Cover Page/Proposal Summary
ROSS-00 NRA 00-OSS-01
Date Due: 4/28/2000
This proposal shall be used and disclosed for evaluation purposes only, and a copy of this Government notice shall be applied to any reproduction or abstract thereof. Any authorized restrictive notices that the submitter places on this proposal shall also be strictly complied with. Disclosure of this proposal for any reason outside the Government evaluation purposes shall be made only to the extent authorized by the Government. |
Proposal Type: New Proposal |
Proposal Category: Laboratory |
Major Equipment Proposal? No |
Do you intend to submit an Education/Public Outreach (E/PO) proposal? No |
Proposal Title: |
Absolute Electron Excitation Cross Sections for Singly- and Highly-Charged Ions in Solar System Objects |
Abbreviated Proposal Title: |
Experimental Excitation Cross Sections in Ions |
Principal Investigator: |
Dr. Ara Chutjian Atomic and Molecular Collisions Team, MS 121-114 Jet Propulsion Laboratory 4800 Oak Grove Drive Pasadena, CA 91109-8099 Phone: (818) 354-7012 Fax: (818) 393-1899 E-mail: ara.chutjian@jpl.nasa.gov |
Signature | Date |
_____________________________________ | ____________ |
Co-Investigators and Collaborators: | |||
Type | Name | Affiliation | |
Sci Collab | Prof. Don E. Shemansky | Univ. So. Calif. | dons@hippolytus.usc.edu |
Sci Co-I | Dr. Steven J. Smith | JPL | steven.j.smith@jpl.nasa.gov |
Sci Collab | Prof. Swaraj S. Tayal | Clark Atlanta Univ. | stayal@cau.edu |
Proposal Summary:
The goal of this proposed work is to continue the measurement of absolute excitation cross sections in singly- and highly-charged positive ions which are detected in emission in the Io torus and Saturn's magnetosphere. Use is made of JPL's Highly-Charged Ion (HCI) Facility in which cross sections are measured by the electron energy-loss method, a versatile technique developed at JPL. The energy range is typically threshold through 5 x threshold. Measurements are compared to, or published together with, accurate multistate R-matrix results in the same energy range. The HCIs are generated using a 14 GHz electron cyclotron resonance ion source. A merged electron-ion beams geometry is used. Emphasis is on measurement of cross sections for resonance and forbidden transitions in O2+, O3+, S3+, and S4+ for the Io torus problem. The status of the singly-charged magnetospheric species, such as He+, Na+, K+ and Cl+, will then be assessed and cross sections measured in those emitters which can provide a diagnostic of ion density and electron temperature. It is planned to submit the new and prior-measured cross sections to the CHIANTI database for ease of access and use by the plasma modelers. The work proposed herein supports the continuing observations of the Galileo UVS instrument at Jupiter, the upcoming Cassini UV Mission at Saturn, and other ground-based and satellite (e.g., Chandra) observations of comets and the outer planets.
Certification of Compliance with Applicable Executive Orders and U.S. Code
By submitting the proposal identified in this Cover Sheet/Proposal Summary in response to this NRA or AO, the Authorizing Official of the proposing institution (or the individual proposer if there is no proposing institution) as identified below:
Willful provision of false information in this proposal and/or its supporting documents, or in reports required under an ensuing award, is a criminal offense (U.S. Code, Title 18, Section 1001).