A5005193709- Planetary Science and Exploration
- Astro and Planetary Science
- Solar and Space Plasma Dynamics
- Ionosphere and magnetosphere dynamics
- Space Science and Extraterrestrial Life
- Space exploration and regulation
- Earthquake Detection and Analysis
- Histone Deacetylase Inhibitors Research
- Geomagnetism and Paleomagnetism Studies
- Geophysics and Gravity Measurements
- GNSS positioning and interference
- Glioma Diagnosis and Treatment
- Cancer therapeutics and mechanisms
Laboratory for Atmospheric and Space Physics
2017-2021
University of Colorado Boulder
2017-2021
University of Colorado System
2020-2021
Duke University
2004
Irinotecan is a topoisomerase I inhibitor previously shown to be active in the treatment of malignant glioma. We now report results phase 1 trial irinotecan plus BCNU, or 1,3-bis(2-chloroethyl)-1-nitrosourea, for patients with recurrent progressive MG. dose escalation occurred independently within 2 strata: receiving enzyme-inducing antiepileptic drugs (EIAEDs) and not EIAEDs. BCNU was administered at 100 mg/m2 over h every 6 weeks on same day as first administered. intravenously 90 min once...
Abstract The Magnetic Pileup Boundary or Induced Magnetosphere (IMB) has been an enigma in Mars aeronomy. Previously dubbed the planetopause, magnetopause, ion‐composition boundary, and protonopause, identification of this unique plasma region marked by difficulty. In case study, we used data from Atmosphere Volatile EvolutioN (MAVEN) mission to identify IMB crossings configurations during month September 2017, with a particular focus on 10, 2017 solar events. It was concluded that...
Abstract The Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft can act as an intermittent upstream solar wind monitor at 1.5 AU. To inspect the evolution of turbulence in Martian exosphere, we have gathered proton (i.e., ionized hydrogen) temperature measurements taken by Solar Wind Ion Analyzer (SWIA) onboard MAVEN spacecraft. Here investigate instabilities driven anisotropy during southern hemisphere fall, winter, spring, summer seasons. We look relationship between anisotropy,...
Abstract Normal solar wind flows and intense transient events interact directly with the upper Martian atmosphere due to absence of an intrinsic global planetary magnetic field. Since launch Mars Atmosphere Volatile EvolutioN (MAVEN) mission, there are now new means observe parameters at planet's orbital location for limited time spans. Due MAVEN's highly elliptical orbit, in situ measurements cannot be taken while MAVEN is inside Mars' magnetosheath. To model conditions during these...
Earth and Space Science Open Archive This work has been accepted for publication in Journal of Geophysical Research - Physics. Version RecordESSOAr is a venue early communication or feedback before peer review. Data may be preliminary. Learn more about preprints. preprintOpen AccessYou are viewing the latest version by default [v1]The Effects Different Drivers on Induced Martian Magnetosphere Boundary: A Case Study September 2017Authors Christy L Lentz iD Daniel N. Baker Laila Andersson...
Earth and Space Science Open Archive This work has been accepted for publication in Journal of Geophysical Research - Physics. Version RecordESSOAr is a venue early communication or feedback before peer review. Data may be preliminary. Learn more about preprints. preprintOpen AccessYou are viewing the latest version by default [v1]On Solar Wind Proton Temperature Anisotropy at Mars' Orbital LocationAuthorsChristy L.LentziDAlexandrosChasapisiDRamiz A.QudsiiDJasper...