Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.naic.edu/vscience/schedule/tpfiles/WaldroptagT2402tp.pdf
Дата изменения: Wed Feb 13 03:44:09 2008
Дата индексирования: Sat Sep 6 05:25:45 2008
Кодировка:

Поисковые слова: mercury surface
Proposal Identification No.:

T2402

Date Received:

2008-Feb-07 18:52:12

Technical Page
Proposal Type: General Category: Sub-Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: ABSTRACT:
Although atomic oxygen density, [O], is a key state parameter of the upper atmosphere, its empirical estimation is notoriously difficult. At mid-latitudes, OI 844.6 nm emission brightness is a potentially excellent proxy for [O], and recent improvements to its forward emission model warrant renewed effort to pursue ground-based sensing using this unique emission. This proposal represents a first step toward the development of this long-overdue capability. The scientific goals are two-fold: (1) to reduce the uncertainty in a key parameter ­ neutral meridional wind speed ­ of the forward model of 844.6 nm emission generation and (2) to assess the conditions for which the existing forward model is justified in its neglect of a key alternative source of 844.6 nm production ­ radiative recombination of O+. To this end, we propose several observational campaigns, spanning a variety of seasonal conditions, using combined passive optical and incoherent scatter radar instrumentation.

Long-term Terrestrial Aeronomy Radar Thermosphere 960 Hours 3 hours

Toward the development of a new [O] estimation technique using the twilight airglow OI 8446 ° emission A

Name Lara S Waldrop

Institution University of Illinois at UrbanaChampaign

E-mail lwaldrop@uiuc.edu

Phone 217-244-5129

Student no

Remote Observing Request

X

Observer will travel to AO Remote Observing In Absentia (instructions to operator)

Instrument Setup
430 G 430 CH receiver 430 CH radar

Atmospheric Observation Instruments: Tilt-Photometer Fabry-Perot 1


Sp ecial Equipment or setup:

none

RFI Considerations Frequency Ranges Planned

2