This Solicitation opportunity from National Aeronautics And Space Administration was posted on January 29, 2016. The submission period has ended. Browse the details below for market research, or find similar active opportunities.
HISAKI Guest Investigator Program 2016
Contract Overview
Solicitation details, issuing organization, response deadlines, documents, and interested companies for this government contract opportunity.
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General Info
Place of Performance
Not specifiedSet-Aside
Timeline
Submission Closed
Organization & Contact Information
Full Description
A resume not to exceed two pages, including relevant activities and publications.
Applications are solicited from individuals at U.S.-based research and academic institutions, Government laboratories, and industry, and from private individuals.
In order to assist with the planning for the review of proposals, interested individuals are requested to submit a Notice of Intent (NOI) by the date given below. The NOI will consist only of the 4000 character Summary, which should describe briefly the investigation(s) to be performed.
Schedule for HISAKI Guest Investigator call
Notices of Intent Due: February 8, 2016, 11:59 PM Eastern Time. Proposals Due: February 29, 2016, 4:30 PM Eastern Time.
Proposal Peer Review: March 2016 Final Selections Announced: Late March/April 2016
Overview of Hisaki Guest Investigator Program
The Hisaki Guest Investigator Program provides membership to the Hisaki Team, for science dialogue of planning of observations in other wavebands, for complementary theoretical studies, and, if viable, EUV observations of Venus and Mars as global systems.
Topics Hisaki Guest Investigators are invited to propose are:
To analyze Hisaki data from the beginning of science operations through its extended mission phase
To analyze the relationship among the Jupiter magnetosphere, auroral activity, the Io plasma torus, and the Europa system.
To analyze HISAKI’s EXCEED instrument data for auroral light-curves of bright or transient events in Jupiter’s atmosphere.
To support correlated observations of EUV sources at other wavelengths directly relevant to Hisaki and other planetary missions (Juno).
To perform theoretical studies of EUV sources and model the energy flow within the Jovian magnetospheric system.
To obtain observing time in ground observing facilities in support of the Hisaki Jupiter science themes.
All investigations must have the Jupiter system as the primary science objective. Observations of other planetary bodies (Venus and Mars) will be considered secondary science objectives.
Questions can be submitted to Dr. Adriana C. Ocampo at aco@nasa.gov or 202 358-2152.
NOIs and proposals should be submitted via NSPIRES (http://nspires.nasaprs.com) by the due dates listed above.
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