RoadWarrior9

December 4, 2021

That should work. I put it in an existing game and it changed to the rate based version with no issues. If you have a harvest pending you may need to complete the harvest to get the rate part working. Also you may need to change the section ":AFTER[KerbalismDefault]" to ":FINAL" depending on what order your patch runs. This should run after kerbalism. I would suggest putting personal patches in a folder called "zz..." so it loads after all of the other patches. I think module manager loads by folder name if everything else is the same.

December 3, 2021

6 minutes ago, adriangm44 said:

The idea is quite good! Why not the smallest one?

Because it is too small to feed anyone and would only be useful as a science experiment.

December 2, 2021

I'm new to these forums and all posts have to be approved by a moderator which is really annoying. Hopefully this is the 5th post and they will free me...

How do you attach a file to a post? Don't see any way to put a csv file here. You have to be careful when changing config settings used by the lab. I have done it in my playthrough and it worked for me but have seen posts where the labs already deployed have been borked and had to be relaunched.

December 2, 2021

30 minutes ago, adriangm44 said:

You are right, the cofigs are outdated due to the new SSPX update.

I just posted a config that converts all kerbalism greenhouses to a rate based food per second instead of harvest based method. It includes all SSPX greenhouse type modules except for the smallest one. See post. To add the SSPX greenhouse modules using the default kerbalism greenhouse just edit the file SSPX.cfg under support in the Kerbalism support section, find greenhouse, copy paste and change the part name.

December 2, 2021

I came up with a workaround (config) that should allow the default greenhouse that comes with kerbalism to use a rate based food per second output instead of having to go to the ship and harvest the food when the harvest is ready every 200 days. This sets the harvest time to >1000 years and adds a resource output of food (along with oxygen) that should match the old output. There are also configs that modify and add the greenhouse functionality to the Stockalike Station Parts Redux greenhouse parts. Create a folder like zMyMods and create a *.cfg file and copy the sections you want to it.

//Kerbalism greenhouse patchs

@PART[kerbalism-greenhouse]:NEEDS[ProfileDefault]:AFTER[KerbalismDefault]  // Default Kerbalism greenhouse
{
  @MODULE[Greenhouse]
  {
    @crop_rate = 0.00000000005
	
	OUTPUT_RESOURCE
	{
		name = Food
		rate = 0.000003190104
	}
  }
}

@PART[sspx-greenhouse-25-1]:NEEDS[StationPartsExpansionRedux,ProfileDefault]:AFTER[KerbalismDefault]  // PPD-F412M Hydroponics Module
{
	@MODULE[Greenhouse]
	{
		@crop_rate = 0.00000000005

		OUTPUT_RESOURCE
		{
			name = Food
			rate = 0.000006380208
		}
	}
	
	MODULE
	{
		name = Comfort
		bonus = plants
		desc =  There's something inherently calming about an artificial slice of nature, kept alive only by the miracles of duct-tape and kerbal engineering. Let's hope the crew doesn't think too much about it.
	}
}

@PART[sspx-greenhouse-375-1]:NEEDS[StationPartsExpansionRedux,ProfileDefault]:AFTER[KerbalismDefault]  // PXL-R4NCH-3R Hydroponics Module
{
	@MODULE[Greenhouse]
	{
		@crop_rate = 0.00000000005

		OUTPUT_RESOURCE
		{
			name = Food
			rate = 0.000006380208
		}
	}
	
	MODULE
	{
		name = Comfort
		bonus = plants
		desc =  There's something inherently calming about an artificial slice of nature, kept alive only by the miracles of duct-tape and kerbal engineering. Let's hope the crew doesn't think too much about it.
	}
}

@PART[sspx-greenhouse-5-1]:NEEDS[StationPartsExpansionRedux,ProfileDefault]:AFTER[KerbalismDefault]  // SDV-4 'Demeter' Cultivation Module
{
	!MODULE[Greenhouse] {}
	MODULE
	{
		name = Greenhouse

		crop_resource = Food
		crop_size = 110.0
		crop_rate = 0.00000000005
		ec_rate = 10
		light_tolerance = 400.0
		pressure_tolerance = 0.1
		radiation_tolerance = 0.000008333

		INPUT_RESOURCE
		{
			name = Ammonia
			rate = 0.0003828125
		}

		INPUT_RESOURCE
		{
			name = Water
			rate = 0.0000127604
		}

		INPUT_RESOURCE
		{
			name = WasteAtmosphere
			rate = 0.004983199
		}

		INPUT_RESOURCE
		{
			name = CarbonDioxide
			rate = 0.0016610663
		}

		OUTPUT_RESOURCE
		{
			name = Oxygen
			rate = 0.006895193
		}

		OUTPUT_RESOURCE
		{
			name = Food
			rate = 0.000012760416
		}
	}

	MODULE
	{
		name = Comfort
		bonus = plants
		desc =  There's something inherently calming about an artificial slice of nature, kept alive only by the miracles of duct-tape and kerbal engineering. Let's hope the crew doesn't think too much about it.
	}

	RESOURCE
	{
		name = Ammonia
		amount = 1000
		maxAmount = 1000
	}

	RESOURCE
	{
		name = CarbonDioxide
		amount = 18000
		maxAmount = 18000
	}

	// To support pressure control
	@MODULE[Configure]
	{
		@SETUP[Pressure?Control]
		{
		!RESOURCE[Nitrogen] {}
		}
	}

	RESOURCE
	{
		name = Nitrogen
		amount = 20000
		maxAmount = 20000
	}

	RESOURCE
	{
		name = Water
		amount = 50	
		maxAmount = 50
	}
}

@PART[sspx-dome-greenhouse-5-1]:NEEDS[StationPartsExpansionRedux,ProfileDefault]:AFTER[KerbalismDefault]  // SDV-G2 'Villa' Cultivation Dome
{
	!MODULE[Greenhouse] {}
	MODULE
	{
		name = Greenhouse

		crop_resource = Food								// name of resource produced by harvests
		// Twice as effective as kerbalism-greenhouse part. 
		// See https://forum.kerbalspaceprogram.com/index.php?/topic/172400-131145-kerbalism-v180/&page=32&tab=comments#comment-3446891 for details.

		// Both growing "rings" of this greenhouse are unfortunately in the same section. No independent growing possible. (Different watering and lighting needs for different grow stages). 
		crop_size = 80.0									// 2x kerbalism-greenhouse
		crop_rate = 0.00000000005					 // regular growth speed
		ec_rate = 7												 // 2x"kerbalism-greenhouse"
		light_tolerance = 400.0						 // minimum lighting flux required for growth, in W/m^2
		pressure_tolerance = 0.1						// minimum pressure required for growth, in sea level atmospheres
		radiation_tolerance = 0.000008333	 // maximum radiation allowed for growth in rad/s, considered after shielding is applied

		INPUT_RESOURCE
		{
			name = Ammonia
			rate = 0.0002777777							// 2x"kerbalism-greenhouse"
		}

		INPUT_RESOURCE
		{
			name = Water
			rate = 0.000009259247							 // 2x"kerbalism-greenhouse"
		}

		INPUT_RESOURCE
		{
			name = WasteAtmosphere						// Plants work on WasteAtmosphere and replace a scrubber, if not enough WasteAtmosphere exists then CO2 is used
			rate = 0.0036159							 // 2x"kerbalism-greenhouse"
		}

		INPUT_RESOURCE
		{
			name = CarbonDioxide							// Kerbals don't provide enough WasteAtmosphere for their required food production. If excess WasteAtmosphere is
																				// present then it will be used in place of CO2 injection
			rate = 0.0012053							// 2x"kerbalism-greenhouse"
		}

		// Note. if there is a deficiency in the amount of WasteAtmosphere needed then the missing amount of WasteAtmosphere will be added to the
		// CarbonDioxide input and Vies Versa if not enough CarbonDioxide is present and there is extra WasteAtmosphere.
		// If there is not enough resources then the plants will suffer.

		OUTPUT_RESOURCE
		{
			name = Oxygen
			rate = 0.00500331							 // 200% of oxygen required by 1 crew member
		}

		OUTPUT_RESOURCE
		{
			name = Food
			rate = 0.00000992592587						 // 200% of oxygen required by 1 crew member
		}
	}

	MODULE
	{
		name = Comfort
		bonus = plants
		desc =  There's something inherently calming about an artificial slice of nature, kept alive only by the miracles of duct-tape and kerbal engineering. Let's hope the crew doesn't think too much about it.
	}

	//	Concider those nice IVA tanks and closets for increasing current resource capacity. I won't touch em for now.
	RESOURCE
	{
		name = Ammonia
		amount = 750												// 2x"kerbalism-greenhouse"
		maxAmount = 750
	}

	RESOURCE
	{
		name = CarbonDioxide
		amount = 15000											 // 2x"kerbalism-greenhouse"
		maxAmount = 15000
	}

	// To support pressure control
	@MODULE[Configure]
	{
		@SETUP[Pressure?Control]
		{
		!RESOURCE[Nitrogen] {}
		}
	}

	RESOURCE
	{
		name = Nitrogen
		amount = 15000											// 1x"kerbalism-greenhouse" as it does not mess with crops
		maxAmount = 15000
	}

	RESOURCE
	{
		name = Water
		amount = 35												 // 2x"kerbalism-greenhouse"
		maxAmount = 35
	}
}


@PART[sspx-aquaculture-375-1]:NEEDS[StationPartsExpansionRedux,ProfileDefault]:AFTER[KerbalismDefault]  // PXL-F15H Aquaculture Module
{
	!MODULE[Greenhouse] {}
	MODULE
	{
		name = Greenhouse

		crop_resource = Food								// name of resource produced by harvests
		// Twice as effective as kerbalism-greenhouse part. 
		// See https://forum.kerbalspaceprogram.com/index.php?/topic/172400-131145-kerbalism-v180/&page=32&tab=comments#comment-3446891 for details.

		// Both growing "rings" of this greenhouse are unfortunately in the same section. No independent growing possible. (Different watering and lighting needs for different grow stages). 
		crop_size = 55									// 2x kerbalism-greenhouse
		crop_rate = 0.00000000005					 // regular growth speed
		ec_rate = 5												 // 2x"kerbalism-greenhouse"
		light_tolerance = 400.0						 // minimum lighting flux required for growth, in W/m^2
		pressure_tolerance = 0.1						// minimum pressure required for growth, in sea level atmospheres
		radiation_tolerance = 0.000008333	 // maximum radiation allowed for growth in rad/s, considered after shielding is applied

		INPUT_RESOURCE
		{
			name = Ammonia
			rate = 0.00019140625							// 2x"kerbalism-greenhouse"
		}

		INPUT_RESOURCE
		{
			name = Water
			rate = 0.0000063802							 // 2x"kerbalism-greenhouse"
		}

		INPUT_RESOURCE
		{
			name = WasteAtmosphere						// Plants work on WasteAtmosphere and replace a scrubber, if not enough WasteAtmosphere exists then CO2 is used
			rate = 0.0024915995							 // 2x"kerbalism-greenhouse"
		}

		INPUT_RESOURCE
		{
			name = CarbonDioxide							// Kerbals don't provide enough WasteAtmosphere for their required food production. If excess WasteAtmosphere is
			rate = 0.00083053315							// 2x"kerbalism-greenhouse"
		}

		// Note. if there is a deficiency in the amount of WasteAtmosphere needed then the missing amount of WasteAtmosphere will be added to the
		// CarbonDioxide input and Vies Versa if not enough CarbonDioxide is present and there is extra WasteAtmosphere.
		// If there is not enough resources then the plants will suffer.

		OUTPUT_RESOURCE
		{
			name = Oxygen
			rate = 0.0034475965							 // 200% of oxygen required by 1 crew member
		}

		OUTPUT_RESOURCE
		{
			name = Food
			rate = 0.000006380208						 // 200% of oxygen required by 1 crew member
		}
	}

	MODULE
	{
		name = Comfort
		bonus = plants
		desc =  There's something inherently calming about an artificial slice of nature, kept alive only by the miracles of duct-tape and kerbal engineering. Let's hope the crew doesn't think too much about it.
	}

	//	Concider those nice IVA tanks and closets for increasing current resource capacity. I won't touch em for now.
	RESOURCE
	{
		name = Ammonia
		amount = 544												// 2x"kerbalism-greenhouse"
		maxAmount = 544
	}

	RESOURCE
	{
		name = CarbonDioxide
		amount = 9000											 // 2x"kerbalism-greenhouse"
		maxAmount = 9000
	}

	// To support pressure control
	@MODULE[Configure]
	{
		@SETUP[Pressure?Control]
		{
		!RESOURCE[Nitrogen] {}
		}
	}

	RESOURCE
	{
		name = Nitrogen
		amount = 10000											// 1x"kerbalism-greenhouse" as it does not mess with crops
		maxAmount = 10000
	}

	RESOURCE
	{
		name = Water
		amount = 22												 // 2x"kerbalism-greenhouse"
		maxAmount = 22
	}
}

December 2, 2021

28 minutes ago, Nathangun said:

I wouldn't know were to start.

Look at the template file !LabExperimentTemplate.cfg.txt. This should have some comments that can help with the config files. The section you are looking for is the 'requirements =' section.

@KERBALISM_GROUP_SETTINGS:NEEDS[FeatureScience]
{
	@LAB_EXPERIMENTS
	{

		TEST01
		{
			ECCost = 4.62			// Value in game is times 5 (kerbalism cfg does this)
			size = 22568			// units in MB. Sample slot size is 1 per 1024 units.
			value = 24			// Default science value
			duration = 4320000		// 21,600 = 1 day. (x2 for JNSQ)
			SetupMass = 3.55		// Mass in tons
			SetupCost = 12800		// Cost added to part
			UnlockTech = advExploration	// Must have this tech to unlock the experiment.
			requirements = Greenhouse	// To remove requirements delete everything after the = sign
			CrewRequirement = Scientist:4	// Type of crew required. Blank is none required. True is any crew. Scientist is any scientist. Scientist:3 is a scientist with 3 stars (level 3).
		}

	}
}

December 2, 2021

Kerbalism Lab Experiments Expanded

Adds 65 new lab experiments that can be configured and run in any Kerbalism lab module. Stock KSP labs were too OP so Kerbalism nerfed them and in my opinion went a bit too far and made the mobile labs and scientists mostly useless. I made these in an attempt to make the labs somewhat more useful and give me an incentive to put up stations and crew them with appropriately level scientists.

Each experiment is in it's own config file so you can only include the experiments you are interested in. The zip file also includes a template file you can use to create your own experiments. In game in the VAB when you are configuring the lab experiment you will see an S<number> at the beginning of each description - S means science value and the number is the base science value you get for running the experiment.

Almost all of these experiments require a science instrument attached to the station to be able to run the experiment. The ones in this file are configured to use instruments from DMagic Orbital Science, SCANsat and Universal Storage 2. You can edit the files however you like to configure the experiment to suit your play style.

NOTE: All of these config files are using a duration designed for JNSQ. If you are using stock scale the times will be twice as long.

Dependency:
   Kerbalism
   DMagic Orbital Science (Can be removed if you edit the config files and remove the part requirement)
   SCANsat (Can be removed if you edit the config files and remove the part requirement)
   Universal Storage II (Can be removed if you edit the config files and remove the part requirement)
    Community Tech Tree (Can be removed if you edit the config files and change the required tech)

Installation:
Copy the KerbalismLabExperimentsExpanded folder to the gamedata dir. There is also an optional file called SSPX-Kerbalism-Labs.cfg that you can put in this folder or another one if you like that will enable the Kerbalism lab feature on the Stockalike Station Parts Redux parts that have lab modules if you have that mod installed.

Download:
Spacedock

=========
LICENSING

The contents of this pack are distributed under a Creative Commons Attribution-NonCommercial 4.0 International License (http://creativecommons.org/licenses/by-nc-sa/4.0/legalcode).
You are free to share and adapt the materials only for non-commercial purposes and when providing appropriate attribution. Any derivatives must be distributed under the same license.

=========

List of experiments:

Short Name	Long Name	Description	Situation	SciVal	DurDays	Tech	Requirements	CrewReq
Lab In Space
AMS-02	Alpha Magnetic Spectrometer	Looks for evidence of dark matter, dark energy and antimatter, along with very high-energy radiation coming from distant stars that could harm crew members traveling in space.	InSpaceHigh	50	364.1	advConstruction	dmSolarCollector	Scientist:4
ADVASC	Advanced Astroculture	Understanding the effects of gravity, radiation and solar light intensity on plant life is essential in preparation for future interplanetary exploration.	BodyGlobal	40	200	advExploration	Greenhouse	Scientist:2
ISSAC	International Space Station Agricultural Camera	Takes frequent infrared and visible-light images with an emphasis on forests, grasslands and agricultural fields. Improves agricultural management decisions.	InSpaceLow@Biomes HomeBody	10	1	basicScience	Part:dmscope SunAngleMax:80	Scientist:1
Platan	PLAstic Track ANalyzer	Measuring microparticle streams in the environment surrounding the Space Station according to damage, in the form of through-and-through holes in heat shielding placed above a nuclei detector.	InSpaceLow InSpaceHigh	25	30	advExploration	dmRoverMat	Scientist:3
BTN-Neutron	Study of the Fluxes of Fast and Thermal Neutrons	Focuses on the spatial and temporal distribution of neutron fluxes and spectra. These investigations help researchers to improve current in-orbit radiation models and examine the complete radiation dose crew members receive during EVAs.	VirtualBiome=InnerBelt VirtualBiome=OuterBelt VirtualBiome=Magnetosphere VirtualBiome=Storm Situation = InSpaceLow@VirtualBiomes Situation = InSpaceHigh@VirtualBiomes	20	10	advExploration	kerbalism-geigercounter	Scientist:2
Tanpopo	Astrobiology Exposure and Micrometeoroid Capture Experiments	Designed to test key questions of the “panspermia” hypothesis, a theory for the origin of life and their transport among celestial bodies.	InSpaceLow InSpaceHigh	25	180	advExploration	GooExperiment	Scientist:3
ECOSTRESS	ECOsystem Spaceborne Thermal Radiometer Experiment on Space Station	Provides the first-ever high spatiotemporal (space-time) resolution thermal infrared measurements of the surface of Kerbin.	InSpaceLow@Biomes HomeBody	12	2	advExploration	dmImagingPlatform	Scientist:3
ASIM	Atmosphere-Space Interactions Monitor	Studies Upper-atmospheric lightning, known as transient luminous events or terrestrial gamma-ray flashes from the external payload platform on the space station.	InSpaceLow Atmospheric	25	60	advExploration	SunAngleMin:95 dmImagingPlatform	Scientist:2
ASTERIA	Arcsecond Space Telescope Enabling Research in Astrophysics	Tests new technologies for astronomical observation, such as the detection of exoplanets. Requires repeated observation of stars over a long period of time from a dark environment.	BodyGlobal HomeBody	300	364.1	advExploration	Shadow scansat-recon-worldview-3-1	Scientist:4
SPOC	The Spectral Ocean Color (SPOC) Satellite	3U CubeSat with an adjustable multispectral sensor used to create images with high spectral resolution that can detect a wide range of environmental phenomena.	InSpaceLow@Biomes Oceans	10	2	advExploration	dmImagingPlatform SunAngleMax:80	Scientist:2
IT-SPINS	Ionosphere Thermosphere Scanning Photometer for Ion-Neutral Studies	Produces two-dimensional (2D) tomographic imaging of a planet's ionosphere in order to increase fundamental understanding of its structure.	InSpaceLow Atmospheric	30	90	advExploration	scansat-multi-msi-1 SunAngleMax:80	Scientist:3
JAGSAT	Spatially Resolved Measurements of Plasma Density Irregularities	Tests using a Time Domain Impedance Probe (TDIP) to measure variation in electron density in the upper layer of the ionosphere.	InSpaceLow Atmospheric	20	45	electrics	Prat:rpwsAnt	Scientist:2
STP-H6-NIRAC	Space Test Program-Houston 6-Near InfraRed Airglow Camera	Demonstrates using a near-infrared camera to make nighttime observations of airglow, the faint emission of light in the upper atmosphere.	InSpaceLow Atmospheric	50	30	advExploration	SunAngleMin:95 dmImagingPlatform	Scientist:2
BeaverCube	Project BeaverCube	Uses multiple cameras in a 3U CubeSat to take color images of a planet’s oceans and detect the temperature of cloud tops and the ocean surface.	InSpaceLow@Biomes Oceanic	10	3	advExploration	Part:dmscope SunAngleMax:80	Scientist:3
Volny	Observation, in the Near-IR Range of the Spectrum, of Wave Disturbances in the Middle Atmosphere	Records and maps wave processes in the upper mesosphere and lower thermosphere of a planet’s atmosphere.	InSpaceLow Atmospheric	30	110	advUnmanned	scansat-recon-worldview-3-1	Scientist:3
NICER	Neutron star Interior Composition Explorer	Studies the extraordinary physics of neutron stars, providing new insights into their nature and behavior.	Situation = Space HomeBody	300	728.2	scienceTech	InfraredTelescope	Scientist:4
CXBN-2	Cosmic X-Ray Background Nanosatellite	second-generation nanosatellite that refines critical measurements for explaining the origin of the Universe using an advanced materials detector system.	Situation = Space HomeBody	300	728.2	advExploration	scansat-sar-tandem-l-1	Scientist:4
Vsplesk	Seismic Effects Bursts of High-Energy Particles	Studies seismo-magnetospheric phenomena linked to a dependence between the dynamics of fluxes of high-energy, charged particles in near-Earth space and seismic activity.	InSpaceLow BodyNotAllowed=Gaseous	35	180	electrics	rpwsAnt	Scientist:3
MAXI	Monitor of All-sky X-ray Image	Designed to continuously monitor, through a systematic survey, X-ray sources and variabilities as the space station orbits a planet.	InSpaceHigh BodyAllowed=Planets	50	225	advConstruction	dmSolarCollector	Scientist:3
xMeteor	Meteor Composition Determination	Space-based observations of the chemical composition of meteors.	Situation = Space	250	15	advExploration	InfraredTelescope MaxAsteroidDistance:5000	Scientist:2
HaloSat	Hot Galactic Halo	Examines X-rays from oxygen atoms surrounding the Milky Way to determine how much matter is in the halo of our galaxy.	Situation = Space HomeBody	500	1820.5	advExploration	InfraredTelescope	Scientist:5
GEDI	Global Ecosystem Dynamics Investigation	Provides laser ranging observations of Kerbin’s forests and topography to advance the understanding of carbon and water cycling processes, biodiversity, and habitat.	InSpaceLow@Biomes HomeBody	10	1	advExploration	Part:dmscope SunAngleMax:80	Scientist:1
CubeRRT	CubeSat Radiometer Radio Frequency Interference Technology Validation	CubeSat Radiometer Radio Frequency Interference Technology Validation: Microwave radiometers provide data such as soil moisture, atmospheric water vapor, sea surface temperature and sea surface winds.	InSpaceLow@Biomes Oceanic	10	1	advExploration	dmImagingPlatform	Scientist:2
CATS	Cloud-Aerosol Transport System	uses a light detection and ranging (LiDAR) system to measure the location, composition and distribution of pollution, dust, smoke, aerosols and other particulates in the atmosphere.	HomeBody InSpaceLow@Biomes	10	1	electrics	SunAngleMax:80 dmscope	Scientist:1
CALET	CALorimetric Electron Telescope	Searches for dark matter and provides the highest measurements of the cosmic ray spectrum in order to observe discrete sources of high energy particle acceleration in our local region of the Galaxy.	Situation = Space HomeBody	350	728.2	electronics	dmSIGINT.End	Scientist:5
PWM-4	Plant Water Management 4	Demonstrates a hydroponic method for ensuring adequate hydration and aeration in no and low gravity environments to the root zone in order to sustain plants from germination through harvest.	Situation = Space HomeBody	75	200	electrics	Greenhouse	Scientist:1
PK-3plus	Plasma Crystal Research	PK-3 will give investigators a better understanding of plasma in space and will determine the critical points for the plasma.	BodyAllowed=Planets InSpaceHigh	30	90	advExploration	Prat:rpwsAnt	Scientist:2
HPRGPE-2	Haze Production Rates on Gaseous Planet Experiments	Haze particles substantially impact atmospheric temperature structures and may provide organic material to the surface of a world, potentially affecting its habitability.	Gaseous Atmospheric Not HomeBody InSpaceLow	25	45	advExploration	SunAngleMax:80 dmImagingPlatform	Scientist:2
TAPAR-1	Theory and application of the polarization-albedo rules	Studies scattering of light from porous, particulate surfaces. This information provides a straightforward method of measuring optical and structural properties of the major soil constituents leading to mineral identification.	NonAtmospheric Non Gaseous InSpaceLow@Biomes	15	2	experimentalScience	SunAngleMax:80 scansat-resources-hyperion-1	Scientist:3
SLAC-LCLS	SLAC's Linac Coherent Light Source X-ray laser	Measures warm dense matter, a super-hot, super-compressed mixture at the heart of gaseous planets.	Gaseous InSpaceLow	35	90	advExploration	rpwsAnt	Scientist:3
GPAC-DFE	Gaseous Planet Atmospheric Composition and Dynamic Flow Experiments.	Tests gaseous planets with instruments providing high-precision bolometric and Bond albedo measurements, phase functions, and mid- and far-infrared thermal luminosity experiments.	Gaseous InSpaceLow	30	60	advExploration	SunAngleMax:80 dmImagingPlatform	Scientist:3
JUNO-GSE	JUNO Gravity Science Experiment	Determine the internal structure of gaseous planets by mapping its gravity field from polar orbit.	InSpaceHigh Gaseous	40	180	advExploration	OrbitMinInclination:85 OrbitMaxInclination:95 Part:sensorGravimeter	Scientist:4
JUNO-MWR	JUNO Microwave Radiometer Experiment	Experiment that allows observing the previously unseen atmospheric features and chemical abundances hundreds of miles/km into a gas planet's atmosphere.	Gaseous InSpaceLow	35	90	scienceTech	DMagic: dmmagBoom	Scientist:3
JUNO-MAG	JUNO Vector Magnetometer Experiment	Experiment designed to detect and map the magnetic field of gaseous planets.	VirtualBiome=InnerBelt VirtualBiome=OuterBelt VirtualBiome=Magnetosphere VirtualBiome=Storm Situation = InSpaceLow@VirtualBiomes Situation = InSpaceHigh@VirtualBiomes Gaseous	30	60	advExploration	DMagic: dmmagBoom	Scientist:3
JUNO-JEDI	JUNO Jupiter Energetic-particle Detector Instrument	Experiment designed to collect data on energy, spectra, mass species (H, He, O, S), and angular distributions of charged particles.	Gaseous InSpaceLow	40	60	advExploration	rpwsAnt	Scientist:2
JUNO-WAVES	JUNO Radio and Plasma Waves	Waves is oriented towards understanding fields and particles in a gaseous planets magnetosphere.	VirtualBiome=InnerBelt VirtualBiome=OuterBelt VirtualBiome=Magnetosphere VirtualBiome=Storm Situation = InSpaceLow@VirtualBiomes Situation = InSpaceHigh@VirtualBiomes Gaseous	35	180	advExploration	DMagic: dmmagBoom	Scientist:3
JUNO-UVS	JUNO Ultraviolet Imaging Spectrometer	Experiment making remote observations of a gas planets aurora, detecting the emissions of gases such as hydrogen in the far-ultraviolet.	Gaseous InSpaceLow	45	90	scienceTech	dmImagingPlatform	Scientist:3
JUNO-JIRAM	JUNO Jovian Infrared Auroral Mapper	Experiment to probe the upper layers of a gas planets atmosphere down to pressures of 5–7 bars at infrared wavelengths in the 2–5 μm interval using an imager and a spectrometer.	Gaseous InSpaceLow	35	60	advExploration	dmImagingPlatform	Scientist:2
SOLAR-FIELDS	Electromagnetic Fields Investigation	This investigation will make direct measurements of electric and magnetic fields, radio waves, Poynting flux, absolute plasma density, and electron temperature.	Suns	45	180	advExploration	rpwsAnt	Scientist:3
SOLAR-ISOIS	Integrated Science Investigation of the Sun	This investigation will measure energetic electrons, protons and heavy ions.	Suns	40	180	advExploration	rpwsAnt	Scientist:3
SOLAR-WISPR	Wide-field Imager for Solar Probe	These optical telescopes will acquire images of the corona and inner heliosphere.	Suns	35	90	advExploration	dmImagingPlatform	Scientist:3
SOLAR-SWEAP	Solar Wind Electrons Alphas and Protons	This investigation will count the electrons, protons and helium ions, and measure their properties such as velocity, density, and temperature.	Suns	35	90	advExploration	dmImagingPlatform	Scientist:3
SOCP-7	Satellite Observation and Classification Project	Record and map satellite biomes and surface features of planetary moons.	Moons	10	2	advExploration	scansat-multi-abi-1 SunAngleMax:80	Scientist:2

Lab On Ground

ChemCam-2	Chemistry & Camera	An instrument that first uses a laser to vaporize materials then later analyzes their elemental composition using an on-board spectrograph.	SrfLanded@Biomes Not HomeBody	12	10	spaceExploration	dmsurfacelaser	Scientist:1
MastCam-1		A camera that takes color images and color video footage of the terrain. The instrument is also used to study the landscape and support the driving and sampling operations of rovers.	SrfLanded@Biomes Not HomeBody	10	15	spaceExploration	dmscope Sunlight	Scientist:2
PPME-1	Planetary Portable Magnetometer Experiment	Studies changes in local planetary magnetic fields by making measurements over several months. Allows differentiation between local and remote fields.	SrfLanded@Biomes Not HomeBody	10	10	spaceExploration	DMagic: dmmagBoom	Scientist:2
PPSE-1	Planetary Passive Seismic Experiment	Studies the propagation of seismic waves through the planet and provides a detailed look at the planet's internal structure.	SrfLanded@Biomes Not HomeBody	8	5	spaceExploration	sensorAccelerometer	Scientist:1
ALSEP-2	Heat Flow Experiment	Measures the rate at which temperature increases with depth. This can be used to determine the rate of heat loss from the interior of a planet.	SrfLanded@Biomes Not HomeBody	10	1	spaceExploration	sensorThermometer	Scientist:1
Strata-1		Investigates the properties and behavior of regolith on airless bodies. Studies how to set anchors in regolith, how to safely move and process large volumes of regolith, and predict and prevent risk to spacecraft and astronauts visiting these small bodies.	SrfLanded@Biomes NonAtmospheric Not HomeBody	10	10	scienceTech	ResourceRates = [email protected]	Scientist:1
SODI-Colloid	Selectable Optical Diagnostics Instrument - Aggregation of Colloidal Suspensions	Studies the growth, mixing, and ordering effects and aggregation from solutions of colloids on airless planets.	SrfLanded Not homebody NonAtmospheric	25	60	advExploration	Part:science_module	Scientist:2
Qucopartex-22		Tests how exposure to the space environment affects various materials, including their rate of deterioration and stability. The materials include high quality beryl and volcanic glass pebbles.	SrfLanded Not homebody NonAtmospheric	25	45	advExploration	Part:science_module	Scientist:2
BASM-4	Broadband Angular Selective Material experiments	Polymer Convection examines the effect of gravity on formation and crystallization of Broadband Angular Selective Material, an optical material with the ability to control the reflection and absorption of light.	SrfLanded Not homebody	25	60	advExploration	Part:science_module	Scientist:2
TPSMMO	Thermophysical Properties of Supercooled Molten Metal Oxides	Measures thermophysical properties (density and viscosity) of high-temperature oxide melts using the Electrostatic Levitation Furnace (ELF)	SrfLanded Not homebody	30	90	advExploration	sensorThermometer	Scientist:3
EGOMDOAF	Experiments with a Global Ocean Model Driven by Observed Atmospheric Forcing	Studies the magnitude and phase of midlatitude heat storage with wind forcing and associated upwelling and downwelling of heat plumes.	Oceanic SrfSplashed@Biomes	20	60	advExploration	dmBathymetry	Scientist:3
MEGCO	Mesoscale Eddies in the General Circulation of the Ocean	Tests a two-layer, quasi-geostrophic, general circulation model of the ocean with fine horizontal resolution on planets with oceans.	Oceanic SrfSplashed@Biomes	20	45	advExploration	dmBathymetry	Scientist:3
SWE-NEMO	Surface wave effects in the NEMO ocean model	Experiments are done with NEMO in ocean-only (forced) mode and coupled to the ECMWF atmospheric and wave models.	Oceanic SrfSplashed@Biomes	20	60	advExploration	dmBathymetry	Scientist:3
GLACE-2	Global Land–Atmosphere Coupling Experiment	Measures land–atmosphere coupling strength, or the degree to which anomalies in land surface state (e.g., soil moisture) can affect rainfall generation and other atmospheric processes.	SrfLanded@Biomes Not homebody Atmospheric	12	90	scienceTech	sensorAtmosphere	Scientist:3
RSA-CA	Reactions at surfaces in the atmosphere-chemistry of aerosols	Study of the nature of particle surfaces and how this determines interactions with gases in the atmosphere, including water, which is important for cloud formation and properties.	SrfLanded@Biomes Not homebody Atmospheric	12	90	advExploration	sensorAtmosphere	Scientist:3
CRISTA-1	Cryogenic Infrared Spectrometers and Telescopes for the Atmosphere	Instrument used to determine whether and to what extent small-scale structures in global trace gas distributions and in dynamics are present in the middle atmosphere.	SrfLanded@Biomes Not homebody Atmospheric	10	30	scienceTech	USFluidSpectroWedge	Scientist:1
IBATE-IWC	Interactions between the atmosphere and terrestrial ecosystems: influence on weather and climate	Examins short-term and long-term influences of the land surface on weather and climate.	SrfLanded@Biomes Not homebody Atmospheric	10	30	advExploration	Part:dmscope Sunlight	Scientist:1
DCT-APB1	Dust charging and transport on airless planetary bodies	Tests theories on dust charging and transport that have been suggested to explain a variety of unusual phenomena on the surfaces of airless planetary bodies.	SrfLanded@Biomes NonAtmospheric	15	180	advExploration	rpwsAnt	Scientist:3
SWAB-5	Space weathering on airless bodies	Tests the optical properties of soils which are shown to be highly dependent on the cumulative amount of npFe, which varies with different starting materials and the energetics of different parts of the solar system.	SrfLanded@Biomes NonAtmospheric	10	30	advExploration	Part:science_module	Scientist:2
MILV-ELDAPB	Measurements of initial launch velocities of electrostatically lofted dust on airless planetary bodies	Tests electrostatic dust loftings role in surface evolution of airless bodies as indicated from a number of unexplained observations, including the munar horizon glow and dust ponding on asteroids	SrfLanded NonAtmospheric	40	180	advExploration	rpwsAnt	Scientist:4
ORZS-3	Optimization of Root Zone Substrates	Tests methods for growing and sustaining plants on other planets with the goal of minimizing imports of food for ground based kerbonaughts.	SrfLanded Not homebody	35	200	advExploration	Greenhouse	Scientist:2
GV-SSPB	Gravity Variations in Substrate Structures on Planetary Bodies	Analyses minute differences in gravity to determine the interior structure of planets.	SrfLanded@Biomes Not homebody	12	200	advExploration	Part:sensorGravimeter	Scientist:2

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Kerbalism Greenhouses - Convert to rate based instead of harvest based.

[1.5 - 1.10] Kerbalism 3.11

[Kerbalism 3.14] Kerbalism Lab Experiments Expanded

[1.5 - 1.10] Kerbalism 3.11

Kerbalism Greenhouses - Convert to rate based instead of harvest based.

[Kerbalism 3.14] Kerbalism Lab Experiments Expanded

[Kerbalism 3.14] Kerbalism Lab Experiments Expanded

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