From: "Saved by Windows Internet Explorer 9"
Subject: Einstein-De Haas Coupling of Geomagnetic Storms to the Earth's Crust
Date: Sat, 19 Feb 2011 20:16:35 -0500
MIME-Version: 1.0
Content-Type: text/html;
	charset="utf-8"
Content-Transfer-Encoding: quoted-printable
Content-Location: http://adsabs.harvard.edu/abs/2010AGUFMNH13A1141W
X-MimeOLE: Produced By Microsoft MimeOLE V6.0.6002.18263

=EF=BB=BF<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN" =
"http://www.w3c.org/TR/1999/REC-html401-19991224/loose.dtd">
<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN" =
"http://www.w3.org/TR/REC-html40/loose.dtd"><HTML><!--RAW FILE--><HEAD>
<LINK rel=3D"canonical" =
content=3D"http://adsabs.harvard.edu/abs/2010AGUFMNH13A1141W">
<META name=3D"robots" content=3D"noarchive">
<META content=3D"text/html; charset=3DUTF-8" =
http-equiv=3D"Content-Type">
<TITLE>Einstein-De Haas Coupling of Geomagnetic Storms to the Earth's=20
Crust</TITLE>
<META name=3D"citation_language" content=3D"en">
<META name=3D"citation_abstract_html_url" =
content=3D"http://adsabs.harvard.edu/abs/2010AGUFMNH13A1141W">
<META name=3D"citation_title" content=3D"Einstein-De Haas Coupling of =
Geomagnetic Storms to the Earth's Crust">
<META name=3D"citation_authors" content=3D"Walkley, R. L.; Lazarus, M.; =
Wang, J. S.; Dahlgren, R.; Freund, F. T.">
<META name=3D"citation_keywords" content=3D"[5440] PLANETARY SCIENCES: =
SOLID SURFACE PLANETS / Magnetic fields and magnetism, [7513] SOLAR =
PHYSICS, ASTROPHYSICS, AND ASTRONOMY / Coronal mass ejections, [7904] =
SPACE WEATHER / Geomagnetically induced currents, [8164] TECTONOPHYSICS =
/ Stresses: crust and lithosphere">
<META name=3D"citation_date" content=3D"12/2010">
<META name=3D"citation_journal_title" content=3D"AGU Fall Meeting =
Abstracts">
<META name=3D"citation_firstpage" content=3D"1141"><LINK =
title=3D"schema(PRISM)" rel=3D"schema.prism"=20
href=3D"http://prismstandard.org/namespaces/1.2/basic/">
<META name=3D"prism.publicationName" content=3D"AGU Fall Meeting =
Abstracts">
<META name=3D"prism.volume" content=3D"-1">
<META name=3D"prism.startingPage" content=3D"1141"><LINK =
title=3D"schema(DC)" rel=3D"schema.dc"=20
href=3D"http://purl.org/dc/elements/1.1/">
<META name=3D"dc.language" content=3D"en">
<META name=3D"dc.date" content=3D"2010-12">
<META name=3D"dc.source" content=3D"American Geophysical Union, Fall =
Meeting 2010, abstract #NH13A-1141">
<META name=3D"dc.title" content=3D"Einstein-De Haas Coupling of =
Geomagnetic Storms to the Earth's Crust">
<META name=3D"dc.creator" content=3D"Walkley, R. L.">
<META name=3D"dc.creator" content=3D"Lazarus, M.">
<META name=3D"dc.creator" content=3D"Wang, J. S.">
<META name=3D"dc.creator" content=3D"Dahlgren, R.">
<META name=3D"dc.creator" content=3D"Freund, F. T."><LINK rel=3D"icon" =
type=3D"image/x-icon"=20
href=3D"/favicon.ico"><LINK rel=3D"shortcut icon" type=3D"image/x-icon" =
href=3D"/favicon.ico">
<SCRIPT language=3D"JavaScript" type=3D"text/javascript">=0A=
<!-- Begin=0A=
function mkemail(parts) {=0A=
    var sep =3D ".";=0A=
    var str =3D arguments[0];=0A=
    for ( var i =3D 1 ; i < arguments.length ; i++ ) {=0A=
        if ( arguments[i] =3D=3D "" ) {=0A=
            sep =3D String.fromCharCode(29+35) ;=0A=
           continue ;=0A=
        } else {=0A=
            str =3D str.concat ( sep ) ;=0A=
            str =3D str.concat ( arguments[i] ) ;=0A=
            sep =3D ".";=0A=
        }=0A=
    }=0A=
    return(str);=0A=
}=0A=
var toggle =3D 0 ;=0A=
function t(){=0A=
if ( toggle =3D=3D 0 ) {=0A=
setStyleByClass("span","a","backgroundColor","#ffffff");=0A=
setStyleByClass("div","h","backgroundColor","#ffffff");=0A=
setStyleByClass("div","h","opacity","0");=0A=
setStyleByClass("div","h","filter","alpha(opacity=3D0)");=0A=
setStyleByClass("span","b","backgroundColor","#ffffff");=0A=
setStyleByClass("div","i","backgroundColor","#ffffff");=0A=
setStyleByClass("div","i","opacity","0");=0A=
setStyleByClass("div","i","filter","alpha(opacity=3D0)");=0A=
setStyleByClass("span","c","backgroundColor","#ffffff");=0A=
setStyleByClass("div","j","backgroundColor","#ffffff");=0A=
setStyleByClass("div","j","opacity","0");=0A=
setStyleByClass("div","j","filter","alpha(opacity=3D0)");=0A=
setStyleByClass("span","d","backgroundColor","#ffffff");=0A=
setStyleByClass("div","k","backgroundColor","#ffffff");=0A=
setStyleByClass("div","k","opacity","0");=0A=
setStyleByClass("div","k","filter","alpha(opacity=3D0)");=0A=
setStyleByClass("span","e","backgroundColor","#ffffff");=0A=
setStyleByClass("div","l","backgroundColor","#ffffff");=0A=
setStyleByClass("div","l","opacity","0");=0A=
setStyleByClass("div","l","filter","alpha(opacity=3D0)");=0A=
setStyleByClass("span","f","backgroundColor","#ffffff");=0A=
setStyleByClass("div","m","backgroundColor","#ffffff");=0A=
setStyleByClass("div","m","opacity","0");=0A=
setStyleByClass("div","m","filter","alpha(opacity=3D0)");=0A=
setStyleByClass("span","g","backgroundColor","#ffffff");=0A=
setStyleByClass("div","n","backgroundColor","#ffffff");=0A=
setStyleByClass("div","n","opacity","0");=0A=
setStyleByClass("div","n","filter","alpha(opacity=3D0)");=0A=
toggle =3D 1 ;=0A=
} else {=0A=
setStyleByClass("span","a","backgroundColor","#ffff88");=0A=
setStyleByClass("div","h","backgroundColor","#ffff00");=0A=
setStyleByClass("div","h","opacity","0.3");=0A=
setStyleByClass("div","h","filter","alpha(opacity=3D30)");=0A=
setStyleByClass("span","b","backgroundColor","#ccccff");=0A=
setStyleByClass("div","i","backgroundColor","#3333ff");=0A=
setStyleByClass("div","i","opacity","0.3");=0A=
setStyleByClass("div","i","filter","alpha(opacity=3D30)");=0A=
setStyleByClass("span","c","backgroundColor","#ffcccc");=0A=
setStyleByClass("div","j","backgroundColor","#ff3333");=0A=
setStyleByClass("div","j","opacity","0.3");=0A=
setStyleByClass("div","j","filter","alpha(opacity=3D30)");=0A=
setStyleByClass("span","d","backgroundColor","#bbffff");=0A=
setStyleByClass("div","k","backgroundColor","#00ffff");=0A=
setStyleByClass("div","k","opacity","0.3");=0A=
setStyleByClass("div","k","filter","alpha(opacity=3D30)");=0A=
setStyleByClass("span","e","backgroundColor","#ffdd77");=0A=
setStyleByClass("div","l","backgroundColor","#ff6600");=0A=
setStyleByClass("div","l","opacity","0.3");=0A=
setStyleByClass("div","l","filter","alpha(opacity=3D30)");=0A=
setStyleByClass("span","f","backgroundColor","#ccffaa");=0A=
setStyleByClass("div","m","backgroundColor","#33ff00");=0A=
setStyleByClass("div","m","opacity","0.3");=0A=
setStyleByClass("div","m","filter","alpha(opacity=3D30)");=0A=
setStyleByClass("span","g","backgroundColor","#ffccff");=0A=
setStyleByClass("div","n","backgroundColor","#ff00ff");=0A=
setStyleByClass("div","n","opacity","0.3");=0A=
setStyleByClass("div","n","filter","alpha(opacity=3D30)");=0A=
toggle =3D 0 ;=0A=
}=0A=
}=0A=
var ie =3D (document.all) ? true : false;=0A=
=0A=
function setStyleByClass(t,c,p,v){=0A=
	var elements;=0A=
	if(t =3D=3D '*') {=0A=
		elements =3D (ie) ? document.all : document.getElementsByTagName('*');=0A=
	} else {=0A=
		elements =3D document.getElementsByTagName(t);=0A=
	}=0A=
	for (var i =3D 0; i < elements.length; i++)=0A=
    {=0A=
		var node =3D elements.item(i);=0A=
		for(var j =3D 0; j < node.attributes.length; j++)=0A=
		{=0A=
			if(node.attributes.item(j).nodeName =3D=3D 'class')=0A=
			{=0A=
				if(node.attributes.item(j).nodeValue =3D=3D c)=0A=
				{=0A=
				eval('node.style.' + p + " =3D '" +v + "'");=0A=
				}=0A=
			}=0A=
		}=0A=
	}=0A=
}=0A=
//  End -->=0A=
</SCRIPT>

<STYLE>.a{background-color: #ffff88}</STYLE>

<STYLE>.h{background-color: #ffff00}</STYLE>

<STYLE>.b{background-color: #ccccff}</STYLE>

<STYLE>.i{background-color: #3333ff}</STYLE>

<STYLE>.c{background-color: #ffcccc}</STYLE>

<STYLE>.j{background-color: #ff3333}</STYLE>

<STYLE>.d{background-color: #bbffff}</STYLE>

<STYLE>.k{background-color: #00ffff}</STYLE>

<STYLE>.e{background-color: #ffdd77}</STYLE>

<STYLE>.l{background-color: #ff6600}</STYLE>

<STYLE>.f{background-color: #ccffaa}</STYLE>

<STYLE>.m{background-color: #33ff00}</STYLE>

<STYLE>.g{background-color: #ffccff}</STYLE>

<STYLE>.n{background-color: #ff00ff}</STYLE>

<STYLE type=3D"text/css">=0A=
a:link {color: #0000ff}=0A=
a.oa:link {color: #00a000}=0A=
a:visited {color: #4000a0}=0A=
a.oa:visited {color: #006666}=0A=
a:hover {color: #ff0000}=0A=
a.oa:hover {color: #cc33cc}=0A=
</STYLE>

<META name=3D"GENERATOR" content=3D"MSHTML 9.00.8080.16413"></HEAD>
<BODY aLink=3D"#ff0000" bgColor=3D"#ffffff" text=3D"#000000" =
vLink=3D"#4000a0" link=3D"#0000ff">
<DIV style=3D"padding-bottom: 4px; font-size: 84%;" align=3D"right"><A =
href=3D"http://adsabs.harvard.edu/cgi-bin/nph-manage_account?man_cmd=3Dlo=
gin&amp;man_url=3Dhttp://adsabs.harvard.edu/abs/2010AGUFMNH13A1141W">Sign=
=20
on</A></DIV>
<P>
<H3><A href=3D"http://www.adsabs.harvard.edu/">SAO/NASA ADS</A> <A =
href=3D"http://adsabs.harvard.edu/physics_service.html">Physics=20
Abstract Service</A></H3>
<HR>

<P>
<DL>
  <DT>
  <TABLE width=3D"100%">
    <TBODY>
    <TR>
      <TD align=3D"left"><STRONG>=C2=B7 <A =
href=3D"http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?return_req=3Dno=
_params&amp;arxiv_sel=3DALL&amp;db_key=3DPHY&amp;text=3DDuring%20geomagne=
tic%20storms%20coronal%20mass%20ejection%20%28CME%29%20often%20arrive%20a=
t%0athe%20Earth%20within%20a%20few%20minutes.%20The%20CME%20carry%20with%=
20them,%20among%20other%0athings,%20rapid%20magnetic%20field%20changes%20=
%26delta%3bB/%26delta%3bt.%20In%20the%20crust,%0a%26delta%3bB/%26delta%3b=
t%20couples%20to%20the%20magnetic%20moments%20of%20paramagnetic%20ions,%0=
aflipping%20their%20electron%20spins%20and%20giving%20rise%20to%20an%20Ei=
nstein%20de-Haas%0aforce%20%5b1%5d.%20In%20this%20study%20the%20magnitude=
%20of%20the%20Einstein%20de-Haas%20force%20is%0acalculated,%20assuming%20=
a%20spin%20density%20in%20crustal%20rocks%20on%20the%20order%20of%0a1035%=
20km-3%20and%20a%20rigid%20300%20km%20x%20300%20km%20crustal%20block%20th=
at%20is%2010%20km%20thick.%0aUnder%20these%20conditions%20a%20400%20nT%20=
%28G4-class%29%20solar%20event%20is%20estimated%20to%0ainduce%20an%20Eins=
tein-De%20Haas%20torque%20of%201.2%20x%201011%20N-m.%20Such%20large%20tor=
ques%0amay%20trigger%20earthquakes%20along%20faults%20where%20tectonic%20=
stresses%20are%20close%0ato%20the%20failure%20threshold.%20We%20therefore=
%20anticipate%20that%20due%20to%0aEinstein-de%20Haas%20coupling,%20there%=
20may%20be%20an%20increase%20in%20seismic%20activity%0awithin%20a%20relat=
ively%20short%20time%20window%20after%20arrival%20of%20large%20magnetic%0=
astorms.%20The%20transient%20augmentation%20in%20crustal%20stress%20may%2=
0also%20manifest%0aitself%20in%20an%20increase%20in%20air%20ionization%20=
at%20the%20Earth%26rsquo%3bs%20surface%20and%0aother%20phenomena%20%5b2%5=
d.%20Time-series%20analysis%20has%20shown%20that%20local%0aseismicity%20a=
nd%20integrated%20earthquake%20energy%20appear%20to%20have%20periodicitie=
s%0awith%20respect%20to%20local%20time,%20possibly%20due%20to%20ionospher=
e-to-solid%20Earth%0acoupling%20%5b3%5d.%20A%20similar%20approach%20will%=
20be%20used%20to%20perform%20a%20correlation%0aanalysis%20of%20seismic%20=
events%20with%20respect%20to%20historical%20CME%20events.%20%5b1%5d%20A.%=
0aEinstein%20and%20W.%20de%20Haas,%20%26ldquo%3bExperimental%20proof%20of=
%20the%20existence%20of%0aAmp%26egrave%3bre%27s%20molecular%20currents,%2=
6rdquo%3b%20Proc.%20Koninklijke%20Akad.%0aWetenschappen%20te%20Amsterdam,=
%2018,%20696-711%20%281915%29.%20%5b2%5d%20F.%20Freund%20et%20al.,%0a%26l=
dquo%3bAir%20ionization%20at%20rock%20surface%20and%20pre-earthquake%20si=
gnals,%26rdquo%3b%0aJ.%20Atmos.%20Sol.%20Terr.%20Phys.,%2071,%201824-1834=
%20%282009%29.%20%5b3%5d%20G.%20Duma%20and%20Y.%0aRuzhin,%20%26ldquo%3bDi=
urnal%20changes%20of%20earthquake%20activity%20and%20geomagnetic%0aSq-var=
iations,%26rdquo%3b%20Natural%20Hazards%20and%20Earth%20System%20Sciences=
,%203,%0a171-177%20%282003%29.%0a+%5b5440%5d%20PLANETARY%20SCIENCES%3a%20=
SOLID%20SURFACE%20PLANETS%20/%20Magnetic%20fields%20and%20magnetism,%20%5=
b7513%5d%20SOLAR%20PHYSICS,%20ASTROPHYSICS,%20AND%20ASTRONOMY%20/%20Coron=
al%20mass%20ejections,%20%5b7904%5d%20SPACE%20WEATHER%20/%20Geomagnetical=
ly%20induced%20currents,%20%5b8164%5d%20TECTONOPHYSICS%20/%20Stresses%3a%=
20crust%20and%20lithosphere+&amp;title=3DEinstein-De%20Haas%20Coupling%20=
of%20Geomagnetic%20Storms%20to%20the%20Earth%27s%20Crust">Find=20
        Similar Abstracts</A> (with <A =
href=3D"http://adsabs.harvard.edu/abs/2010AGUFMNH13A1141W#feedback">defau=
lt=20
        settings below</A>)</STRONG></TD></TR></TBODY></TABLE>
  <DT><STRONG>=C2=B7 <A =
href=3D"http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=3D2010AG=
UFMNH13A1141W&amp;link_type=3DAR&amp;db_key=3DPHY">Also-Read=20
  Articles</A></STRONG> (<A =
href=3D"http://adsabs.harvard.edu/cgi-bin/nph-ref_history?refs=3DAR&amp;b=
ibcode=3D2010AGUFMNH13A1141W">Reads=20
  History</A>)
  <DT>=C2=B7
  <DT><STRONG>=C2=B7 <A =
href=3D"http://www.microsofttranslator.com/BV.aspx?from=3Den&amp;a=3Dhttp=
://adsabs.harvard.edu/abs/2010AGUFMNH13A1141W">Translate=20
  This Page</A></STRONG></DT></DL>
<TABLE>
  <TBODY>
  <TR>
    <TD vAlign=3D"top" noWrap=3D"" align=3D"left"><B>Title:</B></TD>
    <TD><BR></TD>
    <TD vAlign=3D"top" align=3D"left">Einstein-De Haas Coupling of =
Geomagnetic=20
      Storms to the Earth's Crust</TD></TR>
  <TR>
    <TD vAlign=3D"top" noWrap=3D"" align=3D"left"><B>Authors:</B></TD>
    <TD><BR></TD>
    <TD vAlign=3D"top" align=3D"left"><A =
href=3D"http://adsabs.harvard.edu/cgi-bin/author_form?author=3DWalkley,+R=
&amp;fullauthor=3DWalkley,%20R.%20L.&amp;charset=3DUTF-8&amp;db_key=3DPHY=
">Walkley,&nbsp;R.&nbsp;L.</A>;=20
      <A =
href=3D"http://adsabs.harvard.edu/cgi-bin/author_form?author=3DLazarus,+M=
&amp;fullauthor=3DLazarus,%20M.&amp;charset=3DUTF-8&amp;db_key=3DPHY">Laz=
arus,&nbsp;M.</A>;=20
      <A =
href=3D"http://adsabs.harvard.edu/cgi-bin/author_form?author=3DWang,+J&am=
p;fullauthor=3DWang,%20J.%20S.&amp;charset=3DUTF-8&amp;db_key=3DPHY">Wang=
,&nbsp;J.&nbsp;S.</A>;=20
      <A =
href=3D"http://adsabs.harvard.edu/cgi-bin/author_form?author=3DDahlgren,+=
R&amp;fullauthor=3DDahlgren,%20R.&amp;charset=3DUTF-8&amp;db_key=3DPHY">D=
ahlgren,&nbsp;R.</A>;=20
      <A =
href=3D"http://adsabs.harvard.edu/cgi-bin/author_form?author=3DFreund,+F&=
amp;fullauthor=3DFreund,%20F.%20T.&amp;charset=3DUTF-8&amp;db_key=3DPHY">=
Freund,&nbsp;F.&nbsp;T.</A></TD></TR>
  <TR>
    <TD vAlign=3D"top" noWrap=3D"" =
align=3D"left"><B>Affiliation:</B></TD>
    <TD><BR></TD>
    <TD vAlign=3D"top" align=3D"left">AA(Physics, Lancaster University, =
Lancaster,=20
      United Kingdom; <EMAIL>
<SCRIPT language=3D"JavaScript" =
type=3D"text/javascript">document.write(mkemail("r","walkley","","lancast=
er","ac","uk"));</SCRIPT>
      </EMAIL>), AB(Physics, Lancaster University, Lancaster, United =
Kingdom;=20
      <EMAIL>
<SCRIPT language=3D"JavaScript" =
type=3D"text/javascript">document.write(mkemail("m","lazarus","","lancast=
er","ac","uk"));</SCRIPT>
      </EMAIL>), AC(SETI Institute, Mountain View, CA, USA; <EMAIL>
<SCRIPT language=3D"JavaScript" =
type=3D"text/javascript">document.write(mkemail("jswang","","lbl","gov"))=
;</SCRIPT>
      </EMAIL>), AD(SETI Institute, Mountain View, CA, USA; <EMAIL>
<SCRIPT language=3D"JavaScript" =
type=3D"text/javascript">document.write(mkemail("robert","dahlgren","","s=
jsu","edu"));</SCRIPT>
      </EMAIL>), AE(SETI Institute, Mountain View, CA, USA; <EMAIL>
<SCRIPT language=3D"JavaScript" =
type=3D"text/javascript">document.write(mkemail("friedemann","t","freund"=
,"","nasa","gov"));</SCRIPT>
      </EMAIL>)</TD></TR>
  <TR>
    <TD vAlign=3D"top" noWrap=3D"" =
align=3D"left"><B>Publication:</B></TD>
    <TD><BR></TD>
    <TD vAlign=3D"top" align=3D"left">American Geophysical Union, Fall =
Meeting=20
      2010, abstract #NH13A-1141</TD></TR>
  <TR>
    <TD vAlign=3D"top" noWrap=3D"" align=3D"left"><B>Publication =
Date:</B></TD>
    <TD><BR></TD>
    <TD vAlign=3D"top" align=3D"left">12/2010</TD></TR>
  <TR>
    <TD vAlign=3D"top" noWrap=3D"" align=3D"left"><B>Origin:</B></TD>
    <TD><BR></TD>
    <TD vAlign=3D"top" align=3D"left"><A =
href=3D"http://www.agu.org/">AGU</A></TD></TR>
  <TR>
    <TD vAlign=3D"top" noWrap=3D"" align=3D"left"><B>Keywords:</B></TD>
    <TD><BR></TD>
    <TD vAlign=3D"top" align=3D"left">[5440] PLANETARY SCIENCES: SOLID =
SURFACE=20
      PLANETS / Magnetic fields and magnetism, [7513] SOLAR PHYSICS,=20
      ASTROPHYSICS, AND ASTRONOMY / Coronal mass ejections, [7904] SPACE =
WEATHER=20
      / Geomagnetically induced currents, [8164] TECTONOPHYSICS / =
Stresses:=20
      crust and lithosphere</TD></TR>
  <TR>
    <TD vAlign=3D"top" noWrap=3D"" align=3D"left"><B>Bibliographic =
Code:</B></TD>
    <TD><BR></TD>
    <TD vAlign=3D"top" align=3D"left"><A =
href=3D"http://adsabs.harvard.edu/abs/2010AGUFMNH13A1141W">2010AGUFMNH13A=
1141W</A></TD></TR>
  </TBODY></TABLE>
<H3 align=3D"center">                               Abstract</H3>During=20
geomagnetic storms coronal mass ejection (CME) often arrive atthe Earth =
within a=20
few minutes. The CME carry with them, among otherthings, rapid magnetic =
field=20
changes =CE=B4B/=CE=B4t. In the crust,=CE=B4B/=CE=B4t couples to the =
magnetic moments of=20
paramagnetic ions,flipping their electron spins and giving rise to an =
Einstein=20
de-Haasforce [1]. In this study the magnitude of the Einstein de-Haas =
force is
calculated, assuming a spin density in crustal rocks on the order of1035 =
km-3=20
and a rigid 300 km x 300 km crustal block that is 10 km thick.Under =
these=20
conditions a 400 nT (G4-class) solar event is estimated toinduce an =
Einstein-De=20
Haas torque of 1.2 x 1011 N-m. Such large torquesmay trigger earthquakes =
along=20
faults where tectonic stresses are closeto the failure threshold. We =
therefore=20
anticipate that due toEinstein-de Haas coupling, there may be an =
increase in=20
seismic activitywithin a relatively short time window after arrival of =
large=20
magneticstorms. The transient augmentation in crustal stress may also =
manifest
itself in an increase in air ionization at the Earth=E2=80=99s surface =
andother=20
phenomena [2]. Time-series analysis has shown that localseismicity and=20
integrated earthquake energy appear to have periodicitieswith respect to =
local=20
time, possibly due to ionosphere-to-solid Earthcoupling [3]. A similar =
approach=20
will be used to perform a correlationanalysis of seismic events with =
respect to=20
historical CME events. [1] A.Einstein and W. de Haas, =
=E2=80=9CExperimental proof of the=20
existence ofAmp=C3=A8re's molecular currents,=E2=80=9D Proc. Koninklijke =
Akad.Wetenschappen=20
te Amsterdam, 18, 696-711 (1915). [2] F. Freund et al.,=E2=80=9CAir =
ionization at rock=20
surface and pre-earthquake signals,=E2=80=9DJ. Atmos. Sol. Terr. Phys., =
71, 1824-1834=20
(2009). [3] G. Duma and Y.Ruzhin, =E2=80=9CDiurnal changes of earthquake =
activity and=20
geomagneticSq-variations,=E2=80=9D Natural Hazards and Earth System =
Sciences, 3,171-177=20
(2003).
<HR>

<TABLE width=3D"100%">
  <TBODY>
  <TR>
    <TD align=3D"left"><B><A =
href=3D"http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=3D2010AGU=
FMNH13A1141W&amp;data_type=3DBIBTEX&amp;db_key=3DPHY&amp;nocookieset=3D1"=
>Bibtex=20
      entry for this abstract</A></B>&nbsp;&nbsp;&nbsp;<B><A =
href=3D"http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?bibcode=3D2010A=
GUFMNH13A1141W&amp;data_type=3DCustom&amp;format=3D%5c%5cbibitem%5b%25%5c=
2m%25%28y%29%5d%25%7bR%7d%20%25%5c8l%20%25%5cY,%25%5cj,%25%5cV,%25%5cp%5c=
n&amp;return_fmt=3DLONG&amp;db_key=3DPHY&amp;nocookieset=3D1">Preferred=20
      format for this abstract</A></B> (see <A =
href=3D"http://adsabs.harvard.edu/cgi-bin/pref_set">Preferences</A>)</TD>=

  </TR></TBODY></TABLE>
<HR>

<FORM method=3D"POST"=20
action=3D"http://adsabs.harvard.edu/cgi-bin/nph-abs_connect"><A=20
name=3D"private"></A><INPUT name=3D"bibcode" =
value=3D"2010AGUFMNH13A1141W" type=3D"hidden"><INPUT name=3D"library" =
value=3D" Add this article to private library " =
type=3D"submit">&nbsp;&nbsp;&nbsp;<INPUT name=3D"library" value=3D" =
Remove this article from private library " type=3D"submit"><BR>
</FORM>
<HR>

<FORM method=3D"POST"=20
action=3D"http://adsabs.harvard.edu/cgi-bin/nph-abs_connect"><A=20
name=3D"feedback"></A>
<H3>Find Similar Abstracts:</H3><INPUT name=3D"return_req" =
value=3D"no_params" type=3D"hidden">
<TABLE>
  <TBODY>
  <TR>
    <TD>Use:</TD>
    <TD><INPUT name=3D"use_auth" value=3D"YES" type=3D"checkbox"></TD>
    <TD>  Authors</TD></TR>
  <TR>
    <TD></TD>
    <TD><INPUT name=3D"use_title" value=3D"YES" CHECKED=3D"" =
type=3D"checkbox"></TD>
    <TD>  Title</TD></TR>
  <TR>
    <TD></TD>
    <TD><INPUT name=3D"use_kwds" value=3D"YES" CHECKED=3D"" =
type=3D"checkbox"></TD>
    <TD>  Keywords (in text query field)</TD></TR>
  <TR>
    <TD></TD>
    <TD><INPUT name=3D"use_text" value=3D"YES" CHECKED=3D"" =
type=3D"checkbox"></TD>
    <TD>  Abstract Text</TD></TR>
  <TR>
    <TD>Return:</TD>
    <TD><INPUT name=3D"return_req" value=3D"feedback" CHECKED=3D"" =
type=3D"radio"></TD>
    <TD>  Query Results</TD>
    <TD>   Return <INPUT name=3D"nr_to_return" value=3D"100"=20
      size=3D"5">&nbsp;&nbsp;&nbsp;items starting with number <INPUT =
name=3D"start_nr"=20
      value=3D"1" size=3D"5"></TD></TR>
  <TR>
    <TD></TD>
    <TD><INPUT name=3D"return_req" value=3D"form" type=3D"radio"></TD>
    <TD>  Query Form</TD></TR>
  <TR>
    <TD>Database:</TD>
    <TD> <INPUT name=3D"db_key" value=3D"AST" type=3D"checkbox"></TD>
    <TD>  Astronomy</TD></TR>
  <TR>
    <TD></TD>
    <TD><INPUT name=3D"db_key" value=3D"PHY" CHECKED=3D"" =
type=3D"checkbox"></TD>
    <TD>  Physics</TD></TR>
  <TR>
    <TD></TD>
    <TD><INPUT name=3D"db_key" value=3D"PRE" type=3D"checkbox"></TD>
    <TD>  arXiv e-prints</TD></TR></TBODY></TABLE><INPUT =
name=3D"arxiv_sel" value=3D"ALL"=20
type=3D"hidden"><INPUT name=3D"bib_dbkey" value=3D"PHY" =
type=3D"hidden"><INPUT name=3D"selfeedback" value=3D"      Send Query    =
 " type=3D"submit">&nbsp;&nbsp;&nbsp;&nbsp;<INPUT value=3D"      Reset   =
   " type=3D"reset">
<INPUT name=3D"bibcode" value=3D"2010AGUFMNH13A1141W" =
type=3D"hidden"></FORM><BR>
<HR>
<BR></BODY></HTML>
