Published August 1985 | Version v1
Report

Photometric and spectroscopic gamma-ray observations of solar transient phenomena using long duration balloons

Description

A program currently in progress to conduct extended duration spectroscopic and photometric observation of solar x-ray phenomena from balloons is described. High photometric sensitivity to weak hard x-ray bursts is attained using a 600 sq cm array of phoswich scintillators. High spectral resolution for stronger bursts is available from an array of planar germanium detectors. These instruments are carried in a novel balloon gondola dssigned for the 15 to 20 day float durations available through using conventional zero pressure balloons in the radiation controlled (RACOON) mode

Additional details

Publishing Information

Imprint Title
Ninteenth International Cosmic Ray Conference. SH sessions, volume 5
Journal Page Range
vp.
Report number
N--85-34991

Conference

Title
19. international cosmic ray conference.
Dates
11-23 Aug 1985.
Place
La Jolla, CA (USA).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
19055892
Subject category
S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ENERGY SPECTRA; GE SEMICONDUCTOR DETECTORS; PHOTOMETRY; SCINTILLATION COUNTERS; SOLAR X-RAY BURSTS
Descriptors DEC
MEASURING INSTRUMENTS; RADIATION DETECTORS; SEMICONDUCTOR DETECTORS; SOLAR ACTIVITY; SPECTRA