Remember Me
Or use your Academic/Social account:


Or use your Academic/Social account:


You have just completed your registration at OpenAire.

Before you can login to the site, you will need to activate your account. An e-mail will be sent to you with the proper instructions.


Please note that this site is currently undergoing Beta testing.
Any new content you create is not guaranteed to be present to the final version of the site upon release.

Thank you for your patience,
OpenAire Dev Team.

Close This Message


Verify Password:
Verify E-mail:
*All Fields Are Required.
Please Verify You Are Human:
fbtwitterlinkedinvimeoflicker grey 14rssslideshare1
Brunberg, E. A.; Dattner, A. (2011)
Publisher: Co-Action Publishing
Journal: Tellus A
Languages: English
Types: Article

Classified by OpenAIRE into

arxiv: Astrophysics::High Energy Astrophysical Phenomena, Physics::Space Physics
The recorded data of diurnal variation of the cosmic ray intensity are analysed. By using the known deflection of the cosmic ray particles in the geomagnetic field (Brunberg and Dattner 1953) and under an assumption of an anisotropy in the primary cosmic radiation, it is shown that the momentum of the primary radiation and the direction of the anisotropy can be determined. The anisotropy is explained as an effect due to the distribution of cosmic ray particles rotating with the solar magnetic field as suggested by H. Alfvén. The diurnal variation is ascribed to the earth's rotation in the anisotropic distribution of cosmic ray particles. The theoretical amplitude of this variation is calculated.DOI: 10.1111/j.2153-3490.1954.tb01094.x
  • The results below are discovered through our pilot algorithms. Let us know how we are doing!

    • ALFV~NH,., 1938:Registration of the Cosmic Radiation by means of Coincidence Counters. Arkiv f. Matcmatik, Asfronomi och Fysik, 26B, No. 14.
    • - 1950:Cosmical Electrodynamics. Oxford.
    • - 1952: On the Zeeman effect measurements of the sun's general magnetic field. Arkiv f. Fysik, 4B, No. 14.
    • - and MALMFORKS,. G., 1943:Directional Measurements of Cosmic Radiation. A r k i v . f. Matematik, Astronomi och Fysik. 29A. No. 24.
    • BRUNBEREG.,if., and DATTNERA,., 1953 : Electron orbits in the field of a magnetic dipole. Tellus. Vol. 5 , No, 2, 3.
    • COMPTONA,. H. and GETTINGI,. A., 1935:An Apparent Effect of Galactic Rotation on the Intensity of Cosmic Rays. Phys. R e v . 47. 0. 817.
    • ELLIOTH,. and DOLBBARD,. W. N., 1950: Directional measurements of the diurnal variation of cosmic ray intensity. Proceedings of the Physical Soc. A. Vol. LXIII.
    • - 1951: Directional measurements of the diurnal variation of cosmic ray intensity. Journ. ofAtmospheric and Terrestrial Physics Vol. I.
    • - and THAMBYAHPTI L., L1N95,3: World-wide changes in the phase of the cosmic-ray solar daily variation. Nature. May 23.
    • EPSTEINP,. S., 1938:Influence of the solar magnetic field upon cosmic rays. Phys. Rev. 5 3
    • FERRARVO., C. A.,1937:The Non-uniform Rotation of the Sun and its Magnetic Field. Mont. Not. R . As&. SOC.97. p. 458.
    • J ~ N O S S LY., 1937: u b e r einen moglichen Einfiusr des Magnetfeldes der Sonne auf die in Erdnahe beobachtete Hohenstrahlung. 2s.f. Physik, 104.430.
    • KANEE,. 0..SHANLETY.J. B., and WHEELEJ.RA,.,1949: Cosmic Rays and heavenly bodies. R e v . Mod. Phys. VOl. 21.
    • KOLHORSTEWR,. 1941: Der Tagesgang der Hohenstrahlung. Phys. Zs. 42. 55
    • LANGEI. and FORBUSHS,., 1948:Carnegie Instifution of Washington. Publ. 175. 14.
    • MALMFORKS.,G., 1949:Recordings of Cosmic Radiation. Tellus. Vol. I, 2.
    • MONTGOMERDY., J. X., 1949: Cosmic Ray Physics. Princeton University Press.
    • SARABHAVI,. and KANE,R. P., 1953: World-Wide Effects of Continuous Emission of Cosmic Rays from the Sun. Phys. R e v . 90. No 2, p. 204.
    • SEKIDOY, . and KODAMAM, ., 1952: Diurnal variation of vertical cosmic rays. Rep. qflonosph. Research inJapan. Vol. VI nr 2.
    • VALLARTMA,. S., 1937:Cosmic Rays and the Magnetic Moment of the Sun. Nature, May 17.
    • - GRABFC,., and KUSAKAS,., 1939:Galactic Rotation and the Intensity of Cosmic Radiation at the Geomagnetic Equator. Phys. R e v . 55, p. I.
  • No related research data.
  • No similar publications.

Share - Bookmark

Cite this article

Collected from