A broad range of original scientific and engineering papers and documents from all areas of SET’s team member activity.
Solar Irradiance Platform (SIP)
- Tobiska 2008 AIAA 2008-0453: Mitigating orbit planning, satellite ops, and communication from adverse space weather
- Tobiska 2007 AIAA-2007-0495: SOLAR2000 v2.30 & SOLARFLARE v1.01
- Tobiska et al 2006 AIAA-2006-0471: Solar and Geomagnetic operations models
- Tobiska & Bouwer 2006 JASR: SOLAR2000 v2.24 status
- Tobiska 2005 AIAA-2005-0069: X-ray flare evolution model
- Tobiska 2004 AIAA 2004-1078: A description of 2nd generation forecasting through SOLAR2000
- Tobiska 2004 ASR: SOLAR2000 v1.24 status
- Tobiska 2002 ASR: Variability in the solar constant shortward of Lyman-alpha
- Tobiska et al 2000 JASTP: SOLAR2000 model description
- Tobiska 2000 PCE: Status of the SOLAR2000 solar irradiance model
Solar Applications
- Goncharenko et al. 2021 JGR: New model for ionospheric total electron content
- Edwards et al. 2017 JGR: Field-aligned current response to solar indices
- Tobiska 2010 CO1: JB2008 Solar and Geomagnetic Indices
- Tobiska et al 2008 SA: COSPAR CIRA Draft – Solar and Geomagnetic Indices for the JB2008 Thermospheric Density Model
- Tobiska et al 2008 JASTP: JB2006 Solar Indices
- Tobiska 2008 AMS: Aviation communication and satellite orbit operations
- Tobiska et al 2006 AIAA 2006-6165: Improved thermosphere modeling with JB2006 indices
- Tobiska 2005 AAS: Solar inputs for precision orbit determination
- Tobiska 2005 AIAA 2005-0069: X-ray background index and flare predictions, and ISO solar irradiance standards
- Tobiska, et al 2005 IES: SOLARFLARE model v1.00
- Tobiska 2004 AIAA 2004-1078: SOLAR2000 Professional Grade
- Tobiska 2003 AIAA 2003-1224: Validation of 72-hour forecasting
- Tobiska 2003 JSR: Operational forecast E10.7
- Pardini et al 2002 SWW: Strategy for improving orbit decay modeling
- Tobiska 2002 TIGER: EUV integrated irradiance proxies description
- Knipp et al 2002 COSPAR: EUV hemispheric power, Peuv
- Tobiska 2002 AIAA 2002-4892: E10.7 for forecasting Earth atmosphere drivers
- Tobiska 2002 ASR: Variability in the TSI, S(t), below Lyman-alpha
- Tobiska et al 2002 IES: Improved polar HF propagation
- Tobiska 2002 JGR: E10.7 Reply
- Tobiska 2001 JGR: E10.7 derivation and validation
Solar Research
- Riley, et al 2018 SWJ: Forecasting the Arrival Time of Coronal Mass Ejections
- Gonzalez Hernandez, et al 2014 SP: A Full Sun Magnetic Index from Helioseismology Inferences
- Woods, et al 2011 ApJ: Solar EUV observations during flares
- Woods, et al 2010 SP: SDO EVE Overview Science, Instrument, Data, and Models
- Woods, et al 2005 JGR: Solar EUV Experiment (SEE)
- Tobiska 2003 AIAA 2003-1224: A validation study of the 72-hour forecasting algorithm
- Tobiska 2002 AIAA 2002-4892: A description of the 72-hour forecast of solar, geomagnetic, and atmosphere dynamics
- Tobiska 2002 TIGER: A description of new integrated irradiance proxies
- Viereck, et al 2001 GRL: The NOAA Mg II core-to-wing ratio proxy derivation and long-term data set used by SOLAR2000.
- Woods, et al 2000 JGR: Composite Lyman-alpha for 5 solar cycles calibrated to the UARS
- Woods, et al 1998 SPIE: TIMED Solar EUV Experiment
- Tobiska, et al 1998 SP: A description of the EUV97 solar EUV empirical model
- Tobiska, et al 1997 GRL: Two solar cycles of Lyman alpha calibrated to UARS
- Buonsanto, et al 1995 JGR: Comparison of radar data with ionospheric models using modeled solar flux
- Tobiska 1994 SP: SOLRAD-11 soft X-rays data reconstruction and analysis
- Tobiska, et al 1994 ASR: San Marco ASSI data and EUV91 model output compared
- Tobiska, et al 1993 ASR: A Study of the solar EUV flux variations from San Marco ASSI
- Bouwer 1992 SP: A study of the time-varying properties of photospheric, chromospheric, and coronal indices
- Buonsanto, et al 1992 JGR: Comparison of radar data with E-F1 ionosphere models using EUV91 modeled solar flux
- Tobiska 1991 JATP: Revised Solar Extreme Ultraviolet Flux Model
- Barth, et al 1990 GRL: Comparison of 10.7 cm Radio Flux with SME Solar Lyman Alpha Flux
- Tobiska, et al 1990 JGR: A Solar EUV Flux Model
- Pap, et al 1990 SP: An FFT analysis of 5 solar irradiance and proxy periodicities
- Tobiska, et al 1989 GRL: A Study of solar chromospheric and coronal emissions during solar cycle 21
- Tobiska 1989 JGR: A study of modeled solar flux using SERF2
- Tobiska, et al 1987 JAS: A study of predicted solar flux using Jacchia 1971 model and SME satellite orbit decay
- Jacchia 1971: The revised Jacchia model incorporating revised atmospheric chemistry measurements
- Jacchia 1970: The Jacchia thermospheric/exospheric model
Reviews
- Schmidtke, et al 2006 JASR: TIGER symposium held at COSPAR 2004
- Tobiska 2000 PCE: Review of EUV measurement and modeling
- Tobiska 1996 ASR: Current status of EUV measurements and modeling
- Tobiska 1993 JGR: Review of solar EUV measurements and modeling
- Tobiska 1992 SOLERS22: History of EUV measurements and modeling
- Simon, et al 1991 JGG: Solar EUV irradiance variatio\ns review
Status of Standards Publication Links
- Tobiska 2005 AIAA 2005-0069: Development of ISO 21348 “Process for Determining Solar Irradiances”
- Tobiska, et al 2004 COSPAR: Overview of the solar irradiances standard ISO 21348
- Tobiska 2002 COSPAR: Status of the solar irradiances standard ISO 21348
- Tobiska, et al 2000 PCE: Progress of ISO 21348
Heliosphere
- Pryor, et al AA 2024: Modeling Cassini UVIS Interplanetary Hydrogen Lyα Observations
- Pryor, et al AA 2008: Radiation transport of heliospheric Lyman-alpha
- Tobiska 2005 AIAA 2005-0069: A report on the development of a flare evolution model
- Gangopadhyay, et al 2005 APJ: Revision of Pioneer 10 and Voyager 2 data
- Pryor, et al JGR 2003: Hydrogen atom lifetimes in the three-dimensional heliosphere over the solar cycle
- Pryor, et al 1998 JGR: Studies of interplanetary Lyman-alpha over solar cycles 21-22 from Pioneer Venus
- Shemansky, et al JGR 1993b: Pioneer 10 and Voyager H Lyman-α observations suggest existence of termination shock between 70 and 105 AU upstream
- Pryor, et al 1992 APJ: Latitudinal variation of solar Lyman-α derived from Galileo UVS and Pioneer Venus Orbiter UV spectrometer observations
- Hord, et al Science 1991b: EUV Venus atmosphere spectrum and interplanetary H Ly-α observations by the Galileo UVS
- Sandel, et al Nature 1978: H Ly-α and Ly-β lines in the 500 to 1700 Å region from Voyager UVS observation
Mercury
- Killen, et al 2009 APJS: Solar photon scattering probabilities for discrete transitions in the 550–6000 Â region for 12 Mercury exosphere species, from MESSENGER UVVS data
- Shemansky and Morgan 1991 GRL: Possible role of solar activity in sourcing K and Na to the atmosphere
- Shemansky 1980 JGR: Comment on Monte Carlo simulation of lunar and Mercurian exospheres
- Smith, et al 1978 JGR: Monte Carlo model with Maxwell-Boltzmann flux source added to Maxwell-Boltzmann source
- Shemansky and Broadfoot 1977 RGSP: The assumption of thermal accommodation in gas-surface interactions may not be valid in exosphere model
- Broadfoot and Shemansky 1976 GRL: Mariner 10 observations of helium and hydrogen in the Mercury atmosphere
Earth
- Peterson, et al 2012 JGR: Solar energy derived from photoelectron observations
- Liu, et al 2009 JGR: Analysis and modeling of FUSE data
- Knipp, et al 2005 SP: Direct and Indirect Thermospheric Heating Sources for Solar Cycles 21–23
- Knipp, et al 2002 COSPAR: A comparative study of the auroral hemispheric power and the EUV hemispheric power over solar cycle time scales
- Tobiska, et al 1993 JGR: Analysis of E-2 payload on rocket during Energy Budget Campaign (1980)
- Hagan, et al 1992 JGR: A study of the thermosphere and ionosphere for solar minimum winter conditions.
- Shemansky and Broadfoot 1973 JGR: Comment on A 3Σu+ and B 3Πg states of N2
- Shemansky, et al 1972 PSS: Auroral emission model including secondary electrons
- Shemansky, et al 1971 PSS: Cascades from A 3Σu+ molecules account for recent rocket observations of aurora
- Shemansky and Jones 1968 PSS Observations of O2+ 1N and N2 1PG systems in type-B red aurora by scanning spectrometer
Moon
- Morgan and Shemansky 1991b JGR: Limits to the lunar atmosphere
Jupiter
Jupiter Systems
- Tobiska, et al 2007 SET TR: Galileo UV observations of H Lyman-alpha in Jupiter’s low latitude upper atmosphere
- Pryor, et al 2005 Icarus: Cassini UVIS observations of auroral H2and H Lyman-α emissions
- Gladstone, et al 2004 PSS: Constraints on Jupiter’s hydrogen corona from Galileo UVS observations
- Pryor, et al 2001 SSR: Remote Sensing of H from Ulysses and Galileo
- Ajello, et al 2001 Icarus: EUV and FUV auroral spectra from Galileo EUVS (540 — 1280 Å) and HUT (830 — 1850 Å) observations
- Clarke, et al 1998 JGR: Hubble imaging of Jupiter’s UV aurora during the Galileo mission
- Pryor, et al 1998 JGR: Galileo UVS spectrum from 1600 – – 3200 Å
- Ajello, et al 1998 JGR: Spectra from Galileo UVS (540 — 1280 Å) and EUVS (1130 — 4320 Å)
- Hord, et al 1992 SSR: Description of the Galileo Ultraviolet Spectrometer and planned observations at Jupiter
- Bagenal, et al 1992 GRL: Radial profile of O++ abundance between 4.0 and 42 RJ based on Voyager 1 data
- Shemansky and Judge 1988 JGR: Comparison of Voyager data with earlier Pioneer 10 and rocket observations
- Shemansky 1985 JGR: Mechanism for the H Ly-α bulge in EUV equatorial emission
- McConnell, et al 1982 PSS: Photochemical model with vertical transport of ions
- Brown and Shemansky 1982 APJ: Ion-ion and ion-atom reactions may determine the structure of Jupiter’s hot plasma torus
- Festou, et al 1981 JGR: Analysis of stellar occultation observed by Voyager 2
- Cook, et al 1981 JGR: Aurora in darkside Voyager I images at least partially attributed to lo torus aurora
- Broadfoot, et al 1981 JGR: Summary of Voyager UVS observations from the 1977 launch through the 25 March 1979 Jupiter encounter
- Sandel, et al 1979 Science: Voyager 2 encounter with Jupiter
- Broadfoot, et al 1979 Science: Voyager 1 encounter with Jupiter
- Broadfoot, et al 1977 SSR: Description of the Voyager Ultraviolet Spectrometer and planned observations
Jupiter Systems – Io
- Taylor, et al 1995 JGR: Model of EUV Io plasma torus emission developed using Voyager 1 in situ and remote observations
- Hall 1994 APJ: 370 to 735 Å spectrum from the Extreme Ultraviolet Explorer (EUVE)
- Schneider, et al 1991 Science: Sodium-bearing molecules interacting with the lo plasma torus may be the source of fast neutral sodium
- Shemansky 1988 JGR: Neutral cloud theory does not support observed ion partitioning
- Shemansky 1987 JGR: Model of collisional diffusive equilibrium in the lo plasma torus and comparison to Voyager UVS data
- Smyth and Shemansky 1983 APJ: Model of the escape of atomic oxygen from lo and its distribution in the Jupiter magnetosphere
- Brown, et al 1983 APJ: Effects of fast ion-ion and ion-atom reactions on chemistry in the Io plasma torus
- Shemansky and Sandel 1982 JGR: Electron-electron heating appears to be the dominant mechanism transporting energy to the plasma
- Shemansky 1980 APJ: Calculation of limits on ion mass-loading and diffusion-loss rates
- Shemansky 1980 APJ: Calculations of radiative cooling efficiencies and predicted line intensities for species in the torus
Jupiter Systems – Europa
- Hansen, et al 2005 Icarus: Cassini UVIS observes atomic oxygen atmosphere at Europa
Saturn
Saturn System
- Mitchell, et al 2005 GRL: Substorms may account for bursts of energetic neutral atoms from Saturn’s magnetotail
- Esposito, et al 2005 Science: Cassini UVIS observes evidence of rapid changes in the neutral oxygen population
- Esposito, et al 2004 SSR: Description of the Ultraviolet Imaging Spectrograph and planned observations at Saturn
- Blanc, et al 2002 SSR: Planned in-situ observations of the Saturn magnetosphere by Cassini-Huygens
- Shemansky, et al 1993 Nature: HST FOS observation of OH emission
- Shemansky and Hall 1992 JGR: Analysis of Voyager UVS observations suggests Saturn atomospher is the source of atomic hydrogen in the magnetosphere
- Yelle, et al 1986 JGR: Variation of line intensity with altitude derived from Voyager occultation observations
- Smith, et al 1983 JGR: Analysis of Voyager 2 solar and stellar occultations
- Sandel, et al 1982 Science: Voyager 2 encounter with Saturn
- Broadfoot, et al 1981 Science: Observations of the atmosphere, aurora, hydrogen torus, and Titan
Saturn System – Enceladus
- Hansen, et al 2006 Science: Cassini UVIS observation of the water vapor plume near the south pole of Enceladus
Saturn System – Titan
- Liang, et al 2007 APJ: Model of Titan atmosphere including aerosols
- Smith, et al 1982 JGR: Composition and thermal profile from Voyager 1 UVS solar occultation observation
- Strobel and Shemansky 1982 JGR: Voyager 1 encounter with Titan
Uranus
- Herbert, et al 1987 JGR: Composition and thermal profile from Voyager 2 UVS stellar occultations
- Broadfoot, et al 1986 Science: Analysis of Voyager UVS solar and stellar occultation data
- Shemansky and Smith 1986 GRL: Analysis of Voyager and IUE observations and implications for the escape of H I
Neptune
- Broadfoot, et al 1989 Science: Composition and thermal profiles based on Voyager UVS data
Comets
- Weaver, et al 2002 APJ: FUSE observations of the C/1999 T1 (McNaught-Hartley), C/2001 A2 (LINEAR), and C/2000 WM1 (LINEAR) comets
- Hord, et al 1995 GRL: Direct observations of the Comet Shoemaker-Levy 9 fragment G impact by Galileo UVS
- Hall and Shemansky 1988 Nature: Cometesimals are not needed to supply atomic hydrogen to the very local interstellar medium (VLISM)
Atomic and Molecular Physics
- Glass-Maujean, et al 2009 APJS: Extension of previous work which takes more higher Rydberg states into account and extends Cassini UVIS calibration from 920-1640 Å down to 800-1640 Å
- Kanik, et al 2003 JGR: Electron impact excitation functions and absolute emission cross sections for the OI 130.4 nm and 135.6 nm features
- Shemansky, et al 1995 APJ: Experimental MUV cross sections of the electron excited N2 second positive system
- Ajello and Shemansky 1993 APJ: Laboratory measurements of the electron excitation function from 11 to 60 eV for the H2(a 3Σg+ → b 3Σu+) continuum emission
- Smith, et al 1993 JGR: Experimental electron excitation cross sections and comparison to theory
- Ajello, et al 1991 APJ: Experimental cross sections for H(2p, 2s, 1s) production
- Tripp, et al 1991 APJ: Laboratory measurements of electron excited N2 and predicted excitation and emission properties for N II
- Ratliff, et al 1991 JGR: Experimental cross sections of the b 1Πustate
- Bashkin, et al 1991 PRA: Experimental cross sections from 320 to 800 nm
- James, et al 1990 JPB: EUV emission from electron impact in the 102 to 134 nm range
- Bashkin, et al 1989 NIMPRB: Experimental measurement of spectra from 320 to 800 nm
- Ajello, et al 1989 PRA: Experimental cross sections of the c4′1Σu+ and b′ 1Σu+ states
- Ajello, et al 1988 AO: Electron impact laboratory VUV source
- James, et al 1988 JGR: Experimental measurement of O2spectrum produced by 200 eV electron impact from 115 to 300 nm
- Pang, et al 1987 JCP: Experimental cross sections and spectra from 40 to 200 nm for electron impact emission from methane and acetylene
- Shemansky, et al 1985 APJ: Reexamination of H Ly-α cross section by two methods
- Shemansky, et al 1985 APJ: Experimental electron excitation cross sections for He Rydberg series emission
- Ajello, et al 1985 JGR: FUV (120 — 210 nm) spectrum and cross sections for electron-excited N2
- Kunc and Shemansky 1985 SS: Monte Carlo model of interaction between He and α-quartz
- Kunc, et al 1984 LPB: Model of EUV emission from hydrogen glow discharge
- Ajello, et al 1984 PRA: Experimental electron excitation cross sections for H2 Rydberg series EUV emission
- Shemansky and Ajello 1983 JGR: Higher Rydberg series bands make a significant contribution to the EUV emission spectrum
- Shemansky 1976 JCP: The N2 A 3Σu+ state as precursor for afterglow
- Wu and Shemansky 1976 JCP: Electronic transition moment as a function of mean internuclear distance and experimental spectra
- Shemansky 1972 JCP: Laboratory measurement of extinction coefficient in the 1700 to 3000 A region
- Shemansky and Broadfoot 1971 JQSRT: Laboratory measurements of transition probabilities, excitation cross-sections, and afterglow effects of electron excited N2 1P, 2P, and N2+ systems
- Shemansky and Broadfoot 1971 JQSRT: Laboratory measurements of transition probabilities, excitation cross-sections, and afterglow effects of electron excited N2 1P, 2P, and N2+ systems
- Shemansky 1969 JCP: Calculations of band transition probabilities, lifetimes, and collision self-broadening cross section
- Shemansky and Carleton 1969 JCP: Reanalysis of experimental lifetime
- Shemansky 1969 JCP: Experimental absorption spectrum and transition probabilities
Other
- Haisch, et al 1998 SPIE: Proposed 2.4-meter GEO telescope for outer planets and comets observations
- Robb, et al 1997 SPIE: Proposed low-cost, GEO 140-cm telescope with UV instruments
- Holberg, et al 1982 APJ: Absolute fluxes from hot star observations and comparison with other Voyager observations
- Shemansky, et al 1979 APJ: 600 — 1700 Å spectrum from Voyager 2 UVS observations
- Sandel, et al 1979 APJ: Spectrum from 750 — 1200 Å measured by Voyager UVS
- Shemansky, et al 1979 JGR: Voyager UVS (500 to 1700 Å) observations of ISM
- Sandel, et al 1977 AO: Microchannel plate performance tests
