Chemically distinct regions of Venus’s atmosphere revealed by measured N2 concentrations

[1]  M. Way,et al.  Venus as a Laboratory for Exoplanetary Science , 2019, Journal of Geophysical Research: Planets.

[2]  D. Lawrence,et al.  Cosmogenic radionuclide production modeling with Geant4: Experimental benchmarking and application to nuclear spectroscopy of asteroid (16) Psyche , 2019, Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms.

[3]  W. Feldman,et al.  MESSENGER Gamma Ray Spectrometer and Epithermal Neutron Hydrogen Data Reveal Compositional Differences Between Mercury's Hot and Cold Poles , 2019, Journal of geophysical research. Planets.

[4]  G. Schubert,et al.  The deep atmosphere of Venus and the possible role of density-driven separation of CO2 and N2 , 2017 .

[5]  J. Garvin,et al.  DAVINCI: Deep atmosphere venus investigation of noble gases, chemistry, and imaging , 2016, 2017 IEEE Aerospace Conference.

[6]  L. Nittler,et al.  Geochemical terranes of Mercury’s northern hemisphere as revealed by MESSENGER neutron measurements , 2015 .

[7]  L. Nittler,et al.  Evidence for geochemical terranes on Mercury: Global mapping of major elements with MESSENGER's X-Ray Spectrometer , 2015 .

[8]  Giada Arney,et al.  Spatially resolved measurements of H2O, HCl, CO, OCS, SO2, cloud opacity, and acid concentration in the Venus near‐infrared spectral windows , 2014 .

[9]  David Bazell,et al.  Evidence for Water Ice Near Mercury’s North Pole from MESSENGER Neutron Spectrometer Measurements , 2013, Science.

[10]  Franck Montmessin,et al.  Variations of sulphur dioxide at the cloud top of Venus’s dynamic atmosphere , 2012, Nature Geoscience.

[11]  L. Arnold,et al.  Transmission spectrum of Venus as a transiting exoplanet , 2011, 1112.0572.

[12]  H. Rauer,et al.  Venus transit 2004: Illustrating the capability of exoplanet transmission spectroscopy , 2011, 1107.3700.

[13]  L. Nittler,et al.  Identification and Measurement of Neutron-absorbing Elements on Mercury's Surface , 2010 .

[14]  Giuseppe Piccioni,et al.  Venus surface thermal emission at 1 μm in VIRTIS imaging observations: Evidence for variation of crust and mantle differentiation conditions , 2008 .

[15]  Kim Strohbehn,et al.  The MESSENGER Gamma-Ray and Neutron Spectrometer , 2007 .

[16]  Robert W. Farquhar,et al.  MESSENGER Mission Design and Navigation , 2007 .

[17]  Martin H. Israel,et al.  The Level of Solar Modulation of Galactic Cosmic Rays from 1997 to 2005 as Derived from ACE Measurements of Elemental Energy Spectra , 2005 .

[18]  R. D. O'dell,et al.  Gravitational effects on planetary neutron flux spectra , 1989 .

[19]  W. Feldman,et al.  A Doppler filter technique to measure the hydrogen content of planetary surfaces , 1986 .

[20]  G. M. Keating,et al.  The Venus international reference atmosphere , 1986 .

[21]  Henry E. Revercomb,et al.  Models of the structure of the atmosphere of Venus from the surface to 100 kilometers altitude , 1985 .

[22]  L. Esposito,et al.  Sulfur Dioxide: Episodic Injection Shows Evidence for Active Venus Volcanism , 1984, Science.

[23]  Qin Lu,et al.  Preface , 1976, Brain Research Bulletin.

[24]  R. Lingenfelter,et al.  Neutron Leakage Flux and the Nitrogen Abundance of Venus , 1962 .