Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.naic.edu/vscience/schedule/tpfiles/CarlsontagT2567tp.pdf Дата изменения: Mon Feb 15 15:06:36 2010 Дата индексирования: Mon Apr 11 16:46:11 2016 Кодировка: Поисковые слова: ацобс бфмбофйюеулбс бопнбмйс

Proposal Identification No.:

T2567

Date Received:

2010-Jan-29 15:41:05

Technical Page
Proposal Type: General Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: ABSTRACT: Regular Terrestrial Aeronomy HF Heating experiment 40 Hours two

Creating Space Plasma from the Ground

It was predicted (Carlson, 1993) that once high power HF transmitters achieved the Giga-Watt ERP level, they would from the ground produce plasma densities competitive with that produced by the sun, thereby breaking through a new threshold of progress for space science research. Only now has technology allowed testing that prediction, with two publications confirming it (Blagoveshchenskaya et al, 2009; Pedersen et al, 2009). The initial prediction was based on Arecibo HF heating experiment data (Carlson et al, 1982). The confirmations however involve processes expected to be important only at high latitudes (Gurevich, Carlson and Zybin, 2001). The purpose of this proposal is to learn how well the initial prediction scales to higher power densities, plus in light of current theory, test important dependencies on further geophysical processes now anticipated to be important. We know some ionization must be produced, we don' t know what processes determine significant production.

Name Herbert C Carlson

Institution Utah State University, CASS

E-mail herbert.c.carlson@gmail.com

Phone 435-797-2962

Student

Remote Observing Request

X

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

Instrument Setup
430 G 430 CH receiver

Atmospheric Observation Instruments: Tilt-Photometer Fabry-Perot Ionosonde none

Sp ecial Equipment or setup:

RFI Considerations
1


Frequency Ranges Planned

2