Atmosphere from AARDDVARK Subionospheric VLF Observations
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C. Rodger | M. Clilverd | T. Ulich | T. Raita | J. Neal | N. Thomson
[1] G. Reeves,et al. Acceleration and loss of relativistic electrons during small geomagnetic storms , 2015, Geophysical research letters.
[2] I. Whittaker,et al. The effects and correction of the geometric factor for the POES/MEPED electron flux instrument using a multisatellite comparison , 2014 .
[3] Juan V. Rodriguez,et al. A statistical approach to determining energetic outer radiation belt electron precipitation fluxes , 2014 .
[4] B. Ni,et al. Resonant scattering and resultant pitch angle evolution of relativistic electrons by plasmaspheric hiss , 2013 .
[5] Craig J. Rodger,et al. Determining the spectra of radiation belt electron losses: Fitting DEMETER electron flux observations for typical and storm times , 2013 .
[6] C. Rodger,et al. Comparison between POES energetic electron precipitation observations and riometer absorptions: Implications for determining true precipitation fluxes , 2013 .
[7] Xuemin Zhang,et al. DEMETER observations of high‐latitude chorus waves penetrating the plasmasphere during a geomagnetic storm , 2013 .
[8] B. Ni,et al. Constructing the global distribution of chorus wave intensity using measurements of electrons by the POES satellites and waves by the Van Allen Probes , 2013 .
[9] C. Rodger,et al. Longitudinal hotspots in the mesospheric OH variations due to energetic electron precipitation , 2013 .
[10] D. Newnham,et al. The effect of energetic electron precipitation on middle mesospheric night‐time ozone during and after a moderate geomagnetic storm , 2012 .
[11] S. Saito,et al. Relativistic electron microbursts associated with whistler chorus rising tone elements: GEMSIS‐RBW simulations , 2012 .
[12] C. Rodger,et al. Contrasting the responses of three different ground‐based instruments to energetic electron precipitation , 2012 .
[13] J. Green,et al. A Monte Carlo simulation of the NOAA POES Medium Energy Proton and Electron Detector instrument , 2011 .
[14] J. Kieser,et al. Atmospheric Ionization Module Osnabrück (AIMOS): 3. Comparison of electron density simulations by AIMOS‐HAMMONIA and incoherent scatter radar measurements , 2011 .
[15] J. Borovsky,et al. Energetic electron precipitation during high-speed solar wind stream driven storms , 2011 .
[16] Sidney W. Wang,et al. Mesospheric Hydroxyl Response to Electron Precipitation From the Radiation Belts , 2011 .
[17] P. Jöckel,et al. Geomagnetic activity related NOx enhancements and polar surface air temperature variability in a chemistry climate model: modulation of the NAM index , 2010 .
[18] R. J. Gamble,et al. Ground‐based estimates of outer radiation belt energetic electron precipitation fluxes into the atmosphere , 2010 .
[19] Josef Koller,et al. Dropouts of the outer electron radiation belt in response to solar wind stream interfaces: global positioning system observations , 2010, Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences.
[20] Richard M. Thorne,et al. Radiation belt dynamics: The importance of wave‐particle interactions , 2010 .
[21] R. J. Gamble,et al. Radiation belt electron precipitation due to geomagnetic storms: Significance to middle atmosphere ozone chemistry , 2010 .
[22] C. Russell,et al. How unprecedented a solar minimum was it? , 2010, Journal of advanced research.
[23] M. J. Birch,et al. On the fine structure of medium energy electron fluxes in the auroral zone and related effects in the ionospheric D-region , 2010 .
[24] T. Moffat‐Griffin,et al. Origin of energetic electron precipitation >30 keV into the atmosphere , 2010 .
[25] A. Chan,et al. New Directions for Radiation Belt Research , 2009 .
[26] J. Tamminen,et al. Impact of different energies of precipitating particles on NOx generation in the middle and upper atmosphere during geomagnetic storms , 2009 .
[27] C. Rodger,et al. NOx enhancements in the middle atmosphere during 2003–2004 polar winter: Relative significance of solar proton events and the aurora as a source , 2007 .
[28] R. Thorne,et al. Review of radiation belt relativistic electron losses , 2007 .
[29] J. Tamminen,et al. Destruction of the tertiary ozone maximum during a solar proton event , 2006 .
[30] M. Jarvis,et al. Dynamic geomagnetic rigidity cutoff variations during a solar proton event , 2006 .
[31] M. Schlesinger,et al. Atmospheric response to NOy source due to energetic electron precipitation , 2005 .
[32] R. Horne,et al. Resonant diffusion of radiation belt electrons by whistler‐mode chorus , 2003 .
[33] D. Drob,et al. Nrlmsise-00 Empirical Model of the Atmosphere: Statistical Comparisons and Scientific Issues , 2002 .
[34] M. Parrot,et al. The micro-satellite DEMETER , 2002 .
[35] K. R. Lorentzen,et al. Observations of relativistic electron microbursts in association with VLF chorus , 2001 .
[36] Alan D. Lopez,et al. First evidence of Ωc0→Ω−π+ , 1993 .
[37] G. Drevin,et al. Riometer quiet day curves determined by the maximum density method , 1990 .
[38] M. Rees. Physics and Chemistry of the Upper Atmosphere , 1989 .
[39] R. A. Goldberg,et al. Nighttime auroral energy deposition in the middle atmosphere , 1984 .
[40] G. L. Hower,et al. Riometer quiet day curves , 1967 .
[41] Xinlin Li,et al. The Electron Radiation Belt , 2001 .