[radioastro] One Jovian rotation later: more hectometric non-Io-B arcs on 101025, with a comment on their origin

  • From: Victor Herrero <hubbleed@xxxxxxxxx>
  • To: Marco Nicolini <heygio@xxxxxxxx>, Juan Fernando Tonatiuh Hernández Escobar <cecilixz@xxxxxxxxxxx>, Peter Hughes <PHughes@xxxxxxxxxx>, David Fields <fieldsde@xxxxxxx>, Steve McCauley <esmac@xxxxxxxxxx>, Dave Typinski <davetyp@xxxxxxxxxx>, "Whitham D. Reeve" <whitreeve@xxxxxxxxx>, Terrence Flower <tfflower@xxxxxxxxxx>, Jim Thieman <james.r.thieman@xxxxxxxx>, Divyadarshan Purohit <divyadarshan63@xxxxxxxxx>, Ramón Menéndez-Manjón <ramon.ramon.astronomers@xxxxxxxxx>, Tushar Sharma <sharma.tushar17@xxxxxxxxx>, "military.radioman" <samhevener@xxxxxxxxx>, Myamiphil <myamiphil@xxxxxxxxx>, danny garvin <grailknight_2@xxxxxxxxx>, Alfonso CastilloAbrego <cendap@xxxxxxxxxxx>, Thomas Ashcraft <ashcraft@xxxxxxxxxxxxx>, John Avellone <JGAVELLONE@xxxxxxx>, Arturo Garcia Cole <cole@xxxxxxxxxxxxxxxx>, Dalila Martinez <dmarti@xxxxxxxxxxxxxxxxx>, FRANCISCO BERSUNSES <siriober@xxxxxxxxxxx>, Steve Arnold <steve_arnold@xxxxxxxxxx>, Sajjad Mahdizadeh <sajjadea@xxxxxxxxx>, James H Van Prooyen <grro@xxxxxxxxxxxxx>, Cristian Leon Irribarra <celeon2@xxxxxxxxx>, "Karen & Jim Carson" <kjcarson@xxxxxxxxx>, Pablo Gonzalez <pablomgonzalez@xxxxxxxxxxxxx>, Clint Jeffrey <clintonjeffrey1@xxxxxxxxxxx>, Wanda Diaz <wanda@xxxxxxxxxxxxx>, Michael Rudolph <mrudolph@xxxxxxxxxxxxxxxxxxxxx>, Sead Kulenov <skulenov@xxxxxxxxx>, Neil Maron <neil.maron@xxxxxxxxx>, Wesley Greenman <greenman@xxxxxxxxxxxxx>, Jim Sky <radiosky@xxxxxxxxxxxx>, Salvador Aguirre <drsaguirre@xxxxxxxxx>, Abebe Kebede <abkebede@xxxxxxxxx>, Martin Wright <ducksuit@xxxxxxxxxxxxx>, Kibrom Yeibyo <kibromyeibyo@xxxxxxxxx>, Richard Flagg <rf@xxxxxxxxxxxxx>, _gloom_ gloom <_gloom_@xxxxxxx>
  • Date: Wed, 27 Oct 2010 04:32:24 -0700

One Jovian rotation later: more hectometric non-Io-B arcs on 101025, with a
comment on their origin

Hello Radio Astronomers,

I attach an annotated STEREO WAVES spectrum showing the activity  in the 1
to 3 MHz band.

See the 101024 spectrum at:
//www.freelists.org/archives/radioastro/10-2010/jpgxUrSEaQaD0.jpg

What is the origin of these hectometric events ?

Galopeau and Boudjada 2005 "Solar wind control of Jovian auroral emissions"
:
http://adsabs.harvard.edu/abs/2005JGRA..11009221G
propose that "Solar particles go through the polar regions where they
interact with the Jovian magnetic field and give rise in the auroral and
equatorial regions to an increase of Jovian hectometric emissions and/or
injection events."

I have read the abstract, but I need to get the full paper and study it in
detail.

Best regards,

Victor Herrero

Messages  //www.freelists.org/archive/radioastro
Pages   http://herrero.freei.me/
Blog  http://herrero-radio-astronomy.blogspot.com/

Attachment: SWAVES_101025_hecto_non-io-b 2.jpg
Description: JPEG image

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  • » [radioastro] One Jovian rotation later: more hectometric non-Io-B arcs on 101025, with a comment on their origin - Victor Herrero
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