Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.naic.edu/vscience/schedule/tpfiles/KorpelatagP2589tp.pdf Дата изменения: Wed Jun 29 06:39:55 2011 Дата индексирования: Mon Feb 4 22:27:58 2013 Кодировка: Поисковые слова: эффект фарадея

Proposal Identification No.:

P2589

Date Received:

2011-Jun-01 20:09:13

Technical Page
Proposal Type: General Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: Regular Pulsars Galactic 40 Hours 2 hours

Reinvestigation of Unidentified Sources of Dispersed Pulses Found with As-

tropulse
ABSTRACT:
The Astropulse pro ject, a follow-on to the SETI@home distributed computing pro ject, uses the same dataset as SETI@home. But whereas SETI@home searches for narrow band signals of long time duration, Astropulse searches for short duration (us) pulses that have been dispersed by the interstellar medium. Possible sources of such pulses include giant pulses from pulsars or microscopic black holes evaporating due to Hawking radiation. These observations could also reveal the existence of new classes of pulse emitting compact ob jects. Or, more speculatively, an extraterrestrial civilization might use pulsed radio emissions as a beacon. We've identified 114 possible sources of such emission and would like to confirm their existence.

Name Eric J Korpela

Institution University of California, Berkeley

E-mail korpela@ssl.berkeley.edu

Phone 510-643-6538

Student no

Remote Observing Request

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

Instrument Setup
ALFA Atmospheric Observation Instruments:

Description of Observer Equipment: SETI@home data recorder Sp ecial Equipment or setup: We also would like to use the WAPPS and the Mock spectrometer in wide band mode. 1


RFI Considerations Frequency Ranges Planned
1150-1730

2