigated through bispectral analyses the results of these analyses suggest nonlinear interactions of quadratic form between oscillations with periods in the range of 2 to 19 days and the diurnal and semidiurnal tides at various intervals during 1990

density and lithospheric thickness of the tharsis province from mex mars and mro gravity data 1 radio science tracking of mars express mars experiment and mars reconnaissance orbiter produced high resolution martian gravity data applying localized spectral analysis on the new gravity data sets we study the surface density and lithospheric elastic thickness in the tharsis province the gravity signal is predicted with geophysical models either including bottom loading top bottom model or taking into account the loading history top top model volcanic shields are mainly composed of high density lava but their construction could have begun with lower density lava with the exception of ascraeus mons which has a top of lower density buoyant bottom loading may have been present in the form of a mantle plume under olympus mons the elastic thickness was much larger at olympus mons than at other volcanoes suggesting large spatial variations of heat flux during the hesperian alternatively small elastic thicknesses could be artifacts reflecting the presence of very localized high density crustal intrusions beneath the volcanoes thaumasia highlands were probably supported by a mantle plume at the time of formation in valles marineris top bottom models predict low densities and large elastic thicknesses in conflict with the basaltic rock composition and hesperian age of the valley dense mafic dikes underlie the western part of the valley the top top model serves to test another scenario in which the trough is formed with sedimentary infilling removed much later by erosion the elastic thickness increasing in between at the large volcanoes the relation between gravity and topography is anisotropic probably because of density variations

nonlinear interactions in the upper atmosphere the s 1 and s 3 nonmigrating semidiurnal tides 1 a semidiurnal oscillation with zonal wave number s 1 has been observed over the south pole and longitudinal variations of the semidiurnal tide at northern midlatitudes have been ascribed to the presence of nonmigrating tides a three dimensional nonlinear spectral model is used herein to study nonlinear wave wave interaction as a possible mechanism for the generation of nonmigrating tides in the mesosphere and lower thermosphere in particular the s 1 and s 3 nonmigrating semidiurnal tides are studied as a by product of the nonlinear interaction between the semidiurnal s 2 migrating tide and a stationary s 1 planetary wave in the lower and middle atmosphere this process is found to yield significant amplitudes 10 30 m s 1 of the nonmigrating semidiurnal components with s 1 and s 3 in the upper atmosphere comparisons with monthly nonmigrating tidal amplitudes and phases at 95 km derived from high resolution doppler imager and wind imaging interferometer wind measurements from uars show good agreement with the model simulations the effect of the dissipating nonmigrating tides on the zonal mean circulation is found to reinforce that of the migrating component contributing 10 20 m s 1 to the zonal wind field and 5 10 m s 1 to the mean meridional wind field several other wave components are generated through nonlinear interactions including 6 hour tides with zonal wave numbers s 0 1 4 and a semidiurnal oscillation with s 6 these wave components have amplitudes in the range 6 30 m s 1 in the 110 150 km height regime the combination of all nonmigrating tides together with the migrating component suggests significant longitudinal variations in the semidiurnal tide in the e region which may be important for studies of the quiet time generation of ionospheric electric fields by the dynamo mechanism

the relationship between martian gravity and topography the relationship between gravity and topography of various regions of mars is used to estimate their effective elastic thicknesses te using direct measurements of line of sight velocity rather than spherical harmonic coefficients estimates of te vary from 70 km for tharsis 29 km for elysium to 14 5 km for the southern hemisphere and show that the thickness of the martian lithosphere increases with age as the radioactive isotopes of k th and u decay a simple parameterised model of the convective thermal history is used to estimate the temperature structure of the lithosphere and shows that the base of the elastic layer has a temperature of 300 50 c or similar to the value for terrestrial continents in both cases the rheology is probably affected by the presence of water the short wavelength behaviour of the gravity field allows the density of the rocks that form the topography to be estimated and gives values of about 3 0 mg m3 for tharsis and elysium this value is substantially greater than that of 2 7 mg m3 obtained for earth and is in agreement with estimates from snc shergottites nahklites chassigny meteorites of 3 3 mg m3 the density of the topography of valles marineris is only 2 35 mg m3 and suggests that ice may be present below the surface in the heavily bombarded southern hemisphere isostatic compensation occurs at wavelengths as short as 700 km which requires the effective compensation depth to be no more than 10 km the gravity field with wavelengths greater than 1500 km may be supported dynamically by a plume rising beneath the tharsis region the difference in temperature between the solidus and the present areotherm is less than 250 c so melt generation can occur in rising plumes

the olympus mons aureole formation by gravitational spreading new observations of the aureole deposits of olympus mons are in agreement with previous suggestions that the aureole lobes could have been formed by movement under gravity away from the observed scarps the characteristic corrugated morphology of the aureole is probably secondary formed by erosion along structural inhomogeneities geometries of the corrugations and translational faults in the aureole deposits favor a mechanism of emplacement that involves material with substantial shear strength rather than viscous flow estimates of the aspect ratios of terrestrial landslides nappes and ash flows suggest that the aureole deposits are more similar in overall shape to slide emplaced bodies than to pyroclastic flows although martian physical conditions permit the formation of ash flows there is no positive evidence for their existence a gravitational spreading mechanism is proposed that involves imbricate thrusting in distal regions analogous with terrestrial thrust sheets corrugations in the aureole developed by erosion along imbricate or listric faults basal shear stresses on the decoupling surface may have been of the order of 106 pa 10 bars the nature of the decoupling surfaces in the proximal regions is uncertain but is likely to have been the topographic surface in distal parts the aureole deposits were probably emplaced as a series of sheets by spreading under gravity from an ancestral olympus mons which extended farther to the northwest than does the present volcano as a result of the accumulation of lavas under the then prevailing stress conditions recent lava eruptions from the volcano have been concentrated in northeast and southwest sectors indicating a changed stress regime since aureole emplacement

twelve hour tides in the winter northern polar mesosphere and lower thermosphere 1 an investigation of the tidal oscillations near the winter northern polar mesopause has been carried out at resolute bay canada 74 9 n 94 9 w the daily monthly and annual variations of the tidal field were studied using the 1995 1996 and 1996 1997 data ground based measurements were obtained using a fabry perot interferometer with a circle to line interferometric optical system fpi clio and the e region wind interferometer erwin the fpi clio observed the doppler winds of the oh emission near 86 km altitude the erwin provided simultaneous oh near 86 km and oi near 97 km wind measurements monthly data were compared to the global scale wave model gswm and the forbes vial solar semidiurnal tidal model predictions analysis of the 12 hour oscillation near 86 and 97 km altitudes indicates that it is persistent and characteristic of a semidiurnal propagating tide the semidiurnal tide was found to be highly variable in amplitude and phase from day to day the observations presented provide a continuous and extensive data set for the winter season index terms 3332 meteorology and atmospheric dynamics mesospheric dynamics 3334 meteorology and atmospheric dynamics middle atmosphere dynamics 0341 0342 3384 meteorology and atmospheric dynamics waves and tides keywords semidiurnal tide polar mesosphere polar thermosphere fabry perot interferometer resolute bay mesopause

short term variation of the s 1 nonmigrating semidiurnal tide during the 2002 stratospheric sudden warming 1 in this study the ncar thermosphere ionosphere mesosphere electrodynamics general circulation model time gcm is used to examine short term changes in the global structure of the migrating and s 1 nonmigrating semidiurnal tides in a model run approximating the 2002 southern hemisphere stratospheric sudden warming the time gcm is found to resolve an s 1 nonmigrating semidiurnal tide with latitudinal structure similar to that of prior studies and with global structure in the mlt region strongly correlated with southern hemisphere planetary wave 1 pw1 wave events prior to equinox comparison with a control run with no planetary wave activity eliassen palm flux and correlation analysis of the s 1 semidiurnal tide structure suggest that the wave propagates from the source region in the winter hemisphere stratosphere into both the summer and winter lower thermospheres the amplitudes of the migrating semidiurnal tide in the southern hemisphere are anticorrelated with the nonmigrating tide suggesting significant energy loss due to nonmigrating tidal generation a result not previously seen the amplitude of the s 1 nonmigrating semidiurnal tide from time gcm is also compared with data from the south pole meteor radar system while the observations show bursts of nonmigrating tidal activity correlated to pw1 activity of comparable amplitudes to the model results these events do not always appear at the same times as those in the model this suggests that while the processes generating the nonmigrating tide in time gcm are realistic the time gcm run itself displays differences in time evolution compared to the observations during this time

seasonal variations of semidiurnal tidal perturbations in mesopause region temperature and zonal and meridional winds above fort collins colorado 40 6 n 105 1 w 1 on the basis of colorado state university csu na lidar observations over full diurnal cycles from may 2002 to april 2006 a harmonic analysis was performed to extract semidiurnal perturbations in mesopause region temperature and zonal and meridional winds over fort collins colorado 40 6 n 105 1 w the observed monthly results are in good agreement with mf radar tidal climatology for urbana illinois and with predictions of the hamburg model of the neutral and ionized atmosphere hammonia sampled at the csu na lidar coordinates the observed semidiurnal tidal period perturbation within the mesopause region is found to be dominated by propagating modes in winter and equinoctial months with a combined vertical wavelength varying from 50 km to almost 90 km and by a mode with evanescent behavior and longer vertical wavelength 100 150 km in summer months most likely due to dominance of 2 2 and 2 3 tidal hough modes the observed semidiurnal tidal amplitude shows strong seasonal variation with a large amplitude during the winter months with a higher growth rate above 85 90 km and minimal amplitudes during the summer months maximum tidal amplitudes over 50 m s for wind and 12 k for temperature occur during fall equinox a detailed comparison with hammonia predictions shows excellent agreement in semidiurnal phases hammonia predicted semidiurnal amplitudes generally agree well with observations however hommonia underestimates temperature amplitudes in some of the nonsummer months as well as zonal wind and meridional wind amplitudes in april and september but overestimates them in february to reveal the effects of the atmospheric background on vertical propagation of tidal modes and their relative importance in the composite semidiurnal tide during different seasons we use the lidar observed monthly mean temperature and zonal wind from the same data set as well as hammonia output to calculate the vertical wave number seasonal variations of the major tidal modes of the migrating semidiurnal tide this leads to a qualitative understanding of the lidar observed and hammonia predicted seasonal variation of the semidiurnal tidal perturbation