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Showing 32 changed files with 61 additions and 640 deletions.
Binary file added GameData/RP-0/Parts - Shortcut.lnk
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18 changes: 2 additions & 16 deletions GameData/RP-0/Parts/Science/IR01-IRRadiometer.cfg
Original file line number Diff line number Diff line change
@@ -31,7 +31,7 @@ PART
subcategory = 0
title = Infrared Radiometer
manufacturer = Bluedog Design Bureau
description = The Infrared Radiometer measures the thermal emmisions and temperatures of the cloud tops as well as the surface features. Historically, this experiment is based on the one flown on Mariner 2.\nThe science can be transmitted for full recovery. Level 1 Infrared Radiometer Experiment. Can gather 25% of Infrared Radiometer Science.
description = The Infrared Radiometer measures the thermal emmisions and temperatures of the cloud tops as well as the surface features. Historically, this experiment is based on the one flown on Mariner 2.\n\nThe science can be transmitted for full recovery. Level 1 Infrared Radiometer Experiment. Can gather 25% of Infrared Radiometer Science.
attachRules = 0,1,0,0,1
mass = 0.0013
dragModelType = default
@@ -44,19 +44,5 @@ PART

tags = science bdb bluedog infrared IR radiometer nimbus mariner

MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-infraredRad1
experimentActionName = Infrared Radiometer Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}

}
35 changes: 2 additions & 33 deletions GameData/RP-0/Parts/Science/IR02-HRIRRadiometer.cfg
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@@ -37,7 +37,7 @@ PART
subcategory = 0
title = High-Resolution Infrared Radiometer
manufacturer = Coatl Aerospace
description = The High-Resolution Infrared Radiometer is improved equipment that measures the thermal emmisions and temperatures of the cloud tops as well as the surface features. Historically, this experiment is based on the ones flown on the NIMBUS satellites.\nThe science can be transmitted for full recovery. Level 2 Infrared Radiometer Experiment can gather 50% of Infrared Radiometer Science.
description = The High-Resolution Infrared Radiometer is improved equipment that measures the thermal emmisions and temperatures of the cloud tops as well as the surface features. Historically, this experiment is based on the ones flown on the NIMBUS satellites.\n\nThe science can be transmitted for full recovery. Level 2 Infrared Radiometer Experiment can gather 50% of Infrared Radiometer Science.

mass = 0.0051
bulkheadProfiles = size0, srf
@@ -53,38 +53,7 @@ PART
PhysicsSignificance = 1

tags = coatl science infrared IR radiometer nimbus

MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-infraredRad1
experimentActionName = Infrared Radiometer Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-infraredRad2
experimentActionName = Infrared Radiometer Level 2
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}


MODULE
{
name = ModuleAnimateGeneric
49 changes: 2 additions & 47 deletions GameData/RP-0/Parts/Science/IR03-TwoChannelIR.cfg
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@@ -36,7 +36,7 @@ PART
subcategory = 0
title = Two-Channel Infrared Radiometer
manufacturer = Coatl Aerospace
description = The Two-Channel Infrared Radiometer observes and records the thermal emissions from planetary bodies in two broad spectral bands. Historically, this experiment is based on the one flown on Mariner 10.\nThe science can be transmitted for full recovery. Level 3 Infrared Radiometer Experiment can gather 75% of Infrared Radiometer Science.
description = The Two-Channel Infrared Radiometer observes and records the thermal emissions from planetary bodies in two broad spectral bands. Historically, this experiment is based on the one flown on Mariner 10.\n\nThe science can be transmitted for full recovery. Level 3 Infrared Radiometer Experiment can gather 75% of Infrared Radiometer Science.

mass = 0.0036
dragModelType = default
@@ -50,50 +50,5 @@ PART

tags = coatl science ir infrared radiometer mariner venus mercury thermal emission

MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-infraredRad1
experimentActionName = Infrared Radiometer Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-infraredRad2
experimentActionName = Infrared Radiometer Level 2
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-infraredRad3
experimentActionName = Infrared Radiometer Level 3
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}


}
2 changes: 1 addition & 1 deletion GameData/RP-0/Parts/Science/IR04-PMIRR.cfg
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@@ -14,7 +14,7 @@
%RSSROConfig = True

@title = Pressure Modulated Infrared Radiometer (PMIRR)
@description = The PMIRR utilized narrow-band radiometric channels and two pressure modulation cells to measure atmospheric and surface emission in the thermal infrared and a visible channel to measure solar radiation reflected from the atmosphere and surface. Historically, this experiment is based on the instrument that flew on Mars Observer.\nThe science can be transmitted for full recovery. Level 4 Infrared Radiometer Experiment can gather 100% of Infrared Radiometer Science.
@description = The PMIRR utilized narrow-band radiometric channels and two pressure modulation cells to measure atmospheric and surface emission in the thermal infrared and a visible channel to measure solar radiation reflected from the atmosphere and surface. Historically, this experiment is based on the instrument that flew on Mars Observer.\n\nThe science can be transmitted for full recovery. Level 4 Infrared Radiometer Experiment can gather 100% of Infrared Radiometer Science.
@mass = 0.0402
@tags = science dmagic pmirr infrared ir radiometer mars observer
@maxTemp = 1073.15
19 changes: 1 addition & 18 deletions GameData/RP-0/Parts/Science/IS01-IRIS.cfg
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@@ -38,7 +38,7 @@ PART
subcategory = 0
title = Infrared Interferometer Spectrometer (IRIS)
manufacturer = Coatl Aerospace
description = The IRIS experiment is used to provide information on the vertical structure, composition, and dynamics of the atmosphere and on the emmissive properties from the surface and atmospheres of planetary bodies in the infrared wavelengths. Historically, these experiments were flown on many craft including NIMBUS 3/4, Mariner 9 and Voyager 1/2 as well as other Earth Satellites.\nThe science can be transmitted for full recovery. Level 1 Imaging Spectrometry Experiment can gather 25% of Mass Spectrometry Science.
description = The IRIS experiment is used to provide information on the vertical structure, composition, and dynamics of the atmosphere and on the emmissive properties from the surface and atmospheres of planetary bodies in the infrared wavelengths. Historically, these experiments were flown on many craft including NIMBUS 3/4, Mariner 9 and Voyager 1/2 as well as other Earth Satellites.\n\nThe science can be transmitted for full recovery. Level 1 Imaging Spectrometry Experiment can gather 25% of Mass Spectrometry Science.

mass = 0.018
bulkheadProfiles = size0, srf
@@ -55,21 +55,4 @@ PART

tags = coatl infrared IR spectrometer iris science nimbus voyager mariner

MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-imageSpec1
experimentActionName = Image Spectrometry Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}


}
33 changes: 1 addition & 32 deletions GameData/RP-0/Parts/Science/IS02-UVSpectrometer.cfg
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@@ -31,7 +31,7 @@ PART
subcategory = 0
title = Ultraviolet Spectrometer
manufacturer = Bluedog Design Bureau
description = The UV Spectrometer experiment is used to provide information on the vertical structure, composition, and dynamics of the atmosphere and on the emmissive properties from the surface and atmospheres of planetary bodies in the ultraviolet wavelengths. Historically, these experiments were flown on many craft including Mariner 10.\nThe science can be transmitted for full recovery. Level 2 Imaging Spectrometry Experiment. Can gather 50% of Mass Spectrometry Science.
description = The UV Spectrometer experiment is used to provide information on the vertical structure, composition, and dynamics of the atmosphere and on the emmissive properties from the surface and atmospheres of planetary bodies in the ultraviolet wavelengths. Historically, these experiments were flown on many craft including Mariner 10.\n\nThe science can be transmitted for full recovery. Level 2 Imaging Spectrometry Experiment. Can gather 50% of Mass Spectrometry Science.
attachRules = 0,1,0,0,1
mass = 0.0055
dragModelType = default
@@ -44,36 +44,5 @@ PART

tags = science uv ultraviolet spectrometer bdb bluedog

MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-imageSpec1
experimentActionName = Image Spectrometry Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-imageSpec2
experimentActionName = Image Spectrometry Level 2
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}


}
49 changes: 1 addition & 48 deletions GameData/RP-0/Parts/Science/IS03-NIMS.cfg
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@@ -36,7 +36,7 @@ PART
subcategory = 0
title = Near Infrared Mapping Spectrometer (NIMS)
manufacturer = Coatl Aerospace
description = The NIMS experiment is used to provide information on the vertical structure, composition, and dynamics of the atmosphere and on the emmissive properties from the surface and atmospheres of planetary bodies in the infrared wavelengths. Historically, these experiments were flown on many craft including Galileo.\nThe science can be transmitted for full recovery. Level 3 Imaging Spectrometry Experiment. Can gather 75% of Mass Spectrometry Science.
description = The NIMS experiment is used to provide information on the vertical structure, composition, and dynamics of the atmosphere and on the emmissive properties from the surface and atmospheres of planetary bodies in the infrared wavelengths. Historically, these experiments were flown on many craft including Galileo.\n\nThe science can be transmitted for full recovery. Level 3 Imaging Spectrometry Experiment. Can gather 75% of Mass Spectrometry Science.

mass = 0.0195
bulkheadProfiles = srf
@@ -62,51 +62,4 @@ PART
actionGUIName = Toggle IR Scope
evaDistance = 1.85
}

MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-imageSpec1
experimentActionName = Image Spectrometry Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-imageSpec2
experimentActionName = Image Spectrometry Level 2
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-imageSpec3
experimentActionName = Image Spectrometry Level 3
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}

}
2 changes: 1 addition & 1 deletion GameData/RP-0/Parts/Science/IS04-VIMS.cfg
Original file line number Diff line number Diff line change
@@ -14,7 +14,7 @@
%RSSROConfig = True

@title = Advanced Infrared Mapping Spectrometer (AIMS)
@description = The AIMS experiment is used to provide information on the vertical structure, composition, and dynamics of the atmosphere and on the emmissive properties from the surface and atmospheres of planetary bodies in the infrared wavelengths. Historically, this experiment is based on the instrument that flew on Cassini.\nThe science can be transmitted for full recovery. Level 4 Imaging Spectrometry Experiment. Can gather 100% of Mass Spectrometry Science.
@description = The AIMS experiment is used to provide information on the vertical structure, composition, and dynamics of the atmosphere and on the emmissive properties from the surface and atmospheres of planetary bodies in the infrared wavelengths. Historically, this experiment is based on the instrument that flew on Cassini.\n\nThe science can be transmitted for full recovery. Level 4 Imaging Spectrometry Experiment. Can gather 100% of Mass Spectrometry Science.
@mass = 0.025
@tags = science dmagic vims infrared ir spectrometer cassini
@maxTemp = 1073.15
18 changes: 1 addition & 17 deletions GameData/RP-0/Parts/Science/MAGNET01-EarlyMagnet.cfg
Original file line number Diff line number Diff line change
@@ -34,7 +34,7 @@ PART
subcategory = 0
title = Early Magnetometer Boom
manufacturer = Coatl Aerospace
description = Mounted at the end of this folding boom is the Early Magnetometer, used to measure magnetic fields. Historically, this experiment is based on the ones flown on many early satellite and probe missions.\nThe science can be transmitted for full recovery. Level 1 Magnetometer Experiment can gather 25% of Magnetometer Science.
description = Mounted at the end of this folding boom is the Early Magnetometer, used to measure magnetic fields. Historically, this experiment is based on the ones flown on many early satellite and probe missions.\n\nThe science can be transmitted for full recovery. Level 1 Magnetometer Experiment can gather 25% of Magnetometer Science.

mass = 0.015
bulkheadProfiles = size0, srf
@@ -60,22 +60,6 @@ PART
actionGUIName = Toggle Magnetometer
evaDistance = 1.85
}

MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-magScan1
experimentActionName = Magnetic Scan Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
}


35 changes: 1 addition & 34 deletions GameData/RP-0/Parts/Science/MAGNET02-HeliumMagnet.cfg
Original file line number Diff line number Diff line change
@@ -36,7 +36,7 @@ PART
subcategory = 0
title = Helium Magnetometer Boom
manufacturer = Coatl Aerospace
description = Mounted at the end of this folding boom is the main part of a Helium Vector Magnetometer, used to measure magnetic fields. Historically, this experiment is based on the ones flown on many missions, including Mariner 4.\nThe science can be transmitted for full recovery. Level 2 Magnetometer Experiment can gather 50% of Magnetometer Science.
description = Mounted at the end of this folding boom is the main part of a Helium Vector Magnetometer, used to measure magnetic fields. Historically, this experiment is based on the ones flown on many missions, including Mariner 4.\n\nThe science can be transmitted for full recovery. Level 2 Magnetometer Experiment can gather 50% of Magnetometer Science.

mass = 0.0025
bulkheadProfiles = size0, srf
@@ -62,37 +62,4 @@ PART
actionGUIName = Toggle Magnetometer
evaDistance = 1.85
}

MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-magScan1
experimentActionName = Magnetic Scan Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-magScan2
experimentActionName = Magnetic Scan Level 2
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}


}
2 changes: 1 addition & 1 deletion GameData/RP-0/Parts/Science/MAGNET03-FluxgateMagnet.cfg
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@@ -14,7 +14,7 @@
%RSSROConfig = True

@title = Fluxgate Magnetometer Boom
@description = The magnetometer instruments are used to determine the magnitude and direction of planetary magnetic fields. The long boom separates these instruments from any interference caused by magnetic elements on the craft. Historically, this experiment is based on the instruments that flew on Voyager 1/2 and Galileo.\nThe science can be transmitted for full recovery. Level 2 Magnetometer Experiment can gather 100% of Magnetometer Science.
@description = The magnetometer instruments are used to determine the magnitude and direction of planetary magnetic fields. The long boom separates these instruments from any interference caused by magnetic elements on the craft. Historically, this experiment is based on the instruments that flew on Voyager 1/2 and Galileo.\n\nThe science can be transmitted for full recovery. Level 2 Magnetometer Experiment can gather 100% of Magnetometer Science.
@mass = 0.0056
@tags = science dmagic fluxgate magnet magnetometer voyager galileo
@maxTemp = 1073.15
17 changes: 0 additions & 17 deletions GameData/RP-0/Parts/Science/MM01-Micrometeorite.cfg
Original file line number Diff line number Diff line change
@@ -43,21 +43,4 @@ PART
bulkheadProfiles = srf

tags = micro meterorite micrometerorite detector scanner science bdb bluedog

MODULE
{
name = ModuleScienceExperiment
experimentID = micrometeoriteDetect
experimentActionName = Log Impacts
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}

}
7 changes: 6 additions & 1 deletion GameData/RP-0/Parts/Science/MS01-IonMassSpectrometer.cfg
Original file line number Diff line number Diff line change
@@ -33,7 +33,7 @@ PART
subcategory = 0
title = Ion Mass Spectrometer
manufacturer = Bluedog Design Bureau
description = Commonly called Bennet Radio frequency mass spectrometers, they are only sensitive to charged atoms and molecules since they do not incorporate an ion source. Mass spectrometry is an analytical technique that ionizes chemical species and sorts the ions based on their mass-to-charge ratio. Historically, these simple experiments were flown on many Aerobee sounding rockets and return to Earth for study.\nLevel 1 Mass Spectrometry Experiment. Can gather 25% of Mass Spectrometry Science.
description = Commonly called Bennet Radio frequency mass spectrometers, they are only sensitive to charged atoms and molecules since they do not incorporate an ion source. Mass spectrometry is an analytical technique that ionizes chemical species and sorts the ions based on their mass-to-charge ratio. Historically, these simple experiments were flown on many Aerobee sounding rockets and return to Earth for study.\n\nLevel 1 Mass Spectrometry Experiment. Can gather 25% of Mass Spectrometry Science.
attachRules = 0,1,0,0,1
mass = 0.0041
dragModelType = default
@@ -47,6 +47,11 @@ PART

tags = science ion mass spec spectrometer bennett


}

@PART[RO-IonMassSpectrometer]:FOR[RP-0]
{
MODULE
{
name = ModuleScienceExperiment
34 changes: 1 addition & 33 deletions GameData/RP-0/Parts/Science/MS02-MIMS.cfg
Original file line number Diff line number Diff line change
@@ -36,7 +36,7 @@ PART
subcategory = 0
title = Magnetic Ion-Mass Spectrometer (MIMS)
manufacturer = Coatl Aerospace
description = The MIMS was an improvement on the Bennett Radio version. These had miniaturized magnetic sector field instruments and the mass resolution was much higher than the Bennett RF spectrometer. Mass spectrometry is an analytical technique that ionizes chemical species and sorts the ions based on their mass-to-charge ratio. Historically, these experiments were flown on Explorer 31, AE-C, and other Earth Satellites.\nThe science can be transmitted for full recovery. Level 2 Mass Spectrometry Experiment. Can gather 50% of Mass Spectrometry Science.
description = The MIMS was an improvement on the Bennett Radio version. These had miniaturized magnetic sector field instruments and the mass resolution was much higher than the Bennett RF spectrometer. Mass spectrometry is an analytical technique that ionizes chemical species and sorts the ions based on their mass-to-charge ratio. Historically, these experiments were flown on Explorer 31, AE-C, and other Earth Satellites.\n\nThe science can be transmitted for full recovery. Level 2 Mass Spectrometry Experiment. Can gather 50% of Mass Spectrometry Science.

mass = 0.0075
dragModelType = default
@@ -50,36 +50,4 @@ PART

tags = coatl ca experiment research science spec spectrometer mass neutral ion

MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-massSpec1
experimentActionName = Mass Spectrometry Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-massSpec2
experimentActionName = Mass Spectrometry Level 2
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}


}
49 changes: 1 addition & 48 deletions GameData/RP-0/Parts/Science/MS03-QuadropoleMassSpectrometer.cfg
Original file line number Diff line number Diff line change
@@ -33,7 +33,7 @@ PART
subcategory = 0
title = Quadropole Mass Spectrometer
manufacturer = Bluedog Design Bureau
description = Designed to collect data to determine the composition and structure of positive ions and neutral particles in the upper atmosphere of planets and moons as well as the magnetosphere of planets. Mass spectrometry is an analytical technique that ionizes chemical species and sorts the ions based on their mass-to-charge ratio. Historically, these simple experiments were flown on Earth satellites and interplanetary crafts including the Mars Viking Lander and Cassini.\nLevel 3 Mass Spectrometry Experiment. Can gather 75% of Mass Spectrometry Science.
description = Designed to collect data to determine the composition and structure of positive ions and neutral particles in the upper atmosphere of planets and moons as well as the magnetosphere of planets. Mass spectrometry is an analytical technique that ionizes chemical species and sorts the ions based on their mass-to-charge ratio. Historically, these simple experiments were flown on Earth satellites and interplanetary crafts including the Mars Viking Lander and Cassini.\n\nLevel 3 Mass Spectrometry Experiment. Can gather 75% of Mass Spectrometry Science.
attachRules = 0,1,0,0,1
mass = 0.0098
dragModelType = default
@@ -47,52 +47,5 @@ PART

tags = science ion mass spec spectrometer quadropole cassini viking

MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-massSpec1
experimentActionName = Mass Spectrometry Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-massSpec2
experimentActionName = Mass Spectrometry Level 2
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-massSpec3
experimentActionName = Mass Spectrometry Level 3
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}



}
2 changes: 1 addition & 1 deletion GameData/RP-0/Parts/Science/MS04-GC-MS.cfg
Original file line number Diff line number Diff line change
@@ -14,7 +14,7 @@
@rescaleFactor = 0.48
@title = Gas Chromatograph-Mass Spectrometer (GC/MS)
@manufacturer = Generic
@description = The Gas Chromatograph-Mass Spectrometer (GC-MS) is an analytical instrument used for identification of multiple different substances in a selected gas sample, capable of detecting even trace amounts of them. Ideal of analyzing the atmospheric composition of unknown environments. Mass spectrometry is an analytical technique that ionizes chemical species and sorts the ions based on their mass-to-charge ratio. Historically, these simple experiments were flown on interplanetary crafts including the Mars Viking Lander and Cassini.\nLevel 4 Mass Spectrometry Experiment. Can gather 100% of Mass Spectrometry Science.
@description = The Gas Chromatograph-Mass Spectrometer (GC-MS) is an analytical instrument used for identification of multiple different substances in a selected gas sample, capable of detecting even trace amounts of them. Ideal of analyzing the atmospheric composition of unknown environments. Mass spectrometry is an analytical technique that ionizes chemical species and sorts the ions based on their mass-to-charge ratio. Historically, these simple experiments were flown on interplanetary crafts including the Mars Viking Lander and Cassini.\n\nLevel 4 Mass Spectrometry Experiment. Can gather 100% of Mass Spectrometry Science.
@mass = 0.019
@maxTemp = 1073.15
@tags = science gc-ms gas chromatograph mass spectrometer viking cassini
2 changes: 1 addition & 1 deletion GameData/RP-0/Parts/Science/PHOTO01-EarlyFilmCamera.cfg
Original file line number Diff line number Diff line change
@@ -11,7 +11,7 @@

@title = Early Film Camera
@manufacturer = Generic
@description = The Early Film Camera is used to take photographs of Earth from space. This is a very early camera and lacks resolution in the images. Historically, these were flown on V-2 Rockets.\nThe photos cannot be transmitted and must be returned for further study. Level 1 Photograph Experiment. Can gather 20% of Photography Science.
@description = The Early Film Camera is used to take photographs of Earth from space. This is a very early camera and lacks resolution in the images. Historically, these were flown on V-2 Rockets.\nThe photos cannot be transmitted and must be returned for further study.\n\nLevel 1 Photograph Experiment. Can gather 20% of Photography Science.
@mass = 0.1
@tags = science photo photographs film camera

2 changes: 1 addition & 1 deletion GameData/RP-0/Parts/Science/PHOTO02-ImprovedFilmCamera.cfg
Original file line number Diff line number Diff line change
@@ -13,7 +13,7 @@
%RSSROConfig = True

@title = Improved Film Camera
@description = The Improved Film Camera is used to take photographs of Earth from space. This is a vast improvement over the very basic Early Camera. Historically, these were flown as Spy Satellites under the Corona name.\nThe photos can be transmitted, but at a severe penalty of only 25% data. Level 2 Photograph Experiment. Can gather 50% of Photography Science.
@description = The Improved Film Camera is used to take photographs of Earth from space. This is a vast improvement over the very basic Early Camera. Historically, these were flown as Spy Satellites under the Corona name.\n\nThe photos can be transmitted, but at a severe penalty of only 25% data. Level 2 Photograph Experiment. Can gather 50% of Photography Science.
@mass = 0.6
@tags = science photo photographs film camera corona spy sats dmagic
@maxTemp = 1073.15
2 changes: 1 addition & 1 deletion GameData/RP-0/Parts/Science/PHOTO03-HighResFilmCamera.cfg
Original file line number Diff line number Diff line change
@@ -15,7 +15,7 @@
%rescaleFactor = 1.2

@title = High Resolution Film Camera
@description = The High Resolution Film Camera is used to take photographs of Earth from space. This camera provides very high resolution photographs of Earth. They can be transmitted back to Earth, but some fidelity is lost. It is still recommended to physically return them. Historically, these were flown as Spy Satellites under the KH-9 Hexagon name.\nThe photos can be transmitted, but at a penalty of only 50% data. Level 3 Photograph Experiment. Can gather 100% of Photography Science.
@description = The High Resolution Film Camera is used to take photographs of Earth from space. This camera provides very high resolution photographs of Earth. They can be transmitted back to Earth, but some fidelity is lost. It is still recommended to physically return them. Historically, these were flown as Spy Satellites under the KH-9 Hexagon name.\n\nThe photos can be transmitted, but at a penalty of only 50% data. Level 3 Photograph Experiment. Can gather 100% of Photography Science.
@mass = 5.0
@tags = science photo photographs film camera keyhole spy sats dmagic hexagon kh-9
@maxTemp = 1073.15
2 changes: 1 addition & 1 deletion GameData/RP-0/Parts/Science/PHOTO04-DigitalCamera.cfg
Original file line number Diff line number Diff line change
@@ -20,7 +20,7 @@
%rescaleFactor = 1.0

@title = Ultra Resolution Digital Imaging Camera
@description = The Ultra Resolution Digital Imaging Camera is used to take photographs of Earth from space. This camera stores all of the imaging data digitally and can be transmitted fully back to Earth. Historically, these were flown as Spy Satellites under the KH-11 Kennen name.\nLevel 4 Photograph Experiment. Can gather 100% of Photography Science. You can store up to 10 different photos before you need to transmit them to Earth.
@description = The Ultra Resolution Digital Imaging Camera is used to take photographs of Earth from space. This camera stores all of the imaging data digitally and can be transmitted fully back to Earth. Historically, these were flown as Spy Satellites under the KH-11 Kennen name.\n\nLevel 4 Photograph Experiment. Can gather 100% of Photography Science.
@mass = 6.0
@tags = science photo photographs film camera keyhole spy sats dmagic kennen kh-11 hubble
@maxTemp = 1073.15
17 changes: 1 addition & 16 deletions GameData/RP-0/Parts/Science/RPWS01-PlasmaWave.cfg
Original file line number Diff line number Diff line change
@@ -36,7 +36,7 @@ PART
subcategory = 0
title = Plasma Wave Detector
manufacturer = Coatl Aerospace
description = The Plasma Wave Detector measures the electrostatic and electromagnetic plasma waves from the solar wind. Historically, this experiment is based on the one flown on Pioneer 5,6,7,8 that studied the interplanetary space between Earth and Venus.\nThe science can be transmitted for full recovery. Level 1 Radio-Plasma Wave Experiment can gather 25% of Radio and Plasma Wave Science.
description = The Plasma Wave Detector measures the electrostatic and electromagnetic plasma waves from the solar wind. Historically, this experiment is based on the one flown on Pioneer 5,6,7,8 that studied the interplanetary space between Earth and Venus.\n\nThe science can be transmitted for full recovery. Level 1 Radio-Plasma Wave Experiment can gather 25% of Radio and Plasma Wave Science.

mass = 0.005
dragModelType = default
@@ -50,19 +50,4 @@ PART

tags = coatl science plasma wave detector pioneer

MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-RPWS1
experimentActionName = RPWS Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
}
35 changes: 2 additions & 33 deletions GameData/RP-0/Parts/Science/RPWS02-SWPlasmaWave.cfg
Original file line number Diff line number Diff line change
@@ -36,7 +36,7 @@ PART
subcategory = 0
title = Solar Wind Plasma Analyzer
manufacturer = Coatl Aerospace
description = The Solar Wind Plasma Analyzer measures the electrostatic plasma waves from the solar wind. Historically, this experiment is based on the one flown on Helios-A and B and many other craft.\nThe science can be transmitted for full recovery. Level 2 Radio-Plasma Wave Experiment can gather 50% of Radio and Plasma Wave Science.
description = The Solar Wind Plasma Analyzer measures the electrostatic plasma waves from the solar wind. Historically, this experiment is based on the one flown on Helios-A and B and many other craft.\n\nThe science can be transmitted for full recovery. Level 2 Radio-Plasma Wave Experiment can gather 50% of Radio and Plasma Wave Science.

mass = 0.005
bulkheadProfiles = srf
@@ -53,36 +53,5 @@ PART

tags = coatl ca solar wind swis experiment research science plasma

MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-RPWS1
experimentActionName = RPWS Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-RPWS2
experimentActionName = RPWS Level 2
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}



}
2 changes: 1 addition & 1 deletion GameData/RP-0/Parts/Science/RPWS03-RPWS.cfg
Original file line number Diff line number Diff line change
@@ -19,7 +19,7 @@
}

@title = Radio and Plasma Wave Science (RPWS)
@description = The Radio and Plasma Wave Science instrument measures electrostatic and electromagnetic fields generated by the interaction of planetary magnetospheres and the interplanetary plasma medium. Historically, this experiment is based on the one flown on Cassini.\nThe science can be transmitted for full recovery. Level 3 Radio-Plasma Wave Experiment can gather 100% of Radio and Plasma Wave Science.
@description = The Radio and Plasma Wave Science instrument measures electrostatic and electromagnetic fields generated by the interaction of planetary magnetospheres and the interplanetary plasma medium. Historically, this experiment is based on the one flown on Cassini.\n\nThe science can be transmitted for full recovery. Level 3 Radio-Plasma Wave Experiment can gather 100% of Radio and Plasma Wave Science.
@mass = 0.0068
@tags = science dmagic rpws radio plasma wave cassini
@maxTemp = 1073.15
18 changes: 1 addition & 17 deletions GameData/RP-0/Parts/Science/SS01-SurfaceSampler.cfg
Original file line number Diff line number Diff line change
@@ -34,7 +34,7 @@ PART
subcategory = 0
title = Soil Mechanics Surface Sampler
manufacturer = Coatl Aerospace
description = The soil mechanics surface sampler is an instrument designed to test the physical properties of the topsoil (density, porosity, resistivity) and to expose subsoil material for photography. Historically, this experiment is based on the one flown on the Surveyor missions.\nThe science can be transmitted for 25% recovery, but can be returned for full value.
description = The soil mechanics surface sampler is an instrument designed to test the physical properties of the topsoil (density, porosity, resistivity) and to expose subsoil material for photography. Historically, this experiment is based on the one flown on the Surveyor missions.\n\nThe science can be transmitted for 25% recovery, but can be returned for full value.

mass = 0.005
bulkheadProfiles = srf
@@ -60,20 +60,4 @@ PART
actionGUIName = Toggle Soil Scoop
evaDistance = 1.85
}

MODULE
{
name = ModuleScienceExperiment
experimentID = surfaceSample
experimentActionName = Scoop Surface Material
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 0.25
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
}
19 changes: 1 addition & 18 deletions GameData/RP-0/Parts/Science/VI01-EarlyTVCamera.cfg
Original file line number Diff line number Diff line change
@@ -31,7 +31,7 @@ MODEL
subcategory = 0
title = Early Television Camera
manufacturer = Bluedog Design Bureau
description = The Early Television Camera is used to take images in the visibile wavelength of planetary bodies from space. This is a very early camera and lacks resolution in the images. Historically, these were flown on Explorer 6, which was the first craft to send images of Earth from orbit, and Luna 3 which was the first craft to return images from the far side of the Moon.\nThe images can be transmitted for full science value. Level 1 Visible Imaging Experiment can gather 10% of Visible Imaging Science. You can keep up to 5 different images in the storage available.
description = The Early Television Camera is used to take images in the visibile wavelength of planetary bodies from space. This is a very early camera and lacks resolution in the images. Historically, these were flown on Explorer 6, which was the first craft to send images of Earth from orbit, and Luna 3 which was the first craft to return images from the far side of the Moon.\n\nThe images can be transmitted for full science value. Level 1 Visible Imaging Experiment can gather 10% of Visible Imaging Science.
attachRules = 0,1,0,0,1
mass = 0.005
dragModelType = default
@@ -53,21 +53,4 @@ MODEL
actionGUIName = Toggle Aperature
evaDistance = 1.85
}

MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-visibleImaging1
experimentActionName = Visible Imaging Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}

}
33 changes: 1 addition & 32 deletions GameData/RP-0/Parts/Science/VI02-BasicTVCamera.cfg
Original file line number Diff line number Diff line change
@@ -39,7 +39,7 @@ PART
subcategory = 0
title = Basic TV Camera
manufacturer = Coatl Aerospace
description = The Basic TV Camera is used to take images in the visibile wavelength of planetary bodies from space. This is an early camera and lacks resolution in the images. Historically, this type of camera was flown on Mariner 4 and took the first images of another planet.\nThe images can be transmitted for full science value. Level 2 Visible Imaging Experiment can gather 25% of Visible Imaging Science. You can keep up to 5 different images in the storage available.
description = The Basic TV Camera is used to take images in the visibile wavelength of planetary bodies from space. This is an early camera and lacks resolution in the images. Historically, this type of camera was flown on Mariner 4 and took the first images of another planet.\n\nThe images can be transmitted for full science value. Level 2 Visible Imaging Experiment can gather 25% of Visible Imaging Science.

mass = 0.00512
bulkheadProfiles = size0, srf
@@ -56,36 +56,5 @@ PART

tags = coatl tv television science camera visible imaging mariner mars

MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-visibleImaging1
experimentActionName = Visible Imaging Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-visibleImaging2
experimentActionName = Visible Imaging Level 2
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}


}
50 changes: 2 additions & 48 deletions GameData/RP-0/Parts/Science/VI03-ImprovedTVCamera.cfg
Original file line number Diff line number Diff line change
@@ -37,7 +37,7 @@ PART
subcategory = 0
title = Improved TV Camera
manufacturer = Coatl Aerospace East
description = The Improved TV Camera is used to take images in the visibile wavelength of planetary bodies from space. Historically, this type of camera was flown on Mariner 10 and took the first images of Mercury.\nThe images can be transmitted for full science value. Level 3 Visible Imaging Experiment can gather 50% of Visible Imaging Science. You can keep up to 5 different images in the storage available.
description = The Improved TV Camera is used to take images in the visibile wavelength of planetary bodies from space. Historically, this type of camera was flown on Mariner 10 and took the first images of Mercury.\n\nThe images can be transmitted for full science value. Level 3 Visible Imaging Experiment can gather 50% of Visible Imaging Science.

mass = 0.04
bulkheadProfiles = srf
@@ -81,53 +81,7 @@ PART
evaDistance = 1.85
}

MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-visibleImaging1
experimentActionName = Visible Imaging Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-visibleImaging2
experimentActionName = Visible Imaging Level 2
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-visibleImaging3
experimentActionName = Visible Imaging Level 3
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}



}


64 changes: 1 addition & 63 deletions GameData/RP-0/Parts/Science/VI04-AdvancedImager.cfg
Original file line number Diff line number Diff line change
@@ -38,7 +38,7 @@ PART
subcategory = 0
title = Advanced Visible Imaging Device
manufacturer = Coatl Aerospace
description = The Advanced Visible Imaging Device is used to take images in the visibile wavelength of planetary bodies from space. Historically, this type of camera was flown on Galileo and took images of Jupiter and it's moons.\nThe images can be transmitted for full science value. Level 4 Visible Imaging Experiment can gather 75% of Visible Imaging Science. You can keep up to 5 different images in the storage available.
description = The Advanced Visible Imaging Device is used to take images in the visibile wavelength of planetary bodies from space. Historically, this type of camera was flown on Galileo and took images of Jupiter and it's moons.\n\nThe images can be transmitted for full science value. Level 4 Visible Imaging Experiment can gather 75% of Visible Imaging Science.
mass = 0.028
bulkheadProfiles = size0, srf
@@ -55,66 +55,4 @@ PART
tags = coatl tv television science camera visible imaging galileo jupiter
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-visibleImaging1
experimentActionName = Visible Imaging Level 1
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-visibleImaging2
experimentActionName = Visible Imaging Level 2
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-visibleImaging3
experimentActionName = Visible Imaging Level 3
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-visibleImaging4
experimentActionName = Visible Imaging Level 4
resetActionName = Discard Data
reviewActionName = Review Stored Data
useStaging = False
useActionGroups = True
hideUIwhenUnavailable = True
rerunnable = True
xmitDataScalar = 1
usageReqMaskInternal = 1
usageReqMaskExternal = 4
}
}
3 changes: 2 additions & 1 deletion GameData/RP-0/Parts/Science/VI05-HIResImager.cfg
Original file line number Diff line number Diff line change
@@ -11,11 +11,12 @@
+PART[dmscope]:FOR[RP-0]
{
%name = RO-HIRES
%RSSROConfig = True
%RSSROConfig = True
%rescaleFactor = 1.8

@title = High Resolution Imaging Device
@description = The High Resolution Imaging Device is used to take images in the visibile wavelength of planetary bodies from space. This imager takes very high resolution images and can show details previously undsicovered on other planetary bodies. Historically, this type of camera was flown on the Mars Reconaissance Orbiter.\nThe images can be transmitted for full science value. Level 5 Visible Imaging Experiment can gather 100% of Visible Imaging Science. You can keep up to 5 different images in the storage available.
@description = The High Resolution Imaging Device is used to take images in the visibile wavelength of planetary bodies from space. This imager takes very high resolution images and can show details previously undsicovered on other planetary bodies. Historically, this type of camera was flown on the Mars Reconaissance Orbiter.\n\nThe images can be transmitted for full science value. Level 5 Visible Imaging Experiment can gather 100% of Visible Imaging Science.
@mass = 0.065
@tags = science dmagic hirise mro imaging visible mars
@maxTemp = 1073.15
44 changes: 22 additions & 22 deletions GameData/RP-0/Science/CleanupParts/PartExperimentAdder.cfg
Original file line number Diff line number Diff line change
@@ -133,7 +133,7 @@
//**********************************************************************************

// Level 1 (Geiger-Muller Counter) 100%
@PART[RP0probeVanguardXray|sputnik2|pioneer_0_1_2|bluedog_Pioneer1|pioneer_3_4|bluedog_Pioneer4|sputnik3|explorer_6|bluedog_explorer7probe|luna2|vanguard-3|pioneer_5|rn_mariner1_2|pioneer_6_7_8_9|quetzal|pioneer_10_11|rn_voyager|torekka|galileo_aprobe|galileo_mb|bluedog_Explorer1|FASAExplorerProbe|luna_als|luna11_als|neo_dawn|rn_lro|rn_juno_spacecraft]:FOR[RP-0]
@PART[RP0probeVanguardXray|sputnik2|pioneer_0_1_2|bluedog_Pioneer1|pioneer_3_4|bluedog_Pioneer4|sputnik3|explorer_6|bluedog_explorer7probe|luna2|vanguard-3|pioneer_5|rn_mariner1_2|pioneer_6_7_8_9|quetzal|pioneer_10_11|rn_voyager|torekka|galileo_aprobe|galileo_mb|bluedog_Explorer1|FASAExplorerProbe|luna_als|luna11_als|neo_dawn|rn_lro|rn_juno_spacecraft|RO-GeigerMuller]:FOR[RP-0]
{
MODULE
{
@@ -175,7 +175,7 @@
//**********************************************************************************

// Level 1 (IRIS) 25%
@PART[luna_als|rn_voyager|torekka|galileo_mb|rn_cassini|neo_dawn|neo_deepimpact|neo_ds1|rn_juno_spacecraft|rn_ladee|rn_messenger|neo_near|rn_new_horizons|eos_terra]:FOR[RP-0]
@PART[RO-IRIS|luna_als|rn_voyager|torekka|galileo_mb|rn_cassini|neo_dawn|neo_deepimpact|neo_ds1|rn_juno_spacecraft|rn_ladee|rn_messenger|neo_near|rn_new_horizons|eos_terra|RO-UVSpectrometer|RO-NIMS]:FOR[RP-0]
{
MODULE
{
@@ -196,7 +196,7 @@
}

// Level 2 (Ultraviolet Spectrometer) 50%
@PART[luna_als|rn_voyager|torekka|galileo_mb|rn_cassini|neo_dawn|neo_deepimpact|neo_ds1|rn_juno_spacecraft|rn_ladee|rn_messenger|neo_near|rn_new_horizons|eos_terra]:FOR[RP-0]
@PART[luna_als|rn_voyager|torekka|galileo_mb|rn_cassini|neo_dawn|neo_deepimpact|neo_ds1|rn_juno_spacecraft|rn_ladee|rn_messenger|neo_near|rn_new_horizons|eos_terra|RO-UVSpectrometer|RO-NIMS]:FOR[RP-0]
{
MODULE
{
@@ -217,7 +217,7 @@
}

// Level 3 (NIMS) 75%
@PART[galileo_mb|rn_cassini|neo_dawn|neo_deepimpact|neo_ds1|rn_juno_spacecraft|rn_ladee|rn_messenger|neo_near|rn_new_horizons|eos_terra]:FOR[RP-0]
@PART[galileo_mb|rn_cassini|neo_dawn|neo_deepimpact|neo_ds1|rn_juno_spacecraft|rn_ladee|rn_messenger|neo_near|rn_new_horizons|eos_terra|RO-NIMS]:FOR[RP-0]
{
MODULE
{
@@ -262,7 +262,7 @@
//**********************************************************************************

// Level 1 (Infrared Radiometer) 25%
@PART[luna_als|quetzal|pioneer_10_11|rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|rn_new_horizons|eos_terra|galileo_aprobe|rn_huygens|rn_lro]:FOR[RP-0]
@PART[luna_als|quetzal|pioneer_10_11|rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|rn_new_horizons|eos_terra|galileo_aprobe|rn_huygens|rn_lro|RO-IRRadiometer|RO-HRIRRadiometer|RO-TwoChannelIR]:FOR[RP-0]
{
MODULE
{
@@ -283,7 +283,7 @@
}

// Level 2 (High-Resolution Infrared Radiometer) 50%
@PART[luna_als|quetzal|pioneer_10_11|rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|rn_new_horizons|eos_terra|galileo_aprobe|rn_huygens|rn_lro]:FOR[RP-0]
@PART[luna_als|quetzal|pioneer_10_11|rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|rn_new_horizons|eos_terra|galileo_aprobe|rn_huygens|rn_lro|RO-HRIRRadiometer|RO-TwoChannelIR]:FOR[RP-0]
{
MODULE
{
@@ -304,7 +304,7 @@
}

// Level 3 (Two-Channel Infrared Radiometer) 75%
@PART[rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|rn_new_horizons|eos_terra|galileo_aprobe|rn_huygens|rn_lro]:FOR[RP-0]
@PART[rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|rn_new_horizons|eos_terra|galileo_aprobe|rn_huygens|rn_lro|RO-TwoChannelIR]:FOR[RP-0]
{
MODULE
{
@@ -350,7 +350,7 @@
//**********************************************************************************

// Level 1 (Early Magnetometer) 30%
@PART[explorer_6|luna2|pioneer_0_1_2|bluedog_Pioneer1|pioneer_5|sputnik3|vanguard-3|rn_mariner1_2|luna_als|quetzal|pioneer_10_11|rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|neo_near|pioneer_6_7_8_9|neo_ulysses]:FOR[RP-0]
@PART[explorer_6|luna2|pioneer_0_1_2|bluedog_Pioneer1|pioneer_5|sputnik3|vanguard-3|rn_mariner1_2|luna_als|quetzal|pioneer_10_11|rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|neo_near|pioneer_6_7_8_9|neo_ulysses|RO-EarlyMagnet|RO-HeliumMagnet]:FOR[RP-0]
{
MODULE
{
@@ -371,7 +371,7 @@
}

// Level 2 (Helium Magnetometer) 60%
@PART[rn_mariner1_2|luna_als|quetzal|pioneer_10_11|rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|neo_near|pioneer_6_7_8_9|neo_ulysses]:FOR[RP-0]
@PART[rn_mariner1_2|luna_als|quetzal|pioneer_10_11|rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|neo_near|pioneer_6_7_8_9|neo_ulysses|RO-HeliumMagnet]:FOR[RP-0]
{
MODULE
{
@@ -423,7 +423,7 @@
//**********************************************************************************

// Level 1 (Ion Mass Spectrometer) 25%
@PART[explorer_6|pioneer_0_1_2|bluedog_Pioneer1|pioneer_5|sputnik3|RP0probeVanguardXray|luna_als|luna11_als|quetzal|pioneer_10_11|rn_voyager|torekka|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|neo_ulysses|rn_new_horizons|galileo_aprobe|rn_huygens|neo_ds1|rn_ladee]:FOR[RP-0]
@PART[explorer_6|pioneer_0_1_2|bluedog_Pioneer1|pioneer_5|sputnik3|RP0probeVanguardXray|luna_als|luna11_als|quetzal|pioneer_10_11|rn_voyager|torekka|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|neo_ulysses|rn_new_horizons|galileo_aprobe|rn_huygens|neo_ds1|rn_ladee|RO-MIMS|RO-QuadropoleMassSpectrometer|SXTsciencenosecone]:FOR[RP-0]
{
MODULE
{
@@ -444,7 +444,7 @@
}

// Level 2 (MIMS) 50%
@PART[luna_als|luna11_als|quetzal|pioneer_10_11|rn_voyager|torekka|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|neo_ulysses|rn_new_horizons|galileo_aprobe|rn_huygens|neo_ds1|rn_ladee]:FOR[RP-0]
@PART[luna_als|luna11_als|quetzal|pioneer_10_11|rn_voyager|torekka|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|neo_ulysses|rn_new_horizons|galileo_aprobe|rn_huygens|neo_ds1|rn_ladee|RO-MIMS|RO-QuadropoleMassSpectrometer|SXTsciencenosecone]:FOR[RP-0]
{
MODULE
{
@@ -465,7 +465,7 @@
}

// Level 3 (Quadropole Mass Spectrometer) 75%
@PART[quetzal|pioneer_10_11|rn_voyager|torekka|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|neo_ulysses|rn_new_horizons|galileo_aprobe|rn_huygens|neo_ds1|rn_ladee]:FOR[RP-0]
@PART[quetzal|pioneer_10_11|rn_voyager|torekka|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|neo_ulysses|rn_new_horizons|galileo_aprobe|rn_huygens|neo_ds1|rn_ladee|RO-QuadropoleMassSpectrometer|SXTsciencenosecone]:FOR[RP-0]
{
MODULE
{
@@ -486,7 +486,7 @@
}

// Level 4 (GC-MS) 100%
@PART[rn_voyager|torekka|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|neo_ulysses|rn_new_horizons|galileo_aprobe|rn_huygens|neo_ds1|rn_ladee]:FOR[RP-0]
@PART[rn_voyager|torekka|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|neo_ulysses|rn_new_horizons|galileo_aprobe|rn_huygens|neo_ds1|rn_ladee|SXTsciencenosecone]:FOR[RP-0]
{
MODULE
{
@@ -511,7 +511,7 @@
//**********************************************************************************

// Level 1 (Micrometeorite Detector) 100%
@PART[explorer_6|pioneer_0_1_2|bluedog_Pioneer1|pioneer_5|sputnik3|luna_als|luna11_als|quetzal|pioneer_10_11|vanguard-3|bluedog_Explorer1|FASAExplorerProbe|RP0probeVanguardXray]:FOR[RP-0]
@PART[explorer_6|pioneer_0_1_2|bluedog_Pioneer1|pioneer_5|sputnik3|luna_als|luna11_als|quetzal|pioneer_10_11|vanguard-3|bluedog_Explorer1|FASAExplorerProbe|RP0probeVanguardXray|RO-Micrometeorite]:FOR[RP-0]
{
MODULE
{
@@ -632,7 +632,7 @@
//**********************************************************************************

// Level 1 (Plasma Wave Detector) 30%
@PART[luna_als|quetzal|pioneer_10_11|rn_mariner1_2|neo_ulysses|rn_voyager|torekka|galileo_mb|pioneer_6_7_8_9|neo_near|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|rn_new_horizons|rn_lro|neo_deepimpact]:FOR[RP-0]
@PART[luna_als|quetzal|pioneer_10_11|rn_mariner1_2|neo_ulysses|rn_voyager|torekka|galileo_mb|pioneer_6_7_8_9|neo_near|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|rn_new_horizons|rn_lro|neo_deepimpact|RO-PlasmaWave|RO-SWPlasmaAnalyzer]:FOR[RP-0]
{
MODULE
{
@@ -653,7 +653,7 @@
}

// Level 2 (Solar Wind Plasma Analyzer) 60%
@PART[neo_ulysses|rn_voyager|torekka|galileo_mb|pioneer_6_7_8_9|neo_near|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|rn_new_horizons|rn_lro|neo_deepimpact]:FOR[RP-0]
@PART[neo_ulysses|rn_voyager|torekka|galileo_mb|pioneer_6_7_8_9|neo_near|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|rn_new_horizons|rn_lro|neo_deepimpact|RO-SWPlasmaAnalyzer]:FOR[RP-0]
{
MODULE
{
@@ -705,7 +705,7 @@
//**********************************************************************************

// Level 1 (Soil Mechanics Surface Sampler) 100%
@PART[rn_surveyor3]:FOR[RP-0]
@PART[rn_surveyor3|RO-SurfaceSampleScoop]:FOR[RP-0]
{
MODULE
{
@@ -734,7 +734,7 @@
MODULE
{
name = ModuleScienceExperiment
experimentID = RP0-temperature1
experimentID = temperatureScan
experimentActionName = Log Temperature
resetActionName = Discard Data
reviewActionName = Review Stored Data
@@ -753,7 +753,7 @@
//**********************************************************************************

// Level 1 (Early TV Camera) 10%
@PART[vanguard-2|explorer_6|pioneer_0_1_2|bluedog_Pioneer1|luna3|tiros-1|rn_surveyor3|luna13_als|quetzal|pioneer_10_11|rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|rn_new_horizons|rn_lro|neo_deepimpact]:FOR[RP-0]
@PART[vanguard-2|explorer_6|pioneer_0_1_2|bluedog_Pioneer1|luna3|tiros-1|rn_surveyor3|luna13_als|quetzal|pioneer_10_11|rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|rn_new_horizons|rn_lro|neo_deepimpact|RO-EarlyTVCamera|RO-BasicTVCamera|RO-ImprovedTVCamera|RO-AdvancedImager]:FOR[RP-0]
{
MODULE
{
@@ -774,7 +774,7 @@
}

// Level 2 (Basic TV Camera) 25%
@PART[rn_surveyor3|luna13_als|quetzal|pioneer_10_11|rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|rn_new_horizons|rn_lro|neo_deepimpact]:FOR[RP-0]
@PART[rn_surveyor3|luna13_als|quetzal|pioneer_10_11|rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|rn_new_horizons|rn_lro|neo_deepimpact|RO-BasicTVCamera|RO-ImprovedTVCamera|RO-AdvancedImager]:FOR[RP-0]
{
MODULE
{
@@ -795,7 +795,7 @@
}

// Level 3 (Improved TV Camera) 50%
@PART[quetzal|pioneer_10_11|rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|rn_new_horizons|rn_lro|neo_deepimpact]:FOR[RP-0]
@PART[quetzal|pioneer_10_11|rn_voyager|torekka|galileo_mb|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|rn_new_horizons|rn_lro|neo_deepimpact|RO-ImprovedTVCamera|RO-AdvancedImager]:FOR[RP-0]
{
MODULE
{
@@ -816,7 +816,7 @@
}

// Level 4 (Advanced Visible Imaging Device) 75%
@PART[galileo_mb|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|rn_new_horizons|rn_lro|neo_deepimpact]:FOR[RP-0]
@PART[galileo_mb|rn_cassini|rn_juno_spacecraft|neo_dawn|rn_messenger|rn_new_horizons|rn_lro|neo_deepimpact|RO-AdvancedImager]:FOR[RP-0]
{
MODULE
{
37 changes: 0 additions & 37 deletions GameData/RP-0/Science/CleanupParts/StockSXTVensScienceParts.cfg
Original file line number Diff line number Diff line change
@@ -11,41 +11,4 @@
@title = Barometer
}

//**********************************************************************************
// Fix SXT GC-MS + Antenna
//**********************************************************************************
@PART[SXTsciencenosecone]:FOR[RP-0]
{
!MODULE[ModuleScienceExperiment] {}

MODULE
{
name = DMModuleScienceAnimateGeneric
experimentAnimation = false // No animation
collectActionName = Collect Data // EVA collection message
dataIsCollectable = true // EVA can be collected
experimentActionName = Run Mass Spectrum Analysis // Right Click Action
experimentID = atmosphereAnalysis // Experiment name
hideUIwhenUnavailable = false // Hide right-click collection
interactionRange = 1.2 // EVA Range
rerunnable = true // Can be used multiple times
resettable = true // Does nothing???
resettableOnEVA = true // EVA can Reset Experiment
resourceResetCost = 1 // Cost to reset
resourceToReset = ElectricCharge // Can't change????
resetActionName = Reset Experiment // Right click Action
reviewActionName = Review Data // Right click Review
useActionGroups = True // Allow Action Groups
useStaging = False // Always set False
xmitDataScalar = 1.0 // Transmission Data Value %
usageReqMaskInternal = 1
usageReqMaskExternal = -1 // Bit Mask to define external usage conditions; 8 specifies that the EVA kerbal must be a scientist to deploy the experiment; 4 will allow any Kerbal to deploy from EVA; -1 means nothing can use the experiment externally
totalScienceLevel = 1.0 // Science % of experimentID
resourceExpCost = 0 // Cost per second while collecting
asteroidReports = True // Allow results near Asteroids
storageFullMessage = No more samples can be analyzed right now
experimentsLimit = 4 // # of experiments that can be stored
externalDeploy = True // EVA can activate
}
}

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