Letters announcing the results of the competition for new Fiscal Year (FY) 1996 awards from the SR&T and Suborbital Program in Solar Physics were mailed to Principal Investigators in March 1996. These awards were made on the basis of proposals submitted in response to NASA Research Announcement NRA-95-OSS-11. FY 1996 Supporting Research and Technology (SR&T) funding approximately matches that of FY 1995, at $6.2 M. The Suborbital Program budget was augmented about five per cent to $3.6 M. The selections were based on these budgets.
Proposals describing 84 investigations (including five Suborbital) were received in the competition for FY 1996 funding from the Solar Physics program. These were rated in a peer review of their scientific merit. The total FY 1996 funding requested was $8.2 M and the funding available for competition was $3.5 M (including $0.6 M in Suborbital). The assignment of ratings was based on requirements set out in the NRA. Selection for funding from among scientifically competitive proposals is typically based on a combination of programmatic, budgetary and operational considerations. The available funding proved sufficient to allow selection of 37 proposals, 35 of which were the highest ranked by peer review. All selected proposals were funded at the levels recommended by the review panels; in only two cases was this level less than requested by the proposer.
The next opportunity to propose for Solar Physics funding will be in response to the 1996 NRA for the Sun-Earth Connections Supporting Research and Technology and Suborbital Program, which was released May 20, 1996. This NRA is now available on the Web at:
A list of the proposals selected for FY 1996 is appended. A full list of the Solar Physics investigations which are being supported in FY 1996 will be posted in the future.
Solar Physics SR&T Program Investigations Selected for Initiation in FY 1996:
Aschwanden/U of MD
Electron Time-of-Flight Kinematics in Solar Flares
Antiochos/NRL
Physics of the Solar Corona and Transition Region
Avrett/SAO
Basic Modeling of the Solar Atmosphere and Spectrum
Bagenal/U of CO
Evolution and Activity in the Solar Corona: A comparison of
Coronal and Chromospheric Structures Seen in Soft X-Rays,
White Light & Emission Lines
Bhatia/GSFC
Modelling the Effects of Optical Depth on Solar Active Region
and Flare Diagnostics
Birn/LANL
Modeling of Three-Dimensional Reconnection Related to
Coronal Eruption and Ejection Processes
Brosius/Hughes/STX
Solar Coronal Plasma Properties of Active Regions, Quiet
Sun Areas, and a Polar Coronal Hole from SERTS EUV Spectra
and Images
Bruner/L-MPARL
Solar Coronal Structure Study
Canfield/MT State U
Magnetic Helicity and the Solar Dynamo
Chutjian/JPL
Measurement of Absolute Electron-Ion Collision Cross
Sections for Solar Plasma Diagnostics
DeLuca/SAO
Chinks in Solar Dynamo Theory: Turbulent Diffusion,
Dynamo Waves & Magnetic Helicity
Emslie/U AL-H
Diagnostics of Mass Motions in Solar Flares
Esser/SAO
Mapping the Solar Wind from its Source Region into the
Outer Corona
Fisher, G./UCB
The Interrelation of Soft and Hard X-ray Emission During
Solar Flares
Fisher, G./UCB
Large Scale Currents as a Coronal Heating Source
Gary/MSFC
Analysis and Properties of Magnetic and Electric Current
Systems in Solar Active Regions
Hoyt/Hughes/STX
Additional Work on the Reconstruction of Solar Activity,
1610 - 1994
Huba/NRL
Ion-Neutral Dynamics in the Solar Chromosphere: First
Ionization Potential Fractionation
Krieger/Rad Sci
Development of a Focussing Hard X-Ray Telescope:
Preliminary Design of a Wolter Type I Hard X-Ray Telescope
Lang/Tufts U
Radio Studies of the Solar Corona in Support of NASA Missions
Lean/NRL
Co-Temporal Evolution of Magnetic Variability Structures in
the Global Corona, Chromosphere and Photosphere
Mariska/NRL
Solar Flare Looptop Emission
McAllister/Helio Res
X-Ray Structures in and Around Filament Channels
McConnell/U NH
The Development of a Solar Flare Hard X-Ray/Gamma-Ray
Polarimeter
Miller/U AL-H
Electron Acceleration in Impulsive Solar Flares
Ryan/U NH
Demonstration of SONTRAC Principles: A Solar Neutron
Track Chamber Telescope
Share/NRL
Gamma-Ray Spectroscopy of Flares in Cycles 21 and 22
Sheeley/NRL
Magnetic Fields, the Corona, and the Solar Wind
Stein/MI SU
Solar Convection and Atmospheric Dynamics
Title/L-MPARL
Michelson Vector Magnetograph for Solar Lite
Thomas, J./U Roch
Sunspot Dynamics
Vestrand/U NH
New Technology CdZnTe Detectors for High-Energy Flare
Spectroscopy: The Room Temperature Semiconductor
Spectrometer for JAWSAT
Webb/Bos Col
Study of Disconnection of Magnetic Fields Associated with
Coronal Mass Ejections
Wolfson/Middlebury Col
Coronal Mass Ejections and Large-Scale Evolution of the
Solar Corona
Woo/JPL
Probing Coronal Structures with Radio Propagation
Measurements
***
Solar Physics Suborbital Program Investigations Selected for
Initiation in FY 1996:
Golub/SAO
Global Corona Structure Investigation
Hassler/NCAR
Coronal Helium Imager and Abundance Experiment
Rust/JHU-APL
Solar Activity Research with the Flare Genesis Telescope
FINDINGS OF THE SOLAR PHYSICS MOWG--December 1994
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