Mathematical and Physical Sciences


Programs in the Mathematical and Physical Sciences (MPS) Directorate are designed with the following goals: To help the programs meet these goals, the directorate encourages collaborations with other NSF directorates, other agencies, and industrial organizations.

Support for research and education in the mathematical and physical sciences can take many forms.

The operational activities of MPS are organized around divisional and disciplinary lines that cover Astronomical Sciences, Chemistry, Materials Research, Mathematical Sciences, and Physics. However, MPS recognizes that "Nature knows no boundaries." MPS emphasizes communication among the divisions and across directorate boundaries to ensure effective support of research and education projects in emerging fields that cut across those lines. By contacting any of the programs or divisions of MPS related to their work, potential proposers can gain information and access to a full range of opportunities open to them.

MPS is an active participant in a number of inter- and intraagency areas that are focused on interdisciplinary areas of importance to the national interest. These include the Advanced Materials and Processing Program; Biotechnology; the U.S. Global Change Research Program; Environment; High Performance Computing and Communications; Advanced Manufacturing Technologies; Civil Infrastructure Systems; and Science, Mathematics, Engineering, and Technology Education. Researchers and educators interested in exploring opportunities in these areas should contact the division most closely related to their own interests to determine the best mechanism for submitting proposals.

For More Information
For further information, contact the appropriate Division Director, National Science Foundation, 4201 Wilson Boulevard, Arlington, Virginia 22230.

Astronomical Sciences

Areas of Research The overall objective of the Astronomical Sciences Division is to increase our knowledge of the universe. Research is aimed at determining the composition, structure, and evolution of planets, stars, and galaxies, including our sun and the Milky Way.

In addition to providing research grants, NSF supports the development and operation of three National Astronomy Centers, where radio, optical, infrared, and special telescopes are made available on a competitive basis to the scientific community. Resident staff at the centers give technical assistance to visiting scientists, conduct studies of their own, and develop advanced instrumentation. Astronomical Sciences also supports the Center for Particle Astrophysics, an NSF Science and Technology Center. These centers meet national needs for research in specific areas of science requiring facilities, equipment, staffing, and operational support that could not appropriately be offered by a single institution.

ASTRONOMY PROJECTS

The program of Astronomy and Astrophysics Research Projects provides a broad base for support of fundamental research aimed at an understanding of the states of matter and physical processes in the solar system, our Milky Way galaxy, and the origin and evolution of the present universe. Proposals to support searches for extraterrestrial intelligence are not supported in the program.

Deadlines
Stellar Astronomy and Astrophysics has a deadline of May 15, 1995, for research to be done commencing on or after October 1, 1995. Proposals for research in other areas by individual investigators should preferably be submitted in the spring or early summer. Proposers are urged to contact a program officer in advance of submitting a proposal to any of the programs.

For More Information
For further information, contact the Division of Astronomical Sciences, National Science Foundation, Arlington, Virginia 22230, (703) 306-1820.

Areas of Research

NATIONAL ASTRONOMY AND IONOSPHERE CENTER

NSF supports the National Astronomy and Ionosphere Center (NAIC), a visitor-oriented national research center devoted to researching radio and radar astronomy and atmospheric sciences. NAIC is operated and managed for NSF by Cornell University. NAIC headquarters are in Ithaca, New York, and its principal observing facilities are 19 kilometers south of the city of Arecibo, Puerto Rico.

NAIC provides telescope users with a wide range of research and observing instrumentation, including receivers, transmitters, movable line feeds, and digital data acquisition and processing equipment. The center has a permanent staff of scientists, engineers, and technicians who are available to help visiting investigators with their observing programs.

NAIC's principal astronomical research instrument is a 305-meter, fixed spherical radio/radar telescope--the world's largest single radio reflector. Its frequency capabilities range from 50 megahertz to 5 gigahertz. Transmitters include an S-band (2,380-megahertz) radar system for planetary studies and a 430- megahertz radar system for aeronomy studies. A second observing site, located 9.6 kilometers from the main site, has a 30.5-meter steerable parabolic antenna and is paired with the main antenna to provide an effective interferometric S-band radar mapping system. This antenna pair is also available for radio astronomy interferometry at a wavelength of 12 centimeters.

The S-Band Planetary Radar System is now available for high-spatial-resolution studies of stratospheric dynamics. A high-power ionospheric heating facility provides a unique capability to investigate nonlinear plasma phenomena in the ionosphere.

A major three-phase upgrade of NAIC's main antenna facility is presently under way. First, a large reflecting screen is being erected around the periphery of the 305-meter reflector to reduce the effect of scattered ground radiation on the observations. Second, a pair of wide- band aberration-correcting reflectors are being installed to replace the line feeds above around 250 megahertz. Finally, the power of the S-band radar system is being doubled. Completion of the upgrade is expected in 1996.

Eligibility
NAIC facilities and instrumentation are available on a competitive basis to qualified scientists from all over the world. Telescope time is assigned after judgment of research proposals on the basis of scientific merit, the capability of the instruments to do the work, and available telescope time.

For More Information
For further information, contact the Director, National Astronomy and Ionosphere Center, Cornell University, Ithaca, New York 14853.

GEMINI 8-METER TELESCOPES

The Gemini 8-Meter Telescopes Project is an international undertaking that will provide astronomers of the partner countries (United States, United Kingdom, Canada, Chile, Brazil, and Argentina) with 8-meter telescopes in the northern hemisphere on Mauna Kea, Hawaii, and in the southern hemisphere on Cerro Pachon, in Chile. The Mauna Kea telescope will be infrared optimized and have superb image quality. The Chilean telescope will be its near twin. NSF acts as the executive agency for the partnership, and the Association of Universities for Research in Astronomy, Inc. (AURA), a consortium of 20 major universities, is managing the construction of the telescopes.

When operational (approximately 1998 on Mauna Kea and 2000 in Chile), these telescopes will provide astronomers of the partner countries with world-class observing facilities. Observing time will be assigned on the basis of scientific merit.

NATIONAL OPTICAL ASTRONOMY OBSERVATORIES

NSF supports the National Optical Astronomy Observatories (NOAO), the national center for research in ground-based optical and infrared astronomy and solar physics. Large optical telescopes, observing instrumentation, and data analysis equipment are made available to qualified visiting scientists. The NOAO staff of astronomers, engineers, and various support personnel is available to assist visiting scientists in their use of the facilities.

The headquarters of NOAO are in Tucson, Arizona. NOAO includes the Kitt Peak National Observatory (KPNO), the Cerro Tololo Inter-American Observatory (CTIO), and the National Solar Observatory (NSO). NOAO is operated and managed by AURA.

The observing facilities of KPNO are located on Kitt Peak, a 2,089-meter mountain 90 kilometers southwest of Tucson. The facilities include the 4-meter Mayall Telescope, a 2.1- meter general-purpose reflector, a 92- centimeter coudĒ feed (associated with the 2.1- meter), a 1.3-meter reflector instrumented for the infrared, and the Burrell Schmidt Telescope of Case Western University. A full complement of state-of-the-art spectroscopic, photometric, and imaging instrumentation is available for use on these telescopes.

CTIO provides qualified scientists with telescopes and related facilities for astronomical research in the southern hemisphere. CTIO has offices, laboratories, and living quarters in the coastal city of La Serena, Chile, about 482 kilometers north of Santiago, Chile. The observing facilities are located on Cerro Tololo, a 2,194-meter mountain on the western slopes of the Andes, about 64 kilometers inland from La Serena.

CTIO operates six telescopes, including the 4- meter, a near twin to the Kitt Peak 4-meter. Other telescopes are the 1.5-meter, 0.91-meter, 0.61-meter reflector, a Schmidt telescope on loan from the University of Michigan, and a 1- meter reflector on loan from Yale. These telescopes are equipped with instruments similar to those at KPNO.

NSO is devoted to research in the fields of solar physics, solar-terrestrial relationships, and related areas. NSO makes available the world's largest collection of modern optical solar telescopes and auxiliary instrumentation designed to observe the solar photosphere, chromosphere, and corona.

NSO has observing facilities atop Kitt Peak, Arizona (NSO/KP), and Sacramento Peak, New Mexico (NSO/SP). The Kitt Peak facilities consist of the 1.5-meter McMath-Pierce Solar Telescope--the world's largest solar research instrument--and a solar vacuum telescope/magnetograph. The McMath complex, designed primarily for solar observations, is also used for planetary and stellar observations and for laboratory high- resolution spectroscopy.

NSO/SP is located in Sunspot, New Mexico, at an elevation of 2,800 meters on a crest of the Sacramento Mountains. The principal instruments are the 0.76-meter aperture Solar Vacuum Tower Telescope, equipped with spectrographs, optical benches, and the Advanced Stokes Polarimeter; and the Evans Solar Facility, equipped with a 40-centimeter aperture coronagraph, spectrographs, and a coronal photometer.

Eligibility
The NOAO facilities and instrumentation are available on a competitive basis to all qualified U.S. scientists and, on occasion, foreign visitors. Telescope time is assigned on the basis of scientific merit, the capability of the instruments to do the work, and the available telescope time.

For More Information
For further information, contact the Director, National Optical Astronomy Observatories, P.O. Box 26732, Tucson, Arizona 85726.

NATIONAL RADIO ASTRONOMY OBSERVATORY

NSF supports the National Radio Astronomy Observatory (NRAO), which makes radio astronomy facilities available to qualified scientists. The NRAO staff helps visiting scientists use the large radio antennas, receivers, and other equipment needed to detect, measure, and identify radio waves from astronomical objects.

Headquarters for NRAO are in Charlottesville, Virginia. Observing sites are located in Green Bank, West Virginia; Kitt Peak near Tucson, Arizona; a site 80 kilometers west of Socorro, New Mexico; and 10 sites in the continental United States and the islands of Hawaii and St. Croix, where the individual antennas of the Very-Long-Baseline Array (VLBA) are located. NRAO is supported under the terms of a cooperative agreement between NSF and Associated Universities, Inc. (AUI), the organization responsible for the operation and management of the observatory.

Only one telescope is currently operated at the Green Bank site. It is a 43-meter aperture instrument, which permits the study of spectral lines at centimeter wave lengths and is an integral part of the Very-Long-Baseline- Interferometer network. This network is involved in studies of quasars and the high- resolution mapping of galactic objects based on simultaneous observations by combinations of telescopes over transcontinental and intercontinental distances. Currently under construction at Green Bank is a 100-meter telescope expected to be fully operational in 1995, at which time the 43-meter telescope will be retired.

A 12-meter millimeter-wavelength telescope is located on Kitt Peak to take advantage of the high altitude and dry climate necessary for short radio wavelengths. This telescope is capable of both continuum and spectral-line studies at wavelengths from 1 centimeter to as short as 1 millimeter.

The Very Large Array (VLA) west of Socorro, New Mexico, consists of 27 antennas, available for use in an interferometric mode for aperture synthesis observations of faint radio sources. Both continuum and spectral-line observations at wavelengths of 1.3, 2, 6, and 20 centimeters can be made. The VLBA operates on the basis of the same physical principles as the VLA but, because of the much larger distances between antennas, the data are recorded at each site and compared later at Socorro, New Mexico. Because of its larger antenna separation, the VLBA is capable of resolving much smaller details in astronomical sources than is the VLA.

Eligibility
NRAO makes observing time on each instrument available for the use of all qualified U.S. scientists and, on occasion, foreign visitors. Telescope time is assigned after judgment of research proposals on the basis of scientific merit, the capability of the instruments to do the work, and the available telescope time.

For More Information
For further information, contact the Director, National Radio Astronomy Observatory, Edgemont Road, Charlottesville, Virginia 22903.

Mathematical Sciences

The Division of Mathematical Sciences (DMS) supports a wide range of projects aimed at developing and exploring the properties and applications of mathematical structures. Most of these projects represent the research programs of single investigators or small groups of investigators working with graduate students and postdoctoral researchers. The Mathematical Sciences Infrastructure Program and the Special Projects Program handle a variety of different activities falling outside this mode.

The following three activities cut across all disciplinary programs.

Deadlines
The division will continue to have two target dates for proposals submitted to the following programs.

October 12, 1994:
Algebra and Number Theory Program
Applied Mathematics Program
Classical Analysis Program
Modern Analysis Program

November 9, 1994:
Computational Mathematics Program
Geometric Analysis Program
Statistics and Probability Program
Topology and Foundations Program
The above dates do not apply to the activities of the Mathematical Sciences Infrastructure Program or the Special Projects Program; most of these activities have specified target or deadline dates.

For More Information
For further information, contact the Division of Mathematical Sciences, National Science Foundation, 4201 Wilson Boulevard, Arlington, Virginia 22230, (703) 306-1870.

Each applicant will be required to submit a research plan for the tenure period requested. The fellowships are not intended to support the preparation of prior research results for publication or the writing of textbooks. Deadline for submission is October 15, 1994.

The postdoctoral activities will also include a university-industry cooperative postdoctoral program with 10 or more awards. In fiscal year 1995, it is anticipated that the university- industry program will be expanded to include sabbatical support for mid-career scientists and graduate assistantships and internships. Submission deadline for the university-industry activities is anticipated to be in mid-December, 1994.

For More Information
For further information, contact the Program Officer, Office of Special Projects, Mathematical Sciences Division, National Science Foundation, 4201 Wilson Boulevard, Arlington, Virginia 22230, (703) 306-1883.

Physics

The Division of Physics (PHY) supports wide-ranging programs in the areas of Atomic, Molecular, and Optical Physics; Elementary Particle Physics; Gravitational Physics; Nuclear Physics; and Theoretical Physics. Among these programs, which for the most part support individual investigators and small groups, the division operates a few large-scale facilities. These include the Cornell Electron Storage Ring (CESR), the Indiana University Cyclotron Facility (IUCF), and the Michigan State University National Superconducting Cyclotron Laboratory (NSCL). In addition, the Laser Interferometer Gravity Wave Observatory (LIGO) is being constructed under the supervision of PHY. The division also operates several smaller centers specializing in optical physics and in various aspects of theoretical physics. Programs in Elementary Particle Physics and Nuclear Physics benefit greatly from the use of the large accelerator facilities constructed by the Department of Energy.

Recently the division, in cooperation with other divisions in MPS, began small-scale initiatives in Biological Physics and in Particle Astrophysics.

The research activities of the division are inextricably linked to education. On the graduate level, it supports about 1,000 students who are fully engaged in research programs. In addition, these programs involve substantial numbers of undergraduates, especially in the summer activities that are centered around the Research Experiences for Undergraduates Program. Research activities at four-year colleges are supported through the Research at Undergraduate Institutions Program. Significant training of young people also occurs through the support of about 500 postdoctoral fellowships.<

Chemistry

The Chemistry Division supports research activities and research infrastructure development in most of the principal subdisciplines of the chemical sciences. However, support is also available from the Divisions of Atmospheric Sciences (atmospheric chemistry), Molecular and Cellular Biosciences (biochemistry, biophysics), Chemical and Transport Systems (chemical engineering), Earth Sciences (geochemistry), and Materials Research (solid-state and polymer science).

The Chemistry Division supports research activities in emerging areas of national interest that cut across "traditional" subdisciplines. These areas include biological chemistry and biotechnology; the chemistry of advanced materials; environmental chemistry, including research in greenhouse gas dynamics and the program in Environmentally Benign Chemical Synthesis and Processing jointly supported with the Engineering Directorate (see brochure NSF 92-13 for more information); high performance computing and communications; and advanced manufacturing, including fundamental research underpinning chemical and pharmaceutical manufacture. Many of these activities are part of research programs that are coordinated through the National Science and Technology Council.

Research in subdisciplinary areas is also a vital part of the Chemistry Research Project Support investment portfolio. These areas include the following:

Much of the Chemistry Division's support of instrumentation and infrastructure is coordinated through the Office of Special Projects. Among these activities is a program of portable Postdoctoral Research Fellowships in Chemistry (see brochure NSF 93-91 for more information); a nationwide network of 60 sites for Research Experiences for Undergraduates (see brochure NSF 93-112 for more information); Research Planning Grants for women and minorities; grants for Faculty Early Career Development; and occasional grants for special purposes in education, curriculum development, and graduate training.

Equally important infrastructure and instrumentation investments, made in the Chemical Instrumentation and Facilities Program (see brochure NSF 93-94 for more information), provide funds to research institutions and consortia thereof for the purchase of multiuser instruments, for major instrumentation development and construction, and for the establishment and support of multiuser research facilities in the chemical sciences. This program is designed to support the following types of academic instrumentation needs: (1) the purchase or upgrade of shared, multiuser instruments (requires a one-third to one-half cost contribution from the grantee institution); (2) the development plans for Chemistry Departments' multiyear instrument centers; (3) instrumentation development, including the construction of new prototype instruments; and (4) the establishment and support of unique national and regional instrumentation facilities. This program focuses on shared instruments and facilities; specialized equipment dedicated for use in particular chemistry research projects is funded as part of individual investigator awards, along with personnel and other direct project costs in other Chemistry Division programs.

Materials Research

The Division of Materials Research (DMR) supports a wide range of programs that address fundamental phenomena in materials, materials synthesis and processing, materials structure and composition, materials properties and performance, and materials education. Formal research program areas include Condensed Matter Physics; Solid-State Chemistry and Polymers; Metals, Ceramics, and Electronic Materials; Materials Theory; and Materials Research Science and Engineering Centers. Investments in research infrastructure in materials science are also made through the National Facilities and Instrumentation Program.

DMR plays a significant role in various broad, interdisciplinary areas and programs, including the Advanced Materials and Processing Program (AMPP), High Performance Computing and Communications (HPCC), and Advanced Manufacturing Technology (AMT). DMR is also a participant in the Biotechnology, Civil Infrastructure Systems, and Environmental Research Initiatives. The division's interest in HPCC ranges from computational approaches to real materials and processes to materials for new or advanced computational and communications devices and systems. In AMT, the division's interests range from the understanding of the fundamental materials science basis of phenomena (e.g., lubrication, adhesion, joining, forming, packaging) that broadly crosscuts strategically significant industrial sectors, to materials for specific manufacturing processes and applications. In addition to the impact of materials on manufacturing, the division also has an interest in the impact of advanced manufacturing technologies on materials research (e.g., through the cost-effective enhancement of the instrumentation and equipment infrastructure for materials research). In Environmental Research, the division is concerned with the preparation of innovative materials and with new processes that are more environmentally benign, as well as with novel concepts for reuse or recycling of materials.

DMR funding modes include support for individual investigators, groups, centers, national facilities, and instrumentation. Individual investigator proposals need not be confined or targeted to a specific program. Division staff and management will work to facilitate the co-funding of highly meritorious proposals across appropriate program, division, or directorate boundaries.

For More Information
For further information, contact the National Facilities as follows:
Center for High-Resolution Electron Microscopy
Center for Solid-State Science
Arizona State University
Tempe, Arizona 85287-1704
(602) 965-4540

Center for High-Resolution Neutron Scattering
National Institute of Standards and Technology
Reactor Radiation Division
Gaithersburg, Maryland 20899
(301) 975-6242

Cornell High-Energy Synchrotron Source
Wilson Laboratory
Cornell University
Ithaca, New York 14853
(607) 255-7163

Francis Bitter National Magnet Laboratory
Massachusetts Institute of Technology
170 Albany Street
Cambridge, Massachusetts 02139
(617) 253-5517

National High Magnetic Field Laboratory (under development--operated by Florida State University, University of Florida, and Los Alamos National Laboratory)
Florida State University
1800 E. Paul Dirac Drive
Tallahassee, Florida 32306-4005
(904) 644-0311

Synchrotron Radiation Center
University of Wisconsin-Madison
3731 Schneider Drive
Stoughton, Wisconsin 53589-2200
(608) 873-2000
Footnote
The term "national of the United States" designates a citizen of the United States or a permanent resident of a possession of the United States (such as American Samoa). It does not refer to a citizen of another country who has applied for U.S. citizenship.


Return to Guide to Programs Table of Contents