2309939
Project Grant
Overview
Grant Description
High resolution observations and studies of solar eruptions using the 1.6-meter telescope in Big Bear - New Jersey Institute of Technology (NJIT) has been operating Big Bear Solar Observatory (BBSO) for more than two decades. The observatory has remained highly productive - both in science output and in the development of state-of-the-art instrumentation.
This includes more than a hundred peer-reviewed publications over the past four years, as well as operations of the Goode Solar Telescope (GST) as a community facility and upgrading GST instrumentation to meet the evolving scientific requirements of users in the U.S. and worldwide. GST is one of the highest-resolution solar telescopes in the world.
Owing to the extended periods of stable excellent seeing at Big Bear Lake, GST with its high-order adaptive optics (AO), routinely collects diffraction-limited spatial resolution (~ 0.1, or 70 km on the solar surface) photometric, spectroscopic and polarimetric data, with a high cadence (< 40 s), across the spectrum from 430 nm to 8.2 μm.
This award supports five years of backbone support for BBSO operations, science, and education activities. BBSO will continue operating GST as a community facility. GST data and a substantial portion of the GST observing time are open to any solar physicists in the U.S. GST data have been and will be used in many Ph.D. theses.
BBSO will continue supporting the NSF-REU program by providing undergraduate students with hands-on experience in astronomical data analysis, high-resolution observations, and instrument development. The graduate student support will include involvement by members of underrepresented groups in astrophysics and includes two summer schools at BBSO, to train graduate students/postdocs/junior researchers on techniques in ground-based solar physics. Over 30% of the team members on the project are female researchers.
GST will continue playing a crucial and irreplaceable role in high-resolution solar physics to advance our understanding of the origin of space weather and the fundamental nature of the solar atmosphere. GST is the only large-aperture solar telescope that commonly experiences excellent seeing conditions lasting many hours on a regular basis.
During the upcoming maximum of Solar Cycle 25, the period covered by the award, BBSO will obtain, analyze, and interpret a wealth of high-resolution solar data. Using this resource, BBSO will develop and apply analytical tools to attack a number of critical, leading-edge problems in space weather research, with a particular focus on high-resolution observations and studies of solar eruptions, including (1) elementary magnetic reconnection, (2) flare energetics in lower solar atmosphere, (3) 3-D magnetic structure of flare productive active regions, (4) data-based modeling to understand flare triggering, and (5) small-scale magnetic flux ropes and associated jets.
Solar eruptions are the key sources of space weather, impacting the daily life of humans through effects on communication, transportation, power systems, national defense, and space travel. Moreover, BBSO will work to enhance coordination with NSF's Daniel K. Inouye Solar Telescope (DKIST) in telescope operations, instrumentation development, and science. GST and DKIST are complementary in instrument capabilities and discovery space.
BBSO community users, who are distributed across 61 universities, observatories, and institutes in 21 countries have been granted the majority of the GST observing time (> 80%). BBSO actively supports coordinated campaign observations with NASA space, rocket, and balloon missions (e.g., Parker Solar Probe), and other large ground-based facilities.
BBSO now provides a permanent home to the NSF's Synoptic Optical Long-term Investigation of the Sun (SOLIS) facility built by the National Solar Observatory. This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.
This includes more than a hundred peer-reviewed publications over the past four years, as well as operations of the Goode Solar Telescope (GST) as a community facility and upgrading GST instrumentation to meet the evolving scientific requirements of users in the U.S. and worldwide. GST is one of the highest-resolution solar telescopes in the world.
Owing to the extended periods of stable excellent seeing at Big Bear Lake, GST with its high-order adaptive optics (AO), routinely collects diffraction-limited spatial resolution (~ 0.1, or 70 km on the solar surface) photometric, spectroscopic and polarimetric data, with a high cadence (< 40 s), across the spectrum from 430 nm to 8.2 μm.
This award supports five years of backbone support for BBSO operations, science, and education activities. BBSO will continue operating GST as a community facility. GST data and a substantial portion of the GST observing time are open to any solar physicists in the U.S. GST data have been and will be used in many Ph.D. theses.
BBSO will continue supporting the NSF-REU program by providing undergraduate students with hands-on experience in astronomical data analysis, high-resolution observations, and instrument development. The graduate student support will include involvement by members of underrepresented groups in astrophysics and includes two summer schools at BBSO, to train graduate students/postdocs/junior researchers on techniques in ground-based solar physics. Over 30% of the team members on the project are female researchers.
GST will continue playing a crucial and irreplaceable role in high-resolution solar physics to advance our understanding of the origin of space weather and the fundamental nature of the solar atmosphere. GST is the only large-aperture solar telescope that commonly experiences excellent seeing conditions lasting many hours on a regular basis.
During the upcoming maximum of Solar Cycle 25, the period covered by the award, BBSO will obtain, analyze, and interpret a wealth of high-resolution solar data. Using this resource, BBSO will develop and apply analytical tools to attack a number of critical, leading-edge problems in space weather research, with a particular focus on high-resolution observations and studies of solar eruptions, including (1) elementary magnetic reconnection, (2) flare energetics in lower solar atmosphere, (3) 3-D magnetic structure of flare productive active regions, (4) data-based modeling to understand flare triggering, and (5) small-scale magnetic flux ropes and associated jets.
Solar eruptions are the key sources of space weather, impacting the daily life of humans through effects on communication, transportation, power systems, national defense, and space travel. Moreover, BBSO will work to enhance coordination with NSF's Daniel K. Inouye Solar Telescope (DKIST) in telescope operations, instrumentation development, and science. GST and DKIST are complementary in instrument capabilities and discovery space.
BBSO community users, who are distributed across 61 universities, observatories, and institutes in 21 countries have been granted the majority of the GST observing time (> 80%). BBSO actively supports coordinated campaign observations with NASA space, rocket, and balloon missions (e.g., Parker Solar Probe), and other large ground-based facilities.
BBSO now provides a permanent home to the NSF's Synoptic Optical Long-term Investigation of the Sun (SOLIS) facility built by the National Solar Observatory. This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.
Funding Goals
THE GOAL OF THIS PROGRAM IS TO SUPPORT RESEARCH PROPOSALS SPECIFIC TO "SOLAR TERRESTRIAL
Grant Program (CFDA)
Awarding / Funding Agency
Place of Performance
Big Bear City,
California
92314-9672
United States
Geographic Scope
Single Zip Code
Related Opportunity
Analysis Notes
Amendment Since initial award the total obligations have increased 281% from $850,030 to $3,239,659.
New Jersey Institute Of Technology was awarded
High-Res Solar Eruption Studies at BBSO
Project Grant 2309939
worth $3,239,659
from the Division of Atmospheric and Geospace Sciences in June 2023 with work to be completed primarily in Big Bear City California United States.
The grant
has a duration of 5 years and
was awarded through assistance program 47.050 Geosciences.
The Project Grant was awarded through grant opportunity Solar Terrestrial.
Status
(Ongoing)
Last Modified 9/10/25
Period of Performance
6/1/23
Start Date
5/31/28
End Date
Funding Split
$3.2M
Federal Obligation
$0.0
Non-Federal Obligation
$3.2M
Total Obligated
Activity Timeline
Transaction History
Modifications to 2309939
Additional Detail
Award ID FAIN
2309939
SAI Number
None
Award ID URI
SAI EXEMPT
Awardee Classifications
Public/State Controlled Institution Of Higher Education
Awarding Office
490602 DIVISION OF ATMOSPHERIC AND
Funding Office
490602 DIVISION OF ATMOSPHERIC AND
Awardee UEI
SGBMHQ7VXNH5
Awardee CAGE
4B854
Performance District
CA-23
Senators
Dianne Feinstein
Alejandro Padilla
Alejandro Padilla
Budget Funding
Federal Account | Budget Subfunction | Object Class | Total | Percentage |
---|---|---|---|---|
Research and Related Activities, National Science Foundation (049-0100) | General science and basic research | Grants, subsidies, and contributions (41.0) | $850,030 | 100% |
Modified: 9/10/25