Published June 2013 | Version v1
Journal article

Early Cosmic Ray Research with Balloons

Description

The discovery of cosmic rays by Victor Hess during a balloon flight in 1912 at an altitude of 5350 m would not have been possible without the more than one hundred years development of scientific ballooning. The discovery of hot air and hydrogen balloons and their first flights in Europe is shortly described. Scientific ballooning was mainly connected with activities of meteorologists. It was also the geologist and meteorologist Franz Linke, who probably observed first indications of a penetrating radiation whose intensity seemed to increase with the altitude. Karl Bergwitz and Albert Gockel were the first physicists studying the penetrating radiation during balloon flights. The main part of the article deals with the discovery of the extraterrestrial radiation by V. Hess and the confirmation by Werner Kolhörster

Availability note (English)

Available from http://dx.doi.org/10.1016/j.nuclphysbps.2013.05.002

Additional details

Identifiers

DOI
10.1016/j.nuclphysbps.2013.05.002;
PII
S0920-5632(13)00369-1;

Publishing Information

Journal Title
Nuclear Physics. B, Proceedings Supplements
Journal Volume
239-240
Journal Page Range
p. 11-18
ISSN
0920-5632
CODEN
NPBSE7

Conference

Title
From high energy gamma sources to cosmic rays, one century after their discovery
Acronym
9. workshop on science with the new generation of high energy gamma-ray experiments
Dates
20-22 Jun 2012
Place
Lecce (Italy)

INIS

Country of Publication
Netherlands
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
45065627
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
AIR; ALTITUDE; BALLOONS; COSMIC RADIATION; HYDROGEN
Descriptors DEC
AIRCRAFT; ELEMENTS; FLUIDS; GASES; IONIZING RADIATIONS; NONMETALS; RADIATIONS

Optional Information

Copyright
Copyright (c) 2013 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.