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
reformLists		colNames values	ETA_Min_List ETA_Max_List Object_List Hit_List
Dummy		dummy
checkLocation		inLat inLong accuracy latList longList	locationStatus log
reformLists		colNames values	latList longList peakTimeList
Beanshell_JoinTimes_SQL		start_t end_t condition	WHERE
reformLists		colNames values	paList paWidthList vDiffList vFinalList
ExceptionHandling		status
Beanshell		url_list	url
Beanshell_JoinTimes_SQL		start_t end_t condition	WHERE
reformLists		colNames values	timeStartList timeEndList xRayClassList
Beanshell_AverageSpeed		text	debug vel_av
Dummy		dummy
reformLists		colNames values	ETA_Min_List ETA_Max_List Object_List Hit_List
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
Beanshell		inputTime	startTimeRange endTimeRange

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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