[radioastro] About the "thickness" of the RSP trace near Solar events
- 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>, _gloom_ gloom <_gloom_@xxxxxxx>
- Date: Mon, 25 Oct 2010 10:28:56 -0700
About the "thickness" of the RSP trace near Solar events
Hello Radio Astronomers,
I quote Dave Typinski in a message dated Oct 24 2010 in the GSFC list:
"All other things being equal, and assuming the bottom of the chart is at
zero kelvin, the trace of the galactic background (or of any other pure
noise source, calibrators included) will always be "thinner" the lower it is
on the chart."
Near a Solar burst we may not assume other things are constant.
The Solar radiation and the Ionospheric opacity may be fluctuating a great
deal, changing the apparent "thickness" of the trace.
I must disagree with the quoted statement.
Best regards,
Victor Herrero
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