Vol. 2 No. 2 - September 2002 | Executive Editor: Dr.
Francis Cucinotta | Contributing Editor: Kay
Nute
NASA Announces Opportunities for Space Radiation Research
On August 30, 2002 NASA's Office of Biological and
Physical Research (OBPR) announced new opportunities for Ground-based
Research in Space Radiation Biology and Space Radiation Shielding
Materials (NRA 02-OBPR-02). Access to application materials and guidelines
for submittal of proposals can be obtained from:
Proposals are due to OBPR on November 25, 2002.
These new grants are anticipated for funding in fiscal
year 2003. The focus of the new NASA Research Announcement (NRA) in Space
Radiation Biology is to solicit research investigations that will support
the first use of the Booster
Application Facility (BAF) at Brookhaven
National Laboratory in 2003. There are seven areas of research that
are emphasized in the NRA:
Space Radiation Health Investigators' Workshop - 2003
The 14th Annual NASA
Space Radiation Health Investigators' Workshop is now scheduled for April
27th (Sunday) through April 30th (Wednesday), 2003. The workshop will be held
at South
Shore Harbour Resort and Conference Center, League City, Texas.
![]()
The scientific committee for the 14th Annual Workshop is: Dr. Francis A. Cucinotta,
NASA Johnson Space Center; Prof. John F. Dicello, Johns Hopkins
University; Dr. Amy Kronenberg, Lawrence Berkeley National
Laboratory; Dr. Greg D. Nelson, Loma Linda University Medical
Center; Dr. Walter Schimmerling, NASA Headquarters; Dr. Michael
D. Story, University of Texas M. D. Anderson Cancer Center; Dr.
Betsy M. Sutherland, Brookhaven National Laboratories; and Dr.
Elizabeth L. Travis, University of Texas M. D. Anderson Cancer
Center. As the scientific committee finalizes the program schedule and
other details, more information will be made available via the SRHP
Website.
2002 NASA Radiation Health Research Grants - Awarded
NASA's Office of Biological and Physical Research (OBPR)
has awarded four new research grants that will support the health and
safety concerns for future human space flight in the area of radiation
damage to biological systems. The four research grants were awarded
to Dr. Aloke Chatterjee of Lawrence Berkeley National Laboratory, Dr.
Lora Green of Loma Linda University, Dr. James Reuben of the University
of Texas M.D. Anderson Cancer Research Center, and Dr. Bjorn Rydberg
of Lawrence Berkeley National Laboratory.
Critical Path Roadmap in Space Radiation Health Research
A useful guide for research proposals is the OBPR
Bioastronautics Programs Critical Path Roadmap, which supports research in
the life sciences aimed at the human exploration of space. The Critical
Path Roadmap Mission Statement is
Figure 1 shows the current CPR in the area of Space
Radiation Health. In support of the CPR for each life science area,
Critical Questions for research and technology efforts needed to further
assess the risk and address its mitigation have been developed. The
current CPR in Space Radiation Health can be viewed on-line at http://bioastroroadmap.nasa.gov/User/discipline.jsp?filterDisciplines=11.
Each radiation risk has an associated set of core questions. The current Critical Questions in radiation are:
As researchers make progress including scientific
breakthroughs, it is important to revise the Critical Questions related to
each risk area. In 2003 a revision of the CPR questions in radiation is
expected to occur and will be reviewed at the 14th Annual Space Radiation Health Investigators
Meeting. Suggestions for CPR questions can be emailed to the SRHP Web
site.
Radiation Shielding on the International Space Station: Topology and Material Selection
Are traditional approaches to radiation shielding effective
against space radiation? NASA researchers have identified some key differences
including in the areas of material selection and topology, which are
leading to improvements
for ISS and new design processes
for exploration. Figure 2 shows the application of CAD models of
the ISS to project the amounts of shielding received by astronauts during
space walks including detailed models of the shielding provided by the
space suit and human body. The use of improved hydrogen-rich materials
such as polyethylene or water reduce the GCR (including secondary radiation
such as neutrons) dose equivalent by 20-30% and by a larger amount for
trapped protons and solar particle events. However, practical amounts
of any material is limited in how much dose reduction can be acheived
from the highly penetrating GCR. A second approach for reducing space
radiation effects on ISS is to optimize topology. Here since astronauts
spend over one-half of their day in common areas such as the sleep stations,
galley, and exercise areas, insuring the optimal topology for common
areas provide a significant benefit.
Figure 3 shows measurements by the Space Radiation Analysis Group (SRAG) at Johnson Space Center from the first four ISS Increments that illustrate the variations in dose due to topology. A range of variation >50% is observed. Critical issues in understanding variations inside spacecraft are the directionality issues related to source particles such as the trapped particles pitch angle distribution and the role of the Earth's shadow on GCR exposures, as well as the variation caused by the vehicle geometry. These results suggest that the combined use of optimal shielding materials and the topology of common areas will be the most effective method to reduce radiation exposures in space in the future. Data and methods developed for the ISS is providing valuable lessons and insights for the design of future spacecraft exploring the moon or Mars.
MARIE Updates Solar Particle Events on the Far Side of the SunThe Martian Radiation Environment Experiment (MARIE)
continues to provide valuable data on the space radiation environment at
Mars. The MARIE experiment is a NASA JSC experiment, led by Dr. Cary
Zeitlin, Principle Investigator from the NSBRI, and Lawrence Berkeley
National Laboratory. In recent months, MARIE has observed several Solar
Particle Events (SPE) including ones from the far side of the Sun. During
April 25th, Mars and Earth were 106
degrees apart with respect to Sun, and the solar disk that is visible from
the Mars is different from the one that is visible from earth. Figure 4
shows the increase in dose-rate at Mars measured by MARIE from the SPE of
April 25, 2002. The MARIE team has been developing procedures and
algorithms to make predictions of the solar disk activities on the far
side of the Sun. Data from the SOHO spacecraft are mapped to 3D views of
the Sun and the solar disk that is visible from Mars is obtained to
identify the solar activity that is likely to have connection to Mars.
Images of the solar disks for April 25th
are shown in Figure 5. On August 11, 2002, the Earth, Sun, and Mars were
in conjunction with Mars opposite to the Sun with respect to the Earth.
The opportunity to collect data on SPE's in this exciting period of
Mars-Earth phasing relative to the Sun should prove valuable in preparing
for future human exploration plans.
SRHP Featured Investigator: John F. Dicello, Ph. D.
Dr. Dicello has been with Johns Hopkins University
School of Medicine as Professor of Oncology in the Division of Radiation
Oncology since 1995. Prior appointments of Dr. Dicello include: professor
of physics with Clarkson University, NY (1982-1995); teaching faculty with
the University of New Mexico - Los Alamos, NM, Campus (1981-1982);
research scientist in the biomedical group with the Los Alamos National
Laboratory of the University of California (1973-1982); and faculty member
with the College of Physicians & Surgeons of Columbia University, NY
(1967-1973). Dr. Dicello received his B.S. degree in Physics from St.
Bonaventure University, NY (1960), M.S. degree in Physics from the
University of Pittsburgh, PA (1962), and Ph. D. degree from the Texas
A&M University in Physics (1968).
Dr. Dicello has been involved in three research areas: radiation therapy, cancer research, and microdosimetry. He began his career in medical physics at Columbia College of Physicians and Surgeons shortly after completing his Ph. D. at Columbia University. Dr. Dicello was as member of the group under the direction of Prof. H. H. Rossi credited with developing the field of microdosimetry. Microdosimetry is the study of energy transfers in matter at micro and sub micrometer levels, and it has found major applications in radiation biophysics and electronics. Dr. Dicello was one of the first researchers to recognize that significant errors in microelectronics were being produced because of microdosimetric effects and was subsequently funded by the Air Force to examine error rates in microelectronics from environmental mesons. He served as a principal investigator for a subcontract from an NIH (National Institute of Health) and AAPM (American Association of Physicists in Medicine) supported dosimetric inter-comparison among research institutions engaged in human trials using protons and heavier ions for radiation therapy. Dr. Dicello was the member of the team at Columbia that was responsible for the first dosimetric and biological measurements of the therapeutic potential of energetic heavy ions. Also, he served as a member of the biomedical group at the Los Alamos National Laboratory (LANL) that carried out first human studies with energetic pion beams. Dr. Dicello served as a consultant to the Loma Linda University for the design and construction of the first clinical based proton therapy facility and collaborated with Fermi National Laboratory for the pre-clinical data to design its neutron therapy facility. Apart from his teaching, research, and executive responsibilities with the Johns Hopkins University School of Medicine, Dr. Dicello has been contributing to the radiation community as a:
Prof. Dicello is currently the Leader of the Radiation-Effects Team of the National Space Biomedical Research Institute (NSBRI), Baylor College of Medicine - Houston, Texas. The research of this team presently includes six projects:
Prof. Dicello comments on his current research investigations that -
"During extended space travel, humans, particularly those going to
Mars, are continuously exposed to unusual and intense radiation fields. As
a result, there is the possibility of biological consequences. Our
research investigations focus on evaluating the health risks from these
radiation particles. Once we establish those risks adequately, we may be
able to develop better physical countermeasures such as structural changes
to the spacecraft to reduce the radiation levels to the astronauts.
Finally, we hope to find pharmaceutical approaches to reduce the risk from
these radiation exposures."Selected Research Publications
Selected Book Chapters
Selected Protocol
|