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	<id>https://gem.epss.ucla.edu/mediawiki/api.php?action=feedcontributions&amp;feedformat=atom&amp;user=Wiltbemj</id>
	<title>gem - User contributions [en]</title>
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	<updated>2026-05-06T02:53:24Z</updated>
	<subtitle>User contributions</subtitle>
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	<entry>
		<id>https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&amp;diff=535</id>
		<title>GEM Focus Groups</title>
		<link rel="alternate" type="text/html" href="https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&amp;diff=535"/>
		<updated>2009-08-14T15:06:04Z</updated>

		<summary type="html">&lt;p&gt;Wiltbemj: /* GEM Planning Activities */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;# [[FG1. GGCM Metrics and Validation|GGCM Metrics and Validation]] (2005 - 2010, RA: [[RA-GGCM|GGCM]])&lt;br /&gt;
# [[FG2. GGCM Modules and Methods|GGCM Modules and Methods]] (2005 - 2010, RA: [[RA-GGCM|GGCM]])&lt;br /&gt;
# [[FG3. Foreshock, Bowshock, Magnetosheath|Foreshock, Bowshock, Magnetosheath]] (2004 - 2009, RA: [[RA-Dayside|Dayside]])&lt;br /&gt;
# [[FG4. Plasma Entry and Transport into and within the Magnetotail|Plasma Entry and Transport into and within the Magnetotail]] (2006 - 2011, RA: [[RA-Tail|Tail]])&lt;br /&gt;
# [[FG5. Dayside Magnetopause Reconnection|Dayside Magnetopause Reconnection]] (2004 - 2009, RA: [[RA-Dayside|Dayside]])&lt;br /&gt;
# [[FG6. Cusp Physics|Cusp Physics]] (2006-2010, RA: [[RA-Dayside|Dayside]])&lt;br /&gt;
# [[FG7. MIC Electrodynamics|MIC Electrodynamics]] (2003 - 2008, RA: [[RA-MIC|MIC]])&lt;br /&gt;
# [[FG8. Near Earth Magnetosphere: plasma, fields, and coupling|Near Earth Magnetosphere: plasma, fields, and coupling]] (2007 - 2012, RA: [[RA-IMS|IMS]], [[RA-Tail|Tail]])&lt;br /&gt;
# [http://virbo.org/wiki/index.php/GEMFG9 Space Radiation Climatology] (2006 - 2011, RA: [[RA-IMS|IMS]], see also [http://groups.google.com/group/gem-2007-space-radiation-climatology-fg9  FG9 google email group])&lt;br /&gt;
# [[FG10. Diffuse Auroral Precipitation|Diffuse Auroral Precipitation]] (2006 - 2011, RA: [[RA-MIC|MIC]], [[RA-IMS|IMS]])&lt;br /&gt;
# [[FG11. Plasmasphere-Magnetosphere Interactions|Plasmasphere-Magnetosphere Interactions]] (2008 - 2013, RA: [[RA-IMS|IMS]])&lt;br /&gt;
# [[FG12. Substorm Expansion Onset: The First 10 Minutes|Substorm Expansion Onset: The First 10 Minutes]] (2008 - 2013, RA: [[RA-Tail|Tail]])&lt;br /&gt;
# [[FG13. Modes of Solar WInd-Magnetosphere Energy Transfer|Modes of Solar WInd-Magnetosphere Energy Transfer]] (2008 - 2013, RA: [[RA-Tail|Tail]])&lt;br /&gt;
&lt;br /&gt;
(RA: Research Area)&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
==GEM Planning Activities==&lt;br /&gt;
&lt;br /&gt;
# [[Geospace System]] - W. Lotko and G. Siscoe (Development work 2009)&lt;/div&gt;</summary>
		<author><name>Wiltbemj</name></author>
		
	</entry>
	<entry>
		<id>https://gem.epss.ucla.edu/mediawiki/index.php?title=Geospace_System&amp;diff=534</id>
		<title>Geospace System</title>
		<link rel="alternate" type="text/html" href="https://gem.epss.ucla.edu/mediawiki/index.php?title=Geospace_System&amp;diff=534"/>
		<updated>2009-08-14T15:04:51Z</updated>

		<summary type="html">&lt;p&gt;Wiltbemj: /* '''Geospace System''' */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Geospace System is a potential new focus group for the GEM community.  In this space we can developed the focus group proposal which will be considered by the Steering Community as part of its process in selecting new focus groups.&lt;br /&gt;
&lt;br /&gt;
As a starting point here is the initial announcement from the GEM messenger describing the discussion session held at the 2009 GEM Meeting.&lt;br /&gt;
&lt;br /&gt;
== Prospectus for a GEM Focus Group on the &amp;quot;Geospace System&amp;quot; ==&lt;br /&gt;
 &lt;br /&gt;
Session Organizers Bill Lotko and George Siscoe&lt;br /&gt;
&lt;br /&gt;
We would like to initiate a discussion among the magnetospheric and aeronomy&lt;br /&gt;
communities (portions, at least) on the prospect of undertaking a global,&lt;br /&gt;
system-dynamics study of the coupled solar&lt;br /&gt;
wind-magnetosphere-ionosphere-thermosphere system, which we identify simply&lt;br /&gt;
as the geospace system.  The suggestion responds to two circumstances:&lt;br /&gt;
first, 50 years of magnetospheric research have shown the geospace system to&lt;br /&gt;
be interactively coupled in multiple ways from the solar wind to the&lt;br /&gt;
thermosphere, and second, as GEM moves in its long-range program from the&lt;br /&gt;
'divide-and-conquer' stage to the more challenging synthesis stage, a focus&lt;br /&gt;
group devoted to problems of the coupled system will leverage scientific&lt;br /&gt;
progress in each GEM research area.  The magnitude of the task to comprehend&lt;br /&gt;
the global system in its coupled complexity is almost certainly too great&lt;br /&gt;
for a single, scientist-centered research team and probably too great for&lt;br /&gt;
the multiple teams of a single institution. Instead it would seem to require&lt;br /&gt;
a sustained collaborative effort by experts of manifold specialties&lt;br /&gt;
distributed among many institutions. It might even take the combined&lt;br /&gt;
collaboration of the GEM community and a sizable portion of the CEDAR&lt;br /&gt;
community.  &lt;br /&gt;
&lt;br /&gt;
The priorities of such a focus group clearly must be enlightened by&lt;br /&gt;
community interest. To begin the conversation we can suggest among many&lt;br /&gt;
possible directions several problems, each global in scope and of&lt;br /&gt;
considerable current interest . We have asked some GEM participants to help&lt;br /&gt;
initiate the discussion with a few slides on each problem. They include: 1)&lt;br /&gt;
the dayside reconnection potential, its relationship to the polar cap&lt;br /&gt;
potential, and the saturation of both at large IMF; 2) global resonance,&lt;br /&gt;
periodicity of the magnetospheric response, and sawtooth phenomena; 3)&lt;br /&gt;
ionospheric-magnetospheric plasma circulation, including ionospheric&lt;br /&gt;
outflows, and its effects on plasmasheet and inner magnetospheric dynamics;&lt;br /&gt;
and 4) prompt penetration electric fields and their relationship to the&lt;br /&gt;
dayside ionospheric superfountain, storm enhanced density, and plasmaspheric&lt;br /&gt;
plumes. While some aspects of these global problems can be treated as&lt;br /&gt;
regional phenomena, differentiated by distinct physical processes, their&lt;br /&gt;
dynamics seem to evolve as an integrated whole during extreme solar wind&lt;br /&gt;
conditions. The geospace system thus behaves coherently across a broad&lt;br /&gt;
spatiotemporal range, making it difficult to unravel its causal behavior by&lt;br /&gt;
considering the response in terms of isolated elements or processes.&lt;br /&gt;
Integration of global problems of this type into a system-dynamics picture&lt;br /&gt;
spans the expertise of all five GEM research areas and several CEDAR working&lt;br /&gt;
groups. We invite participation from the GEM community in deciding whether&lt;br /&gt;
the time is right for this focus group, and, if so, how best to structure&lt;br /&gt;
its direction.&lt;/div&gt;</summary>
		<author><name>Wiltbemj</name></author>
		
	</entry>
	<entry>
		<id>https://gem.epss.ucla.edu/mediawiki/index.php?title=Geospace_System&amp;diff=533</id>
		<title>Geospace System</title>
		<link rel="alternate" type="text/html" href="https://gem.epss.ucla.edu/mediawiki/index.php?title=Geospace_System&amp;diff=533"/>
		<updated>2009-08-14T15:04:29Z</updated>

		<summary type="html">&lt;p&gt;Wiltbemj: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== '''Geospace System''' ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Geospace System is a potential new focus group for the GEM community.  In this space we can developed the focus group proposal which will be considered by the Steering Community as part of its process in selecting new focus groups.&lt;br /&gt;
&lt;br /&gt;
As a starting point here is the initial announcement from the GEM messenger describing the discussion session held at the 2009 GEM Meeting.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Prospectus for a GEM Focus Group on the &amp;quot;Geospace System&amp;quot; ==&lt;br /&gt;
 &lt;br /&gt;
Session Organizers Bill Lotko and George Siscoe&lt;br /&gt;
&lt;br /&gt;
We would like to initiate a discussion among the magnetospheric and aeronomy&lt;br /&gt;
communities (portions, at least) on the prospect of undertaking a global,&lt;br /&gt;
system-dynamics study of the coupled solar&lt;br /&gt;
wind-magnetosphere-ionosphere-thermosphere system, which we identify simply&lt;br /&gt;
as the geospace system.  The suggestion responds to two circumstances:&lt;br /&gt;
first, 50 years of magnetospheric research have shown the geospace system to&lt;br /&gt;
be interactively coupled in multiple ways from the solar wind to the&lt;br /&gt;
thermosphere, and second, as GEM moves in its long-range program from the&lt;br /&gt;
'divide-and-conquer' stage to the more challenging synthesis stage, a focus&lt;br /&gt;
group devoted to problems of the coupled system will leverage scientific&lt;br /&gt;
progress in each GEM research area.  The magnitude of the task to comprehend&lt;br /&gt;
the global system in its coupled complexity is almost certainly too great&lt;br /&gt;
for a single, scientist-centered research team and probably too great for&lt;br /&gt;
the multiple teams of a single institution. Instead it would seem to require&lt;br /&gt;
a sustained collaborative effort by experts of manifold specialties&lt;br /&gt;
distributed among many institutions. It might even take the combined&lt;br /&gt;
collaboration of the GEM community and a sizable portion of the CEDAR&lt;br /&gt;
community.  &lt;br /&gt;
&lt;br /&gt;
The priorities of such a focus group clearly must be enlightened by&lt;br /&gt;
community interest. To begin the conversation we can suggest among many&lt;br /&gt;
possible directions several problems, each global in scope and of&lt;br /&gt;
considerable current interest . We have asked some GEM participants to help&lt;br /&gt;
initiate the discussion with a few slides on each problem. They include: 1)&lt;br /&gt;
the dayside reconnection potential, its relationship to the polar cap&lt;br /&gt;
potential, and the saturation of both at large IMF; 2) global resonance,&lt;br /&gt;
periodicity of the magnetospheric response, and sawtooth phenomena; 3)&lt;br /&gt;
ionospheric-magnetospheric plasma circulation, including ionospheric&lt;br /&gt;
outflows, and its effects on plasmasheet and inner magnetospheric dynamics;&lt;br /&gt;
and 4) prompt penetration electric fields and their relationship to the&lt;br /&gt;
dayside ionospheric superfountain, storm enhanced density, and plasmaspheric&lt;br /&gt;
plumes. While some aspects of these global problems can be treated as&lt;br /&gt;
regional phenomena, differentiated by distinct physical processes, their&lt;br /&gt;
dynamics seem to evolve as an integrated whole during extreme solar wind&lt;br /&gt;
conditions. The geospace system thus behaves coherently across a broad&lt;br /&gt;
spatiotemporal range, making it difficult to unravel its causal behavior by&lt;br /&gt;
considering the response in terms of isolated elements or processes.&lt;br /&gt;
Integration of global problems of this type into a system-dynamics picture&lt;br /&gt;
spans the expertise of all five GEM research areas and several CEDAR working&lt;br /&gt;
groups. We invite participation from the GEM community in deciding whether&lt;br /&gt;
the time is right for this focus group, and, if so, how best to structure&lt;br /&gt;
its direction.&lt;/div&gt;</summary>
		<author><name>Wiltbemj</name></author>
		
	</entry>
	<entry>
		<id>https://gem.epss.ucla.edu/mediawiki/index.php?title=Geospace_System&amp;diff=532</id>
		<title>Geospace System</title>
		<link rel="alternate" type="text/html" href="https://gem.epss.ucla.edu/mediawiki/index.php?title=Geospace_System&amp;diff=532"/>
		<updated>2009-08-14T15:02:53Z</updated>

		<summary type="html">&lt;p&gt;Wiltbemj: New page: '''Geospace System'''  Geospace System is a potential new focus group for the GEM community.  In this space we can developed the focus group proposal which will be considered by the Steeri...&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;'''Geospace System'''&lt;br /&gt;
&lt;br /&gt;
Geospace System is a potential new focus group for the GEM community.  In this space we can developed the focus group proposal which will be considered by the Steering Community as part of its process in selecting new focus groups.&lt;br /&gt;
&lt;br /&gt;
As a starting point here is the initial announcement from the GEM messenger describing the discussion session held at the 2009 GEM Meeting.&lt;br /&gt;
&lt;br /&gt;
Prospectus for a GEM Focus Group on the &amp;quot;Geospace System&amp;quot; &lt;br /&gt;
Bill Lotko, wlotko@dartmouth.edu and George Siscoe, siscoe@skynet.bu.edu&lt;br /&gt;
&lt;br /&gt;
We would like to initiate a discussion among the magnetospheric and aeronomy&lt;br /&gt;
communities (portions, at least) on the prospect of undertaking a global,&lt;br /&gt;
system-dynamics study of the coupled solar&lt;br /&gt;
wind-magnetosphere-ionosphere-thermosphere system, which we identify simply&lt;br /&gt;
as the geospace system.  The suggestion responds to two circumstances:&lt;br /&gt;
first, 50 years of magnetospheric research have shown the geospace system to&lt;br /&gt;
be interactively coupled in multiple ways from the solar wind to the&lt;br /&gt;
thermosphere, and second, as GEM moves in its long-range program from the&lt;br /&gt;
'divide-and-conquer' stage to the more challenging synthesis stage, a focus&lt;br /&gt;
group devoted to problems of the coupled system will leverage scientific&lt;br /&gt;
progress in each GEM research area.  The magnitude of the task to comprehend&lt;br /&gt;
the global system in its coupled complexity is almost certainly too great&lt;br /&gt;
for a single, scientist-centered research team and probably too great for&lt;br /&gt;
the multiple teams of a single institution. Instead it would seem to require&lt;br /&gt;
a sustained collaborative effort by experts of manifold specialties&lt;br /&gt;
distributed among many institutions. It might even take the combined&lt;br /&gt;
collaboration of the GEM community and a sizable portion of the CEDAR&lt;br /&gt;
community.  &lt;br /&gt;
&lt;br /&gt;
The priorities of such a focus group clearly must be enlightened by&lt;br /&gt;
community interest. To begin the conversation we can suggest among many&lt;br /&gt;
possible directions several problems, each global in scope and of&lt;br /&gt;
considerable current interest . We have asked some GEM participants to help&lt;br /&gt;
initiate the discussion with a few slides on each problem. They include: 1)&lt;br /&gt;
the dayside reconnection potential, its relationship to the polar cap&lt;br /&gt;
potential, and the saturation of both at large IMF; 2) global resonance,&lt;br /&gt;
periodicity of the magnetospheric response, and sawtooth phenomena; 3)&lt;br /&gt;
ionospheric-magnetospheric plasma circulation, including ionospheric&lt;br /&gt;
outflows, and its effects on plasmasheet and inner magnetospheric dynamics;&lt;br /&gt;
and 4) prompt penetration electric fields and their relationship to the&lt;br /&gt;
dayside ionospheric superfountain, storm enhanced density, and plasmaspheric&lt;br /&gt;
plumes. While some aspects of these global problems can be treated as&lt;br /&gt;
regional phenomena, differentiated by distinct physical processes, their&lt;br /&gt;
dynamics seem to evolve as an integrated whole during extreme solar wind&lt;br /&gt;
conditions. The geospace system thus behaves coherently across a broad&lt;br /&gt;
spatiotemporal range, making it difficult to unravel its causal behavior by&lt;br /&gt;
considering the response in terms of isolated elements or processes.&lt;br /&gt;
Integration of global problems of this type into a system-dynamics picture&lt;br /&gt;
spans the expertise of all five GEM research areas and several CEDAR working&lt;br /&gt;
groups. We invite participation from the GEM community in deciding whether&lt;br /&gt;
the time is right for this focus group, and, if so, how best to structure&lt;br /&gt;
its direction.&lt;/div&gt;</summary>
		<author><name>Wiltbemj</name></author>
		
	</entry>
	<entry>
		<id>https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&amp;diff=531</id>
		<title>GEM Focus Groups</title>
		<link rel="alternate" type="text/html" href="https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&amp;diff=531"/>
		<updated>2009-08-14T15:00:12Z</updated>

		<summary type="html">&lt;p&gt;Wiltbemj: /* GEM Planning Activities */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;# [[FG1. GGCM Metrics and Validation|GGCM Metrics and Validation]] (2005 - 2010, RA: [[RA-GGCM|GGCM]])&lt;br /&gt;
# [[FG2. GGCM Modules and Methods|GGCM Modules and Methods]] (2005 - 2010, RA: [[RA-GGCM|GGCM]])&lt;br /&gt;
# [[FG3. Foreshock, Bowshock, Magnetosheath|Foreshock, Bowshock, Magnetosheath]] (2004 - 2009, RA: [[RA-Dayside|Dayside]])&lt;br /&gt;
# [[FG4. Plasma Entry and Transport into and within the Magnetotail|Plasma Entry and Transport into and within the Magnetotail]] (2006 - 2011, RA: [[RA-Tail|Tail]])&lt;br /&gt;
# [[FG5. Dayside Magnetopause Reconnection|Dayside Magnetopause Reconnection]] (2004 - 2009, RA: [[RA-Dayside|Dayside]])&lt;br /&gt;
# [[FG6. Cusp Physics|Cusp Physics]] (2006-2010, RA: [[RA-Dayside|Dayside]])&lt;br /&gt;
# [[FG7. MIC Electrodynamics|MIC Electrodynamics]] (2003 - 2008, RA: [[RA-MIC|MIC]])&lt;br /&gt;
# [[FG8. Near Earth Magnetosphere: plasma, fields, and coupling|Near Earth Magnetosphere: plasma, fields, and coupling]] (2007 - 2012, RA: [[RA-IMS|IMS]], [[RA-Tail|Tail]])&lt;br /&gt;
# [http://virbo.org/wiki/index.php/GEMFG9 Space Radiation Climatology] (2006 - 2011, RA: [[RA-IMS|IMS]], see also [http://groups.google.com/group/gem-2007-space-radiation-climatology-fg9  FG9 google email group])&lt;br /&gt;
# [[FG10. Diffuse Auroral Precipitation|Diffuse Auroral Precipitation]] (2006 - 2011, RA: [[RA-MIC|MIC]], [[RA-IMS|IMS]])&lt;br /&gt;
# [[FG11. Plasmasphere-Magnetosphere Interactions|Plasmasphere-Magnetosphere Interactions]] (2008 - 2013, RA: [[RA-IMS|IMS]])&lt;br /&gt;
# [[FG12. Substorm Expansion Onset: The First 10 Minutes|Substorm Expansion Onset: The First 10 Minutes]] (2008 - 2013, RA: [[RA-Tail|Tail]])&lt;br /&gt;
# [[FG13. Modes of Solar WInd-Magnetosphere Energy Transfer|Modes of Solar WInd-Magnetosphere Energy Transfer]] (2008 - 2013, RA: [[RA-Tail|Tail]])&lt;br /&gt;
&lt;br /&gt;
(RA: Research Area)&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
==GEM Planning Activities==&lt;br /&gt;
&lt;br /&gt;
1 - [[Geospace System]] W. Lotko and G. Siscoe&lt;/div&gt;</summary>
		<author><name>Wiltbemj</name></author>
		
	</entry>
	<entry>
		<id>https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&amp;diff=530</id>
		<title>GEM Focus Groups</title>
		<link rel="alternate" type="text/html" href="https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&amp;diff=530"/>
		<updated>2009-08-14T14:57:20Z</updated>

		<summary type="html">&lt;p&gt;Wiltbemj: /* GEM Planning Activities */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;# [[FG1. GGCM Metrics and Validation|GGCM Metrics and Validation]] (2005 - 2010, RA: [[RA-GGCM|GGCM]])&lt;br /&gt;
# [[FG2. GGCM Modules and Methods|GGCM Modules and Methods]] (2005 - 2010, RA: [[RA-GGCM|GGCM]])&lt;br /&gt;
# [[FG3. Foreshock, Bowshock, Magnetosheath|Foreshock, Bowshock, Magnetosheath]] (2004 - 2009, RA: [[RA-Dayside|Dayside]])&lt;br /&gt;
# [[FG4. Plasma Entry and Transport into and within the Magnetotail|Plasma Entry and Transport into and within the Magnetotail]] (2006 - 2011, RA: [[RA-Tail|Tail]])&lt;br /&gt;
# [[FG5. Dayside Magnetopause Reconnection|Dayside Magnetopause Reconnection]] (2004 - 2009, RA: [[RA-Dayside|Dayside]])&lt;br /&gt;
# [[FG6. Cusp Physics|Cusp Physics]] (2006-2010, RA: [[RA-Dayside|Dayside]])&lt;br /&gt;
# [[FG7. MIC Electrodynamics|MIC Electrodynamics]] (2003 - 2008, RA: [[RA-MIC|MIC]])&lt;br /&gt;
# [[FG8. Near Earth Magnetosphere: plasma, fields, and coupling|Near Earth Magnetosphere: plasma, fields, and coupling]] (2007 - 2012, RA: [[RA-IMS|IMS]], [[RA-Tail|Tail]])&lt;br /&gt;
# [http://virbo.org/wiki/index.php/GEMFG9 Space Radiation Climatology] (2006 - 2011, RA: [[RA-IMS|IMS]], see also [http://groups.google.com/group/gem-2007-space-radiation-climatology-fg9  FG9 google email group])&lt;br /&gt;
# [[FG10. Diffuse Auroral Precipitation|Diffuse Auroral Precipitation]] (2006 - 2011, RA: [[RA-MIC|MIC]], [[RA-IMS|IMS]])&lt;br /&gt;
# [[FG11. Plasmasphere-Magnetosphere Interactions|Plasmasphere-Magnetosphere Interactions]] (2008 - 2013, RA: [[RA-IMS|IMS]])&lt;br /&gt;
# [[FG12. Substorm Expansion Onset: The First 10 Minutes|Substorm Expansion Onset: The First 10 Minutes]] (2008 - 2013, RA: [[RA-Tail|Tail]])&lt;br /&gt;
# [[FG13. Modes of Solar WInd-Magnetosphere Energy Transfer|Modes of Solar WInd-Magnetosphere Energy Transfer]] (2008 - 2013, RA: [[RA-Tail|Tail]])&lt;br /&gt;
&lt;br /&gt;
(RA: Research Area)&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
==GEM Planning Activities==&lt;br /&gt;
&lt;br /&gt;
1 - [[Global Dynamics]] W. Lotko and G. Siscoe&lt;/div&gt;</summary>
		<author><name>Wiltbemj</name></author>
		
	</entry>
</feed>