Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.naic.edu/vscience/schedule/tpfiles/JensentagR2257tp.pdf Дата изменения: Mon Jul 31 19:34:30 2006 Дата индексирования: Sat Dec 22 22:50:54 2007 Кодировка: Поисковые слова: europa

Proposal Identification No.:

R2257

Date Received:

2006-Jul-18 13:11:39

Technical Page
Proposal Type: General Category: Observation Category: Total Time Requested: Prop osal Title: ABSTRACT: Urgent Planetary Radar Solar System 6.5 Hours

Faraday Rotation of the Cassini S-Band transponder from Solar Corona

Coordinate observations using the UltraViolet Coronagraph Spectrometer (UVCS) instrument on SOHO and Faraday rotation observations using Cassini's S-band radio frequency carrier can provide valuable measurements of solar coronal plasma. The UVCS instrument is capable of measuring velocity, electron density, and temperature of the coronal plasma while the Cassini radio frequency data can measure the change in electron density and magnetic field. This study is very important because my results from previous Faraday rotation observations suggests the thermal and magnetic forces in the solar wind are balancing each other; however, without the temperature measurement, I cannot calculate the thermal pressure. This is an exciting opportunity for coronal physics research. We have received support to enable the S-band on Cassini to be operational during the conjunction and secured time on the SOHO/UVCS instrument. If possible, we would like to schedule a viewing opportunity on August 6 from 1515 to 1758 UTC, August 7 1511 to 1755 UTC, and/or August 8 from 1508 to 1751 UTC.

Name Elizabeth Jensen

Institution UCLA

E-mail "E. Jensen"

Phone

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
S-band receiver S-low

Atmospheric Observation Instruments:

Sp ecial Equipment or setup:

none

RFI Considerations
1


Frequency Ranges Planned

2