Bibliography
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Found 29 entries in the Bibliography.
Showing entries from 1 through 29
2017 |
The Global-Scale Observations of the Limb and Disk (GOLD) Mission The Earth\textquoterights thermosphere and ionosphere constitute a dynamic system that varies daily in response to energy inputs from above and from below. This system can exhibit a significant response within an hour to changes in those inputs, as plasma and fluid processes compete to control its temperature, composition, and structure. Within this system, short wavelength solar radiation and charged particles from the magnetosphere deposit energy, and waves propagating from the lower atmosphere dissipate. Understanding the global-scale response of the thermosphere-ionosphere (T-I) system to these drivers is essential to advancing our physical understanding of coupling between the space environment and the Earth\textquoterights atmosphere. Previous missions have successfully determined how the \textquotedblleftclimate\textquotedblright of the T-I system responds. The Global-scale Observations of the Limb and Disk (GOLD) mission will determine how the \textquotedblleftweather\textquotedblright of the T-I responds, taking the next step in understanding the coupling between the space environment and the Earth\textquoterights atmosphere. Operating in geostationary orbit, the GOLD imaging spectrograph will measure the Earth\textquoterights emissions from 132 to 162 nm. These measurements will be used image two critical variables\textemdashthermospheric temperature and composition, near 160 km\textemdashon the dayside disk at half-hour time scales. At night they will be used to image the evolution of the low latitude ionosphere in the same regions that were observed earlier during the day. Due to the geostationary orbit being used the mission observes the same hemisphere repeatedly, allowing the unambiguous separation of spatial and temporal variability over the Americas. Eastes, R.; McClintock, W.; Burns, A.; Anderson, D.; Andersson, L.; Codrescu, M.; Correira, J.; Daniell, R.; England, S.; Evans, J.; Harvey, J.; Krywonos, A.; Lumpe, J.; Richmond, A.; Rusch, D.; Siegmund, O.; Solomon, S.; Strickland, D.; Woods, T.; Aksnes, A.; Budzien, S.; Dymond, K.; Eparvier, F.; Martinis, C.; Oberheide, J.; Published by: Space Science Reviews Published on: 10/2017 YEAR: 2017   DOI: 10.1007/s11214-017-0392-2 |
We present the Volume Emission Rate Tomography (VERT) technique for inverting satellite-based, multisensor limb and nadir measurements of atmospheric ultraviolet emission to create whole-orbit reconstructions of atmospheric volume emission rate. The VERT approach is more general than previous ionospheric tomography methods because it can reconstruct the volume emission rate field irrespective of the particular excitation mechanisms (e.g., radiative recombination, photoelectron impact excitation, and energetic particle precipitation in auroras); physical models are then applied to interpret the airglow. The technique was developed and tested using data from the Special Sensor Ultraviolet Limb Imager and Special Sensor Ultraviolet Spectrographic Imager instruments aboard the Defense Meteorological Satellite Program F-18 spacecraft and planned for use with upcoming remote sensing missions. The technique incorporates several features to optimize the tomographic solutions, such as the use of a nonnegative algorithm (Richardson-Lucy, RL) that explicitly accounts for the Poisson statistics inherent in optical measurements, capability to include extinction effects due to resonant scattering and absorption of the photons from the lines of sight, a pseudodiffusion-based regularization scheme implemented between iterations of the RL code to produce smoother solutions, and the capability to estimate error bars on the solutions. Tests using simulated atmospheric emissions verify that the technique performs well in a variety of situations, including daytime, nighttime, and even in the challenging terminator regions. Lastly, we consider ionospheric nightglow and validate reconstructions of the nighttime electron density against Advanced Research Project Agency (ARPA) Long-range Tracking and Identification Radar (ALTAIR) incoherent scatter radar data. Hei, Matthew; Budzien, Scott; Dymond, Kenneth; Nicholas, Andrew; Paxton, Larry; Schaefer, Robert; Groves, Keith; Published by: Radio Science Published on: 07/2017 YEAR: 2017   DOI: 10.1002/2015RS005887 |
2015 |
SSULI/SSUSI UV tomographic images of large-scale plasma structuring Hei, Matthew; Budzien, Scott; Dymond, Kenneth; Paxton, Larry; Schaefer, Robert; Groves, Keith; Published by: Published on: |
2013 |
Tomographic Imaging of Thermospheric Neutral Density Using UV Limb Scanning Dymond, K; Budzien, SA; Nicholas, AC; Published by: Published on: |
2012 |
Global observations of L band scintillation at solar minimum made by COSMIC Published by: Radio Science Published on: Jan-08-2012 YEAR: 2012   DOI: 10.1029/2011RS004931 |
Global-scale Observations of the Limb and Disk (GOLD) Eastes, R; McClintock, W; Aksnes, A; Anderson, D; Andersson, L; Burns, A; Budzien, S; Codrescu, M; Daniell, R; Dymond, K; , others; Published by: AMC Published on: |
Heterogeneous Measurements for Advances in Space Science and Space Weather Forecasting Examples of heterogenous data might include GPS radio occultation limb data and ultraviolet nadir photometry; GUVI/SSUSI cross-track O/N2 maps coupled with SSULI in-track Budzien, Scott; Chua, Damien; Coker, Clayton; Dandenault, Patrick; Dymond, Kenneth; Nicholas, Andrew; Stephan, Andrew; Doe, Richard; Crowley, Geoff; Published by: To emphasize that space weather forecasting with new, full-physics models requires heterogeneous datasets with complementary characteristics—not merely a higher volume of any single data type Published on: |
2011 |
McDonald, Sarah; Coker, Clayton; Dymond, Kenneth; Anderson, David; Araujo-Pradere, Eduardo; Published by: Radio Science Published on: Jan-12-2011 YEAR: 2011   DOI: 10.1029/2011RS004702 |
It is known that there exists a linear relationship between the maximum velocity of the prereversal enhancement (PRE) of the EXB drift and the strength of the equatorial ionization McDonald, Sarah; Coker, Clayton; Dymond, Kenneth; Anderson, David; Araujo-Pradere, Eduardo; Published by: Radio Science Published on: YEAR: 2011   DOI: 10.1029/2011RS004702 |
2010 |
Evolved Tiny Ionospheric Photometer (ETIP): A sensor for ionospheric specification Budzien, Scott; Chua, Damien; Coker, Clayton; Dandenault, Patrick; Dymond, Kenneth; Nicholas, Andrew; Doe, Richard; Crowley, Geoff; Published by: To address the requirements for space weather sensors, and includes adequate flexibility for accommodation on a range of future flight opportunities, including microsatellite constellations Published on: |
Combined in-situ and top-side remote observations of evolution of plasma bubbles Barjatya, A; Eastes, R; Dymond, K; Published by: Published on: |
2009 |
Observations of the Ionosphere Using the Tiny Ionospheric Photometer. Coker, Clayton; Dymond, Kenneth; Budzien, Scott; Chua, Damien; Liu, Jann-Yenq; Anderson, David; Basu, Sunanda; Pedersen, Todd; Published by: Terrestrial, Atmospheric \& Oceanic Sciences Published on: |
Continuous FUV/EUV Imaging of the Ionosphere from Geosynchronous Orbit Wood, Kent; Dymond, KF; Budzien, SA; McDonald, SE; Coker, C; Nicholas, AC; Kowalski, MP; Published by: To use new imaging systems to generate measurements in 2-dimensional formats continuously for large regions with high spatial resolution Published on: |
Remote sensing of nighttime F region peak height and peak density using ultraviolet line ratios We present a newly developed algorithm for simultaneously inferring the peak height and peak density of the O + ions in the nighttime ionosphere. The technique relies on the simultaneous observation of the emissions of atomic oxygen at 130.4 and 135.6 nm that are primarily produced by radiative recombination, a natural decay process of the ionosphere. The 135.6 nm emission has become the workhorse for sensing O + distribution from space from low-Earth platforms where it has been used to infer the peak electron density. Published by: Radio Science Published on: YEAR: 2009   DOI: 10.1029/2008RS004091 |
Ionospheric Electron Density Concurrently Derived by TIP and GOX of FORMOSAT-3/COSMIC. The tiny ion o spheric pho tom e ter (TIP) and GPS occultation ex per i ment (GOX) onboard FORMOSAT-3/COS MIC (F3/C) are em ployed to mea sure the OI 135.6 nm in ten si ties in Hsu, Mei-Lan; Rajesh, Panthalingal; Liu, Jann-Yenq; Tsai, Lung-Chih; Tsai, Ho-Fang; Lin, Chien-Hung; Dymond, Kenneth; Coker, Clayton; Chua, Damien; Budzien, Scott; , others; Published by: Terrestrial, Atmospheric \& Oceanic Sciences Published on: YEAR: 2009   DOI: 10.3319/TAO.2008.04.24.02(F3C) |
2008 |
Eastes, RW; Anderson, DN; McClintock, WE; Aksnes, A; Andersson, L; Burns, AG; Budzien, SA; Codrescu, MV; Daniell, RE; Dymond, KF; , others; Published by: Published on: |
Hemispheric asymmetries in the longitudinal structure of the low-latitude nighttime ionosphere McDonald, SE; Dymond, KF; Summers, ME; Published by: Journal of Geophysical Research: Space Physics Published on: |
2007 |
Eastes, R; Codrescu, M; McClintock, W; Aksnes, A; Anderson, D; Andersson, L; Burns, A; Budzien, S; Daniell, R; Dymond, K; , others; Published by: Published on: |
Global Observations of the Limb and Disk (GOLD): Temperature Measurements Rusch, D; Aksnes, A; Budzien, S; Eastes, R; Anderson, D; Andersson, L; Burns, A; Codrescu, M; Daniell, R; Dymond, K; , others; Published by: Published on: |
2006 |
The High Resolution Airglow and Aurora Spectroscopy (HIRAAS) experiment was launched aboard ARGOS on 23 February 1999. The HIRAAS experiment operated from mid-May Dymond, KF; McDonald, SE; Coker, C; Bernhardt, PA; Selcher, CA; Published by: Radio science Published on: YEAR: 2006   DOI: 10.1029/2005RS003363 |
First Observations of the Ionosphere using the Tiny Ionospheric Photometer Coker, C; Dymond, KF; Budzien, SA; Chua, D; Liu, JY; Published by: Published on: |
Ionospheric Measurements from the Tiny Ionospheric Photometer Coker, C; Dymond, KF; Budzien, SA; Chua, D; Published by: Published on: |
2005 |
Aksnes, A; Eastes, R; Budzien, S; Dymond, K; Bailey, S; Jones, A; Published by: Published on: |
Dymond, KF; Budzien, SA; McCoy, RP; Crowley, G; Published by: Published on: |
2004 |
A Comparison of LORAAS and GUVI Observations of the Low-Latitude Ionosphere McDonald, SE; Makela, JJ; Meier, RR; Dymond, KF; Thonnard, SE; Budzien, SA; Christensen, AB; Paxton, LJ; Morrison, D; McCoy, RP; Published by: Published on: |
2003 |
Ionosphere and Upper Atmosphere (SIA): SIA 8 Stephan, AW; Meier, RR; Dymond, KF; Budzien, SA; McCoy, RP; Published by: Journal of Geophysical Research-Part A-Space Physics Published on: |
Quenching rate coefficients for O+ (2P) derived from middle ultraviolet airglow Stephan, AW; Meier, RR; Dymond, KF; Budzien, SA; McCoy, RP; Published by: Journal of Geophysical Research: Space Physics Published on: |
Airglow observations of low latitude O and N\_2 during a geomagnetic storm Stephan, AW; Meier, RR; Dymond, KF; Budzien, SA; McCoy, RP; Published by: Published on: |
2002 |
ISAAC measurements of MUV airglow derived from thermospheric O, N 2, and NO Stephan, AW; Meier, RR; Dymond, KF; Budzien, SA; McCoy, RP; Published by: Published on: |
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