Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.naic.edu/vscience/schedule/tpfiles/GoldstontagA2050tp.pdf Дата изменения: Fri Aug 11 19:16:50 2006 Дата индексирования: Sat Dec 22 23:35:05 2007 Кодировка:

Proposal Identification No.:

A2050

Date Received:

2006-Feb-01 17:27:45

Technical Page
Proposal Type: General Category: Sub-Category: Observation Category: Total Time Requested: Prop osal Title: ABSTRACT: Regular Astronomy Spectroscopy Galactic 72 Hours

Turbulence and Feedback in the Diffuse ISM

We intend to morphologically and quantitatively identify sources of turbulence in the high galactic latitude interstellar medium. We have already observed isolated cases of ejecta that morphologically resemble outflows from stars and we now wish to classify these as well as constrain the turbulent cascade and energy injection scales. We are able to do this now due to two recent advances. Firstly, the development of new turbulence analysis tools that can better interpret position-position-velocity (PPV) HI cubes and, secondly, the implementation of ALFA, which lends vastly increased mapping speed and associated advanced data reduction techniques.

Name Joshua E. Goldston

Institution UC Berkeley

E-mail goldston@astro.berkeley.edu

Phone 510 643 8592

Student G

Service Observing Request

Remot e Observing Request

X

None All of the observing run. Part of the observing run. Queue Observing X

No Maybe Yes

Instrument Setup
ALFA Atmospheric Observation Instruments:

Sp ecial Equipment or setup:

none

RFI Considerations Frequency Ranges Planned
1370 - 1470

1