LOGIN TO YOUR ACCOUNT

Username
Password
Remember Me
Or use your Academic/Social account:

CREATE AN ACCOUNT

Or use your Academic/Social account:

Congratulations!

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.

Important!

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

CREATE AN ACCOUNT

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

Classified by OpenAIRE into

arxiv: Physics::Space Physics, Astrophysics::High Energy Astrophysical Phenomena
The electric field of the beam of rarified ionised gas ejected from the sun has been invoked by Alfvén in connection with geomagnetic storms and aurorae. An attempt is made to study the effects of this electric field on cosmic rays. From a study of the ionization chamber records published by Carnegie Institution for the years 1945 and 1946, it appears that the deceleration in the electric field seems to be the most important among the types of effects expected in cosmic rays.DOI: 10.1111/j.2153-3490.1957.tb01875.x
  • The results below are discovered through our pilot algorithms. Let us know how we are doing!

    • ALFV~NH,., 1950: Cosmicaal Electrodynamics (Oxford) Ch. VI.
    • - 1954:O n the origin of cosmic radiation, Tellus 6, p. 232.
    • - 1955: Theory of magnetic storms and aurorae, Tellus 7. p- SO.
    • - 1956: International Astronomical Union Conference on the Electromagnetic State in Cosmical Physics.
    • ALLBNC,. W., 1955: Astrophysical Quantities (University of London. Athlone Press) p. 129.
    • BARTBLSJ,., 1935: Terr. Mag. and Atmos. Electr. 40, p. 3.
    • - 1938:2. Geophysik V. p. 14.
    • - 1949:I.A . T . M . E. Bull. Washington No. 12 b, p. 97 -112.
    • BRUNBERGE., A. and DATTNERA,., 1954:Variations of the cosmic ray intensity during magnetic storms, Tellus 6 p. 73 and 6, p. 254.
    • BROXONJ., W., 1941:Recurrence Phenomena in Cosmic Rays. Phys. Rev. 59, p. 773.
    • CARNBGINIESTITUTIO1N9,48:Publication 175.
    • CHREE,C.. 1913:Phil. Trans. A, 212,p. 76.
    • CHRBEC,. and STAGGI., M., 1928:PhiLTrans. A, 2 2 7 , ~ 2.1.
    • FORBUSHS., E., 1937:Phys. Rev. 52, p. 1254.
    • - 1938 a: Terr. Magn. 43, p. 203.
    • - 1938 b: Phys. Rev. 54, p. 975.
    • - 1954: World wide cosmic ray variations 1937-52- J . Geoph. Res. 59, p. 525.
    • FORBUSHS,. E., STINCHCOMBT,. B. and SCHEIN.M., 1950: The extraordinary increase of cosmic ray intensity on November 19,1949.
    • HEBRDANV., and THAMBYPAIHLLAT1.955:The 27-day recurrence tendency of cosmic ray intensity, Phil. Mag. 46, p. 1238.
    • HESSV, . F. andDMMELMhIR,A., 1937:Nature 140,p. 316.
    • HOGC,A. R., 1949:Memoirs of the Commonwealth Observatory, Camberra, No. 10.
    • KANB, R, P., 1955: Recurrence phenomenon in the 24- hour variation of cosmic ray intensity, Phys. Rev. 98, p. 130.
    • LUNDQUISTS.,, 1954:A note on the variation of cosmic ray intensity produced by an electric field, Tellus 6, p. 260.
    • MEYER,P. and SIMPSONJ,. A.. 1954: Changes in amplitude of the cosmic ray 27.day intensity variation with solar activity, Phys. Rev. 96, p. 1085.
    • MBSSBRSCHMIDWT.,, 1933: Z.Phys. 85. p. 332.
    • MONK,A. T. and COMPTONA., H., 1939: Rev. Mod. Phys. 11, p. 175.
    • NEWTONH,. W., 1949:Observational aspects of the sunspot-geomagnetic storm relationships, Month. Not. R . A . S . 5. p. 322.
    • NEWTONH,. W. and MILSOM,A. S., ~954:The distribution of great and small magnetic storms in sunspot cycle, J. Geophys. Res. 59, p. 203.
    • PAWSEYJ,. L., and BRACEWELRL., N., 1955: Radio Astronomy (Oxford) p. 136.
    • ROBERTSJ. A., 1954:Research, 7, no. 10,Oct.
    • SIMPSONJ., A., FONGERW,. and WILCOXL,., 1952a: A solar component of the primary cosmic rays, Phys. Rev. 85, p. 366.
    • - 1952b: Temporal changes of nucleonic component intensity, Phys. Rev. 87, p. 240.
    • SIMPSONJ,. A.. FONGBRW,. and TREIMANS,. B., 1953: Cosmic ray intensity time variations and their origin I, Phys. Rev. 90, p. 934.
    • SIMPSONJ., A., 1954:Cosmic ray intensity time variations and their origin 111,Phys. Rev. 94, p. 426.
    • SINGBRF,., 1954: Storm decrease of the cosmic rays at the pole. Phys. Rev. p. 95,647.
    • - 1956: Maryland Univ. Phys. Dept., Terhn. Rep. 40.
    • STEINMAURERR. ,and GRAZIADEHI,. T., 1933:S. B. Akad. Wiss., Wien, 22,p. 672.
  • No related research data.
  • No similar publications.

Share - Bookmark

Cite this article

Collected from