Synonyms: 
DC8
DC-8
NASA DC8
NASA DC-8 -AFRC
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Diode Laser Hygrometer

The DLH has been successfully flown during many previous field campaigns on several aircraft, most recently ACTIVATE (Falcon); FIREX-AQ, ATom, KORUS-AQ, and SEAC4RS (DC-8); POSIDON (WB-57); CARAFE (Sherpa); CAMP2Ex and DISCOVER-AQ (P-3); and ATTREX (Global Hawk). This sensor measures water vapor (H2O(v)) via absorption by one of three strong, isolated spectral lines near 1.4 μm and is comprised of a compact laser transceiver and a sheet of high grade retroflecting road sign material to form the optical path. Optical sampling geometry is aircraft-dependent, as each DLH instrument is custom-built to conform to aircraft geometric constraints. Using differential absorption detection techniques, H2O(v) is sensed along the external path negating any potential wall or inlet effects inherent in extractive sampling techniques. A laser power normalization scheme enables the sensor to accurately measure water vapor even when flying through clouds. An algorithm calculates H2O(v) concentration based on the differential absorption signal magnitude, ambient pressure, and temperature, and spectroscopic parameters found in the literature and/or measured in the laboratory. Preliminary water vapor mixing ratio and derived relative humidities are provided in real-time to investigators.

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Conical Scanning Millimeter-wave Imaging Radiometer

CoSMIR is an airborne, 9-channel total power imaging radiometer that was originally developed for the calibration/validation of the Special Sensor Microwave Imager/Sounder (SSMIS). When first completed in 2003, the system had four receivers that measured horizontally polarized radiation at 50.3, 52.8, 53.6, 150, 183.3±1, 183.3±3, and 183.3±6.6 GHz, and dual-polarized (vertical and horizontal) radiation at 91.665 GHz. Following the SSMIS calibration/validation efforts, CoSMIR served as the airborne high-frequency simulator for the Global Precipitation Measurement (GPM) Microwave Imager (GMI) in four GPM field campaigns from 2011 to 2015. The channels were modified slightly to match the GMI channels more closely: 53.6 was removed, 91.655 changed to 89.0, 150 changed to 165.5 and made dual-polarized, and 183.3±6.6 changed to 183.3±7. In 2020 and 2022, CoSMIR flew on the NASA ER-2 in IMPACTS (Investigation of Microphysics and Precipitation for Atlantic Coast Threatening Snowstorms). CoSMIR’s submillimeter-wave sibling (CoSSIR) flew in the third deployment of IMPACTS in 2023.

CoSMIR is currently undergoing modifications through Decadal Survey Incubation (DSI) funds to become CoSMIR-Hyperspectral (CoSMIR-H). CoSMIR-H will retain the current 89 and 165 GHz dual-polarized channels and switch out the 50 and 183 GHz receivers for hyperspectral receivers spanning 50-58 GHz and 175-191 GHz, providing thousands of channels at these frequencies instead of the current two 50-GHz and three 183-GHz channels. Test flights of CoSMIR-H are tentatively scheduled for Summer 2024.

All the CoSMIR receivers and radiometer electronics are housed in a small cylindrical scan head (21.5 cm in diameter and 28 cm in length) that is rotated by a two-axis gimbaled mechanism capable of generating a wide variety of scan profiles. Two calibration targets, one maintained at ambient (cold) temperature and another heated to a hot temperature of about 323 K, are closely coupled to the scan head and rotate with it about the azimuth axis. Radiometric signals from each channel are sampled at 10 ms intervals. These signals and housekeeping data are fed to the main computer in an external electronics box.

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Differential Absorption Carbon monOxide Measurement

The in‐situ diode laser spectrometer system, referred to by its historical name DACOM, includes three tunable diode lasers providing 4.7, 4.5, and 3.3 μm radiation for accessing CO, N2O, and CH4 absorption lines, respectively. The three laser beams are combined by the use of dichroic filters and are then directed through a small volume (0.3 liter) Herriott cell enclosing a 36 meter optical path. As the three coincident laser beams exit the absorption cell, they are spectrally isolated using dichroic filters and are then directed to individual detectors, one for each laser wavelength. Wavelength reference cells containing CO, CH4, and N2O are used to wavelength lock the operation of the three lasers to the appropriate absorption lines. Ambient air is continuously drawn through a Rosemount inlet probe and a permeable membrane dryer which removes water vapor before entering the Herriott cell and subsequently being exhausted via a vacuum pump to the aircraft cabin. To minimize potential spectral overlap from other atmospheric species, the Herriott cell is maintained at a reduced pressure of ~90 Torr. At 5 SLPM mass flow rate, the absorption cell volume is exchanged nominally twice per second. Frequent but short calibrations with well documented and stable reference gases are critical to achieving both high precision and accuracy. Calibration for all species is accomplished by periodically (~4 minutes) flowing calibration gas through this instrument. Measurement accuracy is closely tied to the accuracy of the reference gases obtained from NOAA/ESRL, Boulder, CO. Both CO and CH4 mixing ratios are provided in real-time to investigators aboard the DC‐8.

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Carbon Monoxide By Attenuation of Laser Transmission

COBALT makes measurements using off-axis integrated output spectroscopy.

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Cloud Particle Imager

The CPI records high-resolution (2.3 micron pixel size) digital images of particles that pass through the sample volume at speeds up to 200 m/s. In older models, CCD camera flashes up to 75 frames per second (fps), potentially imaging more than 25 particles per frame. More recent camera upgrades capable of bringing frame rate to nearly 500 fps. Real time image processing crops particle images from the full frame, eliminating blank space and compressing data by >1000:1. CPI is designed for ummanned use, with AI parameters to optimize performance without supervision.

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Digital Mapping System

The Digital Mapping System (DMS) is an airborne digital camera system that acquires high resolution natural color and panchromatic imagery from low and medium altitude research aircraft. The DMS includes an Applanix Position and Orientation system to allow precision image geo-rectification. Data acquired by DMS are used by a variety of scientific programs to monitor variation in environmental conditions, assess global change, and respond to natural disasters.

Mission data are processed and archived by the Airborne Sensor Facility (ASF) located at the NASA Ames Research Center in Mountain View, CA. DMS imagery from Operation IceBridge are archived at the National Snow and Ice Data Center in Boulder, CO.

Instrument Type: Canon/Zeiss Camera with IMU/GPS
Measurements: 21-Mpixel natural color Imagery

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Digital Camera System

DCS is a 16-megapixel color infrared digital camera system, providing high resolution imagery for mission tracking purposes Geo-referenced image products may be generated, when used in conjunction with a POS-AV system.

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Cloud Spectrometer and Impactor

The Cloud Spectrometer and Impactor (CSI) combines the counterflow virtual impactor with a new lightweight cloud droplet probe to allow for detailed studies of total condensed water (TCW), liquid and ice, in clouds. The CSI can measure TCW from ~ 1 mg/m3 to several g/m3 depending on the configuration; in addition particle sizes from 2 to 50 μm are resolved with the droplet probe. The instrumentation can be mounted externally on most aircraft.

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Counterflow Virtual Impactor

The NCAR counterflow virtual impactor (CVI) (Noone et al., 1988; Twohy et al., 1997) is an airborne instrument that can be used for studies of aerosol/cloud interactions, cloud physics, and climate. At the CVI inlet tip, cloud droplets or ice crystals larger than about 8 µm aerodynamic diameter are separated from the interstitial aerosol and impacted into dry nitrogen gas. This separation is possible via a counterflow stream of nitrogen out the CVI tip, which assures that only larger particles (cloud droplets or ice crystals) are sampled. Because droplets or crystals in a sampling volume of about 200 l/min are impacted into a sample stream of approximately 10 l/min, concentrations within the CVI are significantly enhanced. The water vapor and non-volatile residual nuclei remaining after droplet evaporation are sampled downstream of the inlet with selected instruments. These may include a Lyman-alpha or similar hygrometer, a condensation nucleus counter, an optical particle counter, filters for chemical analyses, or user instruments.

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Carbon Dioxide Laser Absorption Spectrometer

The CO2LAS instrument was jointly developed by JPL and Lockheed Martin Coherent Technologies under funding from the NASA Earth Science Technology Office Instrument Incubator Program.

The instrument uses three continuous-wave (c.w.) Th:Ho:YLF lasers, one of which is used as an absolute frequency reference and is locked to a carbon dioxide absorption line in an internal gas cell using a phase modulation spectroscopy scheme. The remaining two lasers are offset frequency locked from the reference laser to provide the online and offline beams that are propagated through the atmosphere. The online and offline beams are expanded to an eye-safe level and transmitted to the ground where they are reflected back to the instrument, collected by the receive optics and detected. The use of the offset frequency-locking scheme together with the absolute frequency reference enables the absolute frequency of the online and offline lasers to be held to within 200 kHz of the desired values. The CO2LAS transceiver uses separate co-axial transmit/receive paths for each of the on-line and off-line channels.

A Doppler frequency shift is induced between the outgoing and return signals by pointing the transmit beams slightly off nadir. This frequency offset, together with a polarization transmit/receive architecture, ensures the receive signals are separated from the transmit signals by both polarization and frequency. The nominal Doppler offset is 15 MHz but this will vary as the aircraft attitude changes. The return signals on each channel are digitized and stored during flight for post-processing. Throughput of the data collection system was increased from ~8% to >20% between 2006 and 2007.

In order to ensure the instrument remains stable, the output power and frequency of all three lasers are monitored. The output power values for the online and offline lasers are used in the determination of the on-line and off-line absorption as part of the LAS measurement. The output power value for the reference laser is used primarily as a laser health status to check the integrity of the CO2 line center lock.

The electronics for the CO2LAS are mounted in two racks that typically mount to the seat rails of the host aircraft. One rack contains the control electronics for the transceiver system, laser controller, frequency locking electronics and provides the user interface for the overall system.

The second rack houses the chiller that supplies the optical transceiver with coolant and the signal processor which receives housekeeping data from the electronics rack, and digitizes, stores and analyzes the lidar return signal. The CO2LAS uses a Gigabit Ethernet system to distribute data across the system and to other computers that can be connected into the gigabit hub located in the back of one of the racks.

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