When do the Fastest type II CME should be detected throughout all the heliosphere?

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if (Float.valueOf(PA_WIDTH).compareTo(Float.valueOf("180")) > 0) {
	width = (Float.valueOf(PA_WIDTH)/Float.valueOf("2")).toString();
}
else {
	width = PA_WIDTH;
}
velocity = ((Float.valueOf(velocity_input)+Float.valueOf(v_diff)+Float.valueOf(v_min))/Float.valueOf("2")).toString();
velocity_error = ((Float.valueOf(velocity_input)+Float.valueOf(v_diff)-Float.valueOf(v_min))/Float.valueOf("2")).toString();

url_out = url_list.get(0).replaceFirst(".xml","data.asc")

Name	Description
time_stop	End time of the interval of interest
time_start	Starting time of the interval of interest

Name	Type	Description
ExtractFastestCME_Wind_typeii_soho_cme	workflow
Empty_LatLong	stringconstant	Value
ExtractProperties_goes_sxr_flare	workflow
LASCO_CME_QUERY	workflow
AverageSpeedFromURL	workflow
Data_from_mission	workflow
CME_Object	workflow
Object_Earth	stringconstant	Value EARTH
ACE_Mission	stringconstant	Value ACE
CalculateWidthFromPA_Width	beanshell	It calculates the Longitudinal width of the CME assuming that the CME is symetrical when PA < 180 degrees, and half when larger. Script if (Float.valueOf(PA_WIDTH).compareTo(Float.valueOf("180")) > 0) { width = (Float.valueOf(PA_WIDTH)/Float.valueOf("2")).toString(); } else { width = PA_WIDTH; }
CalculateNewVelocity	beanshell	Script velocity = ((Float.valueOf(velocity_input)+Float.valueOf(v_diff)+Float.valueOf(v_min))/Float.valueOf("2")).toString(); velocity_error = ((Float.valueOf(velocity_input)+Float.valueOf(v_diff)-Float.valueOf(v_min))/Float.valueOf("2")).toString();
CME_multiple_Output	workflow
Url_to_dataurl	beanshell	modify URL to the URL where the data resides. Script url_out = url_list.get(0).replaceFirst(".xml","data.asc")

Name	Description	Inputs	Outputs
CalculateWidthFromPA_Width	It calculates the Longitudinal width of the CME assuming that the CME is symetrical when PA < 180 degrees, and half when larger.	PA_WIDTH	width
CalculateNewVelocity		velocity_input v_diff v_min	velocity velocity_error
Url_to_dataurl	modify URL to the URL where the data resides.	url_list	url_out
Beanshell_TimesObjectHit	extract times of arrival when the object asked has been hit.	ETA_max_List ETA_min_List HitMiss_List Object_List Planet_SC	ETA_max ETA_min
parseVOTable		voTable collumn	valueLists debug collumn
Dummy		dummy
Beanshell_MultipleObjectOutput		ETA_max_List ETA_min_List HitMiss_List Object_List	MERCURY VENUS EARTH SATURN JUPITER ULYSSES STEREOA STEREOB MESSENGER VOYAGER1 VOYAGER2 CASSINI MARS
reformLists		colNames values	ETA_Min_List ETA_Max_List Object_List Hit_List
ExceptionHandling		status
Beanshell		url_list	url
Beanshell		inputTime	startTimeRange endTimeRange
checkLocation		inLat inLong accuracy latList longList	locationStatus log
reformLists		colNames values	latList longList peakTimeList
reformLists		colNames values	ETA_Min_List ETA_Max_List Object_List Hit_List
Beanshell_AverageSpeed		text	debug vel_av
Beanshell_JoinTimes_SQL		start_t end_t condition	WHERE
reformLists		colNames values	timeStartList timeEndList xRayClassList
Beanshell_JoinTimes_SQL		start_t end_t condition	WHERE
reformLists		colNames values	paList paWidthList vDiffList vFinalList

Name	Description
Saturn
Messenger
Mercury
Mars
Jupiter
Earth
Cassini
StereoA
StereoB
Venus
Voyager1
Voyager2
Plot_Inner
Plot_Outer
Plot_Voyager
Sun_StartTime

Source	Sink
time_start	ExtractFastestCME_Wind_typeii_soho_cme:time_start
time_stop	ExtractFastestCME_Wind_typeii_soho_cme:time_stop
ExtractFastestCME_Wind_typeii_soho_cme:xray_class	ExtractProperties_goes_sxr_flare:xrayClassInput
Empty_LatLong:value	ExtractProperties_goes_sxr_flare:inputLongitude
Empty_LatLong:value	ExtractProperties_goes_sxr_flare:inputLatitude
ExtractFastestCME_Wind_typeii_soho_cme:time_start	ExtractProperties_goes_sxr_flare:inputTime
ExtractFastestCME_Wind_typeii_soho_cme:time_start	LASCO_CME_QUERY:start_time
ExtractFastestCME_Wind_typeii_soho_cme:time_stop	LASCO_CME_QUERY:end_time
Url_to_dataurl:url_out	AverageSpeedFromURL:url
CME_Object:ETA_max	Data_from_mission:ENDTIME
CME_Object:ETA_min	Data_from_mission:STARTTIME
ACE_Mission:value	Data_from_mission:MISSION
Object_Earth:value	CME_Object:Planet_SC
LASCO_CME_QUERY:v_final	CME_Object:cme_v
LASCO_CME_QUERY:v_diff	CME_Object:cme_v_error
ExtractProperties_goes_sxr_flare:peak_time	CME_Object:start_time
ExtractProperties_goes_sxr_flare:long_hg	CME_Object:CME_starting_position
CalculateWidthFromPA_Width:width	CME_Object:cme_width
LASCO_CME_QUERY:pa_width	CalculateWidthFromPA_Width:PA_WIDTH
AverageSpeedFromURL:average_sw_vel	CalculateNewVelocity:v_min
LASCO_CME_QUERY:v_final	CalculateNewVelocity:velocity_input
LASCO_CME_QUERY:v_diff	CalculateNewVelocity:v_diff
CalculateNewVelocity:velocity_error	CME_multiple_Output:cme_v_error
CalculateNewVelocity:velocity	CME_multiple_Output:cme_v
CalculateWidthFromPA_Width:width	CME_multiple_Output:cme_width
ExtractProperties_goes_sxr_flare:peak_time	CME_multiple_Output:start_time
ExtractProperties_goes_sxr_flare:long_hg	CME_multiple_Output:cme_position
Data_from_mission:url	Url_to_dataurl:url_list
CME_multiple_Output:Saturn	Saturn
CME_multiple_Output:Messenger	Messenger
CME_multiple_Output:Mercury	Mercury
CME_multiple_Output:Mars	Mars
CME_multiple_Output:Jupiter	Jupiter
CME_multiple_Output:Earth	Earth
CME_multiple_Output:Cassini	Cassini
CME_multiple_Output:StereoA	StereoA
CME_multiple_Output:StereoB	StereoB
CME_multiple_Output:Venus	Venus
CME_multiple_Output:Voyager1	Voyager1
CME_multiple_Output:Voyager2	Voyager2
CME_multiple_Output:Plot_inner	Plot_Inner
CME_multiple_Output:Plot_outer	Plot_Outer
CME_multiple_Output:Plot_voyager	Plot_Voyager
ExtractProperties_goes_sxr_flare:peak_time	Sun_StartTime

When do the Fastest type II CME should be detected throughout all the heliosphere?

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