A perturbation method for evaluating the magnetic field induced from an arbitrary, asymmetric ocean world analytically [0.03%]
一种评估任意非对称海洋世界磁场的摄动方法
Marshall J Styczinski,Steven D Vance,Erika M Harnett et al.
Marshall J Styczinski et al.
Magnetic investigations of icy moons have provided some of the most compelling evidence available confirming the presence of subsurface, liquid water oceans. In the exploration of ocean moons, especially Europa, there is a need for mathemat...
Marshall J Styczinski,Erika M Harnett
Marshall J Styczinski
The five largest planets all have strong intrinsic magnetic fields that interact with their satellites, many of which contain electrically conducting materials on global scales. Conducting bodies exposed to time-varying magnetic fields indu...
The interaction of deep convection with the general circulation in Titan's atmosphere. Part 1: Cloud Resolving Simulations [0.03%]
土卫六大气中深对流与全球环流的相互作用。第1部分：云 resolving 模拟研究
S Rafkin,J M Lora,A Soto et al.
S Rafkin et al.
The deep convective cloud-environment feedback loop is likely important to Titan's global methane, energy, and momentum cycles, just as it is for Earth's global water, energy, and momentum budgets. General circulation models of Titan's atmo...
The interaction of deep convection with the general circulation in Titan's atmosphere. Part 2: Impacts on the climate [0.03%]
土卫六大气中深对流与大循环相互作用的气候影响（第二部分）
J Michael Battalio,Juan M Lora,Scot Rafkin et al.
J Michael Battalio et al.
The impact of methane convection on the circulation of Titan is investigated in the Titan Atmospheric Model (TAM), using a simplified Betts-Miller (SBM) moist convection parameterization scheme. We vary the reference relative humidity (RHSB...
Baroclinic waves in the northern hemisphere of Mars as observed by the MRO Mars Climate Sounder and the MGS Thermal Emission Spectrometer [0.03%]
火星北半球由MRO火星气候探测仪和MGS热辐射光谱仪观测到的横槽波
David P Hinson,R John Wilson
David P Hinson
The climatology of baroclinic waves in the northern hemisphere of Mars is investigated through analysis of observations by the infrared sounders on Mars Reconnaissance Orbiter (MRO) and Mars Global Surveyor (MGS). We focus on the lowest sca...
Colin M Dundas,Glen E Cushing,Laszlo P Keszthelyi
Colin M Dundas
Both the northern and southern arms of Kasei Valles are occupied by platy-ridged flood lavas. We have mapped these flows and examined their morphology to better understand their emplacement. The lavas were emplaced as high-flux, turbulent f...
Colin M Dundas
Colin M Dundas
Recurring Slope Lineae (RSL) on Mars have been enigmatic since their discovery; their behavior resembles a seeping liquid but sources of water remain puzzling. This work demonstrates that the properties of RSL are consistent with observed b...
Multiple mineral horizons in layered outcrops at Mawrth Vallis, Mars, signify changing geochemical environments on early Mars [0.03%]
火星马沃斯地区的层状地层中的多个矿物层表明早期内行星的地球化学环境在发生变化
Janice L Bishop,Christoph Gross,Jacob Danielsen et al.
Janice L Bishop et al.
Refined calibrations of CRISM images are enabling identification of smaller deposits of unique aqueous materials on Mars that reveal changing environmental conditions at the region surrounding Mawrth Vallis. Through characterization of thes...
Mars Perihelion Cloud Trails as revealed by MARCI: Mesoscale Topographically Focussed Updrafts and Gravity Wave Forcing of High Altitude Clouds [0.03%]
火星近日点云系轨迹的MARCI观测：中尺度地形聚焦上升气流和高山云系重力波强迫
R Todd Clancy,Michael J Wolff,Nicholas G Heavens et al.
R Todd Clancy et al.
Daily, global wide angle imaging of Mars clouds in MARCI (MARs Color Imager, (Malin et al., 2008)) ultraviolet and visible bands reveals the spatial/seasonal distributions and physical characteristics of perihelion cloud trails (PCT); a cla...
A P Jordan
A P Jordan
Soil on the Moon is darkened by space weathering, a process generally assumed to be dominated by the solar wind and/or micrometeoroid impacts. Recent work, however, predicts that another process darkens the soil: large solar energetic parti...