Zobrazeno 1 - 10
of 49
pro vyhledávání: '"Stefan E. Thonnard"'
Autor:
Sixto A. González, Andrew W. Stephan, Gary S. Bust, Farzad Kamalabadi, Stefan E. Thonnard, Kenneth F. Dymond, Daniel M. Cotton, Robert P. McCoy, Scott A. Budzien, Paul A. Bernhardt, Supriya Chakrabarti
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 64:1573-1580
Tomographic characterization of ionospheric and thermospheric structures using integrated line-of-sight measurements provides a unifying paradigm for the investigation of various aeronomic phenomena. In radio tomography, measurements of the total ele
Autor:
Kenneth F. Dymond, Scott A. Budzien, Andrew W. Stephan, Robert P. McCoy, Supriya Chakrabarti, Stefan E. Thonnard
Publikováno v:
Journal of Geophysical Research: Space Physics. 106:30323-30330
We report the detection of storm time enhancements in the low-latitude far ultraviolet airglow as observed by the Low-Resolution Airglow and Aurora Spectrograph on the Advanced Research and Global Observation Satellite. The enhancements are present i
Autor:
Kenneth F. Dymond, Ronald J. Thomas, Scott A. Budzien, Andrew C. Nicholas, Robert P. McCoy, Stefan E. Thonnard
Publikováno v:
Journal of Geophysical Research: Space Physics. 106:30315-30321
We present electron density profiles derived by inversion of ultraviolet limb radiances observed on November 24, 1999, by the Low-Resolution Airglow and Aurora Spectrograph instrument on the Advanced Research and Global Observing Satellite. The solar
Publikováno v:
Geophysical Research Letters. 28:927-930
We present electron density profiles derived by inversion of ultraviolet limb scans made by the High Resolution Airglow and Aurora Spectroscopy (HIRAAS) experiment on the Advanced Research and Global Observing Satellite (ARGOS). The ultraviolet limb
Autor:
Scott A. Budzien, Robert P. McCoy, Ronald J. Thomas, T. N. Bullett, Stefan E. Thonnard, Eric Bucsela, Kenneth F. Dymond
Publikováno v:
Journal of Geophysical Research: Space Physics. 105:23025-23033
We present the results of an analysis of the O II 834 A and O I 1356 A altitude profiles measured during a sounding rocket flight on March 19, 1992. The profiles were analyzed using a new set of models that used discrete inverse theory to seek a maxi
Autor:
Nestor Aponte, Stephen C. Collins, Michael C. Kelley, Jonathan J. Makela, Stefan E. Thonnard, Wesley E. Swartz, Craig A. Tepley
Publikováno v:
Geophysical Research Letters. 27:2825-2828
A series of campaigns has been carried out in the Caribbean over a one-year period to study intense mid-latitude spread-F events using a cluster of diversified instrumentation. These events are relatively rare but a number of them have now been captu
Autor:
Kenneth F. Dymond, Stefan E. Thonnard, J. M. Picone, Andrew C. Nicholas, Douglas P. Drob, R. R. Meier
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 62:1317-1326
A key application to be derived from Space Weather research will be to forecast atmospheric drag on low Earth orbit (LEO) satellites with significantly better accuracy than is attainable today. The recently launched STP P91-1 ARGOS mission will serve
Autor:
Judith Lean, Douglas P. Drob, J. M. Picone, Andrew C. Nicholas, R. R. Meier, A. E. Hedin, Stefan E. Thonnard
Publikováno v:
Physics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science. 25:537-542
The Naval Research Laboratory (NRL) has embarked on a development program to upgrade empirical models of the neutral upper atmosphere (thermosphere and upper mesosphere) and to apply these models to scientific and engineering problems. The program fo
Publikováno v:
Radio Science. 32:1985-1996
We present a technique for using the measured variations of ultraviolet emissions produced by radiative recombination at 911 and 1356 A to determine the nighttime altitude distribution of F region O+ ions and electrons. The algorithm uses an iterativ
Autor:
Kenneth F. Dymond, T. Joseph W. Lazio, Pamela J. Loughmiller, Jonathan J. Makela, Clayton Coker, Stefan E. Thonnard
Publikováno v:
Radio Science. 44
[1] Radio astronomers are searching the cosmos for new scientific discoveries at increasingly lower radio frequencies and with larger antenna arrays, but their observations of the sky are blurred by the dynamic ionosphere. At the same time, ionospher