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ADEOS II
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Illustration of ADEOS II | |||||||||||||
| Names | Advanced Earth Observing Satellite II Midori II ADEOS 2 | ||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Mission type | Earth observation Environmental monitoring | ||||||||||||
| Operator | NASDA | ||||||||||||
| COSPAR ID | 2002-056A | ||||||||||||
| SATCAT no. | 27597 | ||||||||||||
| Mission duration | 5 years (planned) 10 months and 9 days (achieved) | ||||||||||||
| Spacecraft properties | |||||||||||||
| Bus | ADEOS | ||||||||||||
| Manufacturer | Mitsubishi Electric Corporation | ||||||||||||
| Launch mass | 3,680 kg (8,110 lb) | ||||||||||||
| Payload mass | 1,300 kg (2,900 lb) | ||||||||||||
| Dimensions | 6 × 4 × 4 m (20 × 13 × 13 ft) | ||||||||||||
| Power | 5.3 kW | ||||||||||||
| Start of mission | |||||||||||||
| Launch date | 14 December 2002, 01:31 UTC | ||||||||||||
| Rocket | H-IIA 202 | ||||||||||||
| Launch site | Tanegashima Space Center, Yoshinobu 1 | ||||||||||||
| Contractor | Mitsubishi Heavy Industries | ||||||||||||
| End of mission | |||||||||||||
| Last contact | 23 October 2003, 23:55 UTC | ||||||||||||
| Orbital parameters | |||||||||||||
| Reference system | Geocentric orbit[1] | ||||||||||||
| Regime | Sun-synchronous orbit | ||||||||||||
| Perigee altitude | 806 km (501 mi) | ||||||||||||
| Apogee altitude | 807 km (501 mi) | ||||||||||||
| Inclination | 98.70° | ||||||||||||
| Period | 101.00 minutes | ||||||||||||
| Instruments | |||||||||||||
| |||||||||||||
ADEOS II (Advanced Earth Observing Satellite 2) was an Earth observation satellite (EOS) launched by NASDA,[2] with contributions from NASA and CNES, in December 2002.[3] and it was the successor to the 1996 mission ADEOS I. The mission ended in October 2003 after the satellite's solar panels failed.[4]
Mission overview
[edit]The three primary objectives of the mission, as identified by NASDA, were to:[5]
- Regularly monitor the water and energy cycle as a part of the global climate system
- Quantitatively estimate the biomass and fundamental productivity as a part of the carbon cycle
- Detect trends in long term climate change as a result of continuing the observations started by ADEOS I
The project had a proposed minimum life of three years, with a five-year goal.[6]
Instruments
[edit]
The satellite was equipped with five primary instruments: Advanced Microwave Scanning Radiometer (AMSR), Global Imager (GLI), Improved Limb Atmospheric Spectrometer-II (ILAS-II), Polarization and Directionality of the Earth's Reflectances (POLDER), and SeaWinds. These instruments were designed to monitor Earth's water cycle, study biomass in the carbon cycle, and detect trends in long-term climate change. The mission was established to continue the work undertaken by ADEOS I between 1996 and 1997.[6][7]
Advanced Microwave Scanning Radiometer (AMSR)
[edit]AMSR monitors water vapor, precipitation, sea surface, wind, and ice by means of microwave radiation emanating from Earth's surface and atmosphere. It is a radiometer that operates in eight frequency bands covering 6.9 GHz to 89 GHz, and monitors the horizontal and vertical polarizations separately. With a dish of 2 m (6 ft 7 in) aperture, the spatial resolution is 5 km (3.1 mi) in the 89 GHz band, degrading to 60 km (37 mi) at 6.9 GHz.[8]
Global Imager (GLI)
[edit]GLI (GLobal Imager) is an optical sensor to observe solar radiation reflected from Earth's surface and map vegetation, clouds, etc. The data is acquired in 23 visible/near-infrared, and in 13 far infrared channels. The scanning is done by a rotating mirror covering 12 km (7.5 mi) along track and 1,600 km (990 mi) cross-track, and at a resolution of 1 km (0.62 mi). [9]
Improved Limb Atmospheric Spectrometer 2 (ILAS-2)
[edit]ILAS-2 maps the vertical distribution of O3, NO2, HNO3, H2O, CFC-11, CFC-12, CH4, N2O, and ClONO2, as well as the distribution of temperature and pressure, all in the stratosphere. It observes the absorption spectrum in Earth's atmospheric limb in the 3-13 micron wavelength band, and in the 753-784 nm band of the occulting Sun. The altitude resolution is 100 m (330 ft).[10]
Polarization and Directionality of Earth's Reflectances (POLDER)
[edit]POLDER measures the polarization, and spectral characteristics of the solar light reflected by aerosols, clouds, oceans and land surfaces. Eight narrow band wavelengths (443, 490, 564, 670, 763, 765, 865, and 910 nm) are covered by the instrument which enables identification of the physical and optical properties of the aerosols and their role in radiation budget.[11]
SeaWinds
[edit]SeaWinds is a scatterometer that provides wind speed and direction by observing the microwave reflection from ocean surfaces. With its 1 m (3 ft 3 in) dish, it scans the surface along conical surfaces at 18 RPM. It provides speed at an accuracy of 2 m/s, wind direction at an accuracy of 20°, both with a spatial resolution of 5 km (3.1 mi).[12]
Subsystems
[edit]In addition to the five main instruments, nine avionic subsystems were allocated to the bus module. These were the Communication and Data-Handling Subsystem (C&DH), Inter-Orbit Communication Subsystem (IOCS), Mission Data Processing Subsystem (MDPS), Optical Data Recorder (ODR), Electrical Power Subsystem (EPS), Paddle Subsystem (PDL), Attitude and Orbit Control Subsystem (AOCS), Reaction Control Subsystem (RCS), and the Direct Transmission Subsystem (DTL).[2]
The C&DH subsystem received and decoded the satellite's tracking control command signals and acted as a processing interface between the instruments. It was capable of adjusting settings on the instruments – such as temperature and voltage. The IOCS was used to communicate with data relay satellites (see Data transfer).[2]
The MDP device formatted mission data to be sent via the IOCS, and would process it into a data packet. The ODR was a large-volume storage device that used an optical magnetic disk system. The EPS provided power to the satellite's subsystems. The PDL managed the satellite's solar panel, and transferred electrical energy to the EPS. The solar panel was capable of generating 5 kW using 55,680 solar cells on a jointed mast.[2]
The AOCS was used to establish the attitude control following the satellite's deployment from the launch vehicle. It was subsequently used to adjust the satellite's attitude, orbit, and solar paddle. The AOCS was equipped with a number of attitude sensors, including a control-standard unit (IRC), an Earth sensor (ESA), and a fine Sun sensor assembly (FSSA).[2]
The RCS was used to generate propulsion power for attitude adjustments after deployment and control orbit using data from the AOCS.[2]
Data transfer
[edit]ADEOS II transferred data to and from Artemis and the Data Relay Test Satellite (DRTS). The Artemis connection transferred information over a 26 GHz Ka-band link (for payload data) and a 2 GHz S-band link (for telemetry, tracking and control data).[2]
These signals were then downlinked to the Earth Observation Center (EOC) via feeder link stations and the Redu Station. ADEOS II also sent mission data directly to NASA stations, which routed information to bodies such as the EOC and sensor-providing organisations.[2]
Launch
[edit]The mission was originally scheduled to launch aboard a H-II launch vehicle in February 2002. This was postponed as the Japanese Space Activities Commission would not launch without having three successful missions aboard the new H-IIA launch vehicle.[13]
The satellite was successfully launched from Tanegashima Space Center pad YLP-1 on 14 December 2002, aboard H-IIA 202.[14] Other payloads onboard included the Japanese MicroLabsat and WEOS microsatellites, as well as the Australian FedSat.[15]
Failure
[edit]On 23 October 2003, the solar panel failed. At 23:49 UTC, the satellite switched to "light load" operation due to an unknown error. This was intended to power down all observation equipment to conserve energy. At 23:55 UTC, communications between the satellite and the ground stations ended, with no further telemetry received.[4] Further attempts to procure telemetry data on 24 October 2003 (at 00:25 and 02:05 UTC) also failed.[16]
Investigation
[edit]After the power failure, JAXA formed the Midori II anomaly investigation team. Analysis of data received before transmissions ceased showed that the solar panel's power output had decreased from 6 kW to 1 kW. The investigation team began surveying the mission to establish whether the failure was due to a technical malfunction or a solar flare.[4]
One hypothesis was that debris had impacted the satellite's power harness between the solar array and the satellite bus. The harness was a core of wires enclosed in multi-layer insulation. The debris impact was theorised to have caused an electric arc,[2] which is an example of the spacecraft charging effect.[17]
The mission officially ended at the end of October 2003, with JAXA conceding that the "possibility of restoring the operations of Midori II [was] extremely slim". The mission, which had cost approximately 70 billion Yen (US$570 million)[15] was only able to recoup an estimated 300 million Yen through insurance.[4]
References
[edit]- ^ "ADEOS 2 2002-056A 27597". NASA. 28 October 2021. Retrieved 29 October 2021.
This article incorporates text from this source, which is in the public domain.
- ^ a b c d e f g h i "ADEOS-II (Advanced Earth Observing Satellite-II) / Midori-II". ESA eoPortal Directory. 2021. Retrieved 29 October 2021.
- ^ "ADEOS-2". NASA. Archived from the original on 27 September 2010. Retrieved 30 October 2021.
This article incorporates text from this source, which is in the public domain.
- ^ a b c d "Midori I (ADEOS I)". Satellite News Digest. 2006. Archived from the original on 5 October 2011. Retrieved 18 September 2010.
- ^ "Scientific Goal". JAXA. 15 November 1999. Retrieved 27 September 2010.
- ^ a b "Advanced Earth Observing Satellite II" (PDF). NASA GSFC. 2007. Archived from the original (PDF) on 9 June 2010. Retrieved 17 September 2010.
This article incorporates text from this source, which is in the public domain.
- ^ "Midori II (ADEOS II)". Satellite News Digest. 2003. Archived from the original on 5 October 2011. Retrieved 17 September 2010.
- ^ "AMSR". NASA. 28 October 2021. Retrieved 30 October 2021.
This article incorporates text from this source, which is in the public domain.
- ^ "GLI". NASA. 28 October 2021. Retrieved 30 October 2021.
This article incorporates text from this source, which is in the public domain.
- ^ "ILAS-2". NASA. 28 October 2021. Retrieved 30 October 2021.
This article incorporates text from this source, which is in the public domain.
- ^ "POLDER". NASA. 28 October 2021. Retrieved 30 October 2021.
This article incorporates text from this source, which is in the public domain.
- ^ "SeaWinds". NASA. 28 October 2021. Retrieved 30 October 2021.
This article incorporates text from this source, which is in the public domain.
- ^ "Missions - SeaWinds on ADEOS II". NASA JPL. 2002. Archived from the original on 20 September 2010. Retrieved 29 October 2021.
This article incorporates text from this source, which is in the public domain.
- ^ "ADEOS 2 (Midori 2)". Gunter's Space Page. Retrieved 19 September 2010.
- ^ a b "Midori 2 (ADEOS 2) - Summary". Space and Tech. 2001. Archived from the original on 22 June 2011. Retrieved 17 September 2010.
- ^ "Operational Anomaly with Midori-II". JAXA. 25 October 2003. Archived from the original on 17 June 2011. Retrieved 27 September 2010.
- ^ "Understanding the Potential Dangers of Spacecraft Charging - NASA". 12 January 2017.
External links
[edit]- Japan Aerospace Exploration Agency (2007), Advanced Earth Observing Satellite-II "Midori II"(ADEOS-II), JAXA, archived from the original on 10 January 2010, retrieved 18 September 2010
ADEOS II
View on GrokipediaMission Background
Development History
The Advanced Earth Observing Satellite II (ADEOS II), also known as Midori II, originated as a successor to the original ADEOS mission launched by Japan's National Space Development Agency (NASDA, now part of JAXA) in August 1996, which provided valuable Earth observation data for nearly a year before failing in June 1997 due to a power system malfunction.[1][4] NASDA initiated planning for ADEOS II in the late 1990s as part of its broader ADEOS program to advance global environmental monitoring, focusing on climate, ocean, and atmospheric studies following the partial success of ADEOS I.[1][5] Key development milestones began with the issuance of the ADEOS Series Research Announcement in January 1997, inviting international proposals for instrument utilization and scientific research, with a submission deadline in April 1997 and selected research teams starting work in August 1997.[5] The project received formal approval from NASDA and Japan's Ministry of the Environment for fiscal year 2000, emphasizing ozone layer monitoring via the ILAS-II instrument, with spacecraft assembly led by Mitsubishi Electric Corporation drawing on lessons from ADEOS I.[4] Integration of international instruments progressed through the early 2000s, culminating in pre-launch completion by late 2002, though the initial target launch date of 1999 was postponed to December 2002 aboard an H-IIA rocket from Tanegashima Space Center.[1][4][6] International collaborations were central to ADEOS II's development, with NASDA serving as the primary lead in Japan while partnering with the U.S. National Aeronautics and Space Administration (NASA) for the SeaWinds scatterometer, developed by NASA's Jet Propulsion Laboratory at a cost of $154 million including operations.[7][1] France's Centre National d'Études Spatiales (CNES) provided the POLDER-2 instrument for aerosol and cloud observation, and Japan's Environment Agency contributed to the ILAS-II for atmospheric profiling.[8][4] These partnerships, aligned with global initiatives like the World Climate Research Programme, ensured diverse sensor capabilities but required extensive coordination for integration and calibration.[4] Development faced challenges, including delays stemming from the analysis of ADEOS I's failure, which shared similar solar panel designs and prompted enhancements in redundancy and reliability to mitigate power risks.[6][1] This analysis influenced ADEOS II's bus design, incorporating improved fault-tolerant systems, though it extended the timeline beyond the original 1999 goal and the revised June 2000 target.[6][4]Objectives and Scope
The ADEOS II mission, launched by Japan's National Space Development Agency (NASDA, now part of the Japan Aerospace Exploration Agency (JAXA)), aimed to advance global environmental monitoring by providing continuous observations of Earth's carbon and water cycles, climate variability, and atmospheric composition, thereby supporting international research on global change.[1][9] These core goals built upon the foundational objectives of its predecessor, ADEOS I, but expanded to emphasize quantitative assessments essential for understanding interactions within the Earth system.[10] The mission's scope encompassed targeted monitoring of key environmental parameters, including ocean surface winds and temperatures to track heat exchange and circulation patterns, land vegetation mapping for assessing ecosystem health and productivity, ozone layer profiling to evaluate stratospheric depletion trends, and studies of aerosols and clouds to analyze their roles in radiative forcing and air quality.[1][11] These efforts were designed to contribute geophysical data products that enhance models of biological and physical processes, such as biomass estimation and trace gas distributions, without delving into specific measurement techniques.[9] ADEOS II was planned for a nominal mission duration of three years, operating in a sun-synchronous orbit at approximately 803 km altitude with a 99° inclination and a 101-minute orbital period, enabling about 14 orbits per day for consistent global coverage at a local solar time of 10:30.[1][10] This configuration supported interdisciplinary Earth system science by integrating data into major global programs, including the Global Energy and Water Cycle Experiment (GEWEX), the Global Observations of Forest Cover and Land Dynamics (GOFC-GOLD), and the Integrated Global Observing Strategy (IGOS).[9][11]Spacecraft Design
Bus and Core Subsystems
The ADEOS II spacecraft featured a modular bus design consisting of a mission module for instruments and a bus module housing core avionics, structured as a rectangular prism with dimensions of approximately 6 meters in length, 4 meters in width, and 4 meters in height when including appendages. This configuration represented an upgraded version of the ADEOS I platform, incorporating enhanced redundancy in critical subsystems to improve reliability for the planned three-year mission lifetime. The total launch mass reached 3,680 kg, enabling deployment into a sun-synchronous orbit at around 800 km altitude.[1][7][4] Core subsystems supported autonomous operations and environmental resilience. The command and data handling (C&DH) subsystem utilized an onboard computer to manage command reception and decoding via a 2 GHz band, telemetry editing for status parameters like temperature and voltage, instrument control, and data processing for weekly operational plans. Thermal control was achieved through a combination of heaters, radiators, and passive elements to maintain component stability across orbital conditions, ensuring operational integrity for the bus and attached modules. The propulsion subsystem employed a reaction control system (RCS) with hydrazine-fueled 1 N and 20 N thrusters for orbit maintenance maneuvers and attitude adjustments, provisioned with fuel sufficient for five years of operations.[4][7][10] Telemetry and tracking integrated S-band communications for housekeeping data transmission and command uplink, with rates supporting real-time monitoring, alongside Ka-band and X-band for higher-volume data relay when interfaced with external systems. Attitude determination relied on a three-axis strapdown system incorporating an inertial reference unit with gyroscopes, Earth sensors, fine sun sensors, and GPS receivers to achieve pointing accuracy better than 0.3 degrees. The deployed solar array spanned approximately 24 meters, generating over 5 kW of power at end-of-life to support these subsystems.[1][4][7]Power and Attitude Control Systems
The power system of ADEOS II was designed to provide reliable energy for its Earth observation instruments and subsystems during its sun-synchronous orbit. It featured two deployable solar array paddles constructed with gallium arsenide (GaAs) solar cells, arranged in 50 flexible blankets containing 55,680 cells total, mounted on a 24-meter extendible mast for optimal sun exposure.[1][10] These panels generated up to 5 kW of power at end-of-life conditions, sufficient to support the satellite's peak demands while accounting for degradation over the mission lifetime.[1][4] For periods of eclipse or peak load, the system included nickel-hydrogen (Ni-H2) batteries to store and supply energy as needed.[1] Power distribution occurred via a 28 V DC bus, managed by the electrical power subsystem (EPS), which handled regulation, battery charge/discharge cycles, and allocation to onboard components, incorporating dual buses for enhanced reliability against single-point failures derived from lessons of the predecessor ADEOS I mission.[1][4] The attitude and orbit control subsystem (AOCS) employed three-axis stabilization with zero-momentum control to maintain precise orientation relative to Earth, essential for nadir-pointing instruments like the Global Imager and SeaWinds. Primary actuation was provided by four reaction wheel assemblies (RWAs) for fine adjustments in roll, pitch, and yaw, supplemented by two magnetic torquers (MTQs) for desaturation and disturbance rejection using Earth's magnetic field.[1][10] Attitude determination integrated a GPS receiver (GPSR) with an inertial reference unit for high-precision navigation, achieving knowledge accuracies of approximately 0.1° in roll, 0.08° in pitch, and 0.14° in yaw, which supported an overall nadir pointing accuracy of 0.1 degrees.[1][4] Redundancy was built in through backup sensors, including Earth sensors and fine sun sensors, and dual-string configurations for critical AOCS electronics to ensure fault-tolerant operation.[1] To optimize power collection, the solar arrays were equipped with solar array drive assemblies (SADAs) that enabled continuous sun-tracking via stepper motors and integrated position sensors, allowing independent rotation of each paddle relative to the spacecraft body for maximum efficiency across orbital phases.[1] This gimbal mechanism, combined with the AOCS, facilitated seamless integration with the satellite's structural bus, ensuring stable power input without compromising attitude stability.[4] Overall, these systems provided the robust foundation for ADEOS II's multi-instrument payload, drawing on proven designs while incorporating redundancies to mitigate risks identified in prior missions.[1]Instruments
Advanced Microwave Scanning Radiometer (AMSR)
The Advanced Microwave Scanning Radiometer (AMSR) was a passive microwave radiometer instrument aboard the ADEOS II satellite, developed and provided by Japan's National Space Development Agency (NASDA, now part of JAXA).[1] It operated as a conically scanning, total-power system with dual polarization at most frequencies, designed to measure Earth's microwave emissions for deriving geophysical parameters related to the water cycle.[12] The instrument featured eight frequencies ranging from 6.925 GHz to 89.0 GHz, enabling observations across a broad spectrum of microwave bands to capture thermal emissions from the surface and atmosphere.[13] The AMSR's antenna was a 2-meter diameter offset parabolic reflector, the largest of its kind for a spaceborne microwave radiometer at the time, which allowed for enhanced spatial resolution in global observations.[10] It scanned conically at a 40 rpm rate with a nominal Earth incidence angle of approximately 55°, directing the beam across the satellite's ground track to provide continuous coverage.[1] This design facilitated the measurement of brightness temperatures, which served as the basis for retrieving parameters such as soil moisture with an accuracy of ±0.04 m³/m³, sea surface salinity, precipitation rates over oceans, and vegetation water content.[1] Additional derived products included sea surface temperature, wind speed, atmospheric water vapor, cloud liquid water, snow water equivalent, and sea ice concentration, supporting applications in climate monitoring and weather forecasting.[14] The instrument achieved a swath width of approximately 1,600 km, enabling near-global coverage in its sun-synchronous orbit.[13] Spatial resolutions varied by frequency, ranging from about 5 km at 89.0 GHz to 60 km at 6.925 GHz, with the higher frequencies providing finer detail for features like precipitation structures while lower frequencies penetrated deeper into vegetation for soil and moisture assessments.[12] For example, the 6.925 GHz channel offered resolutions around 40 × 70 km, suitable for large-scale soil moisture mapping, whereas the 89.0 GHz channel resolved details at 3 × 6 km for ice and rain detection.[1] Calibration was performed using onboard references, including a hot load target at approximately 300 K and a cold-sky mirror reflecting deep space at about 3 K, applied at the start and end of each scan rotation.[13] These internal methods were supplemented by vicarious calibration techniques, leveraging known targets such as stable land surfaces or ocean areas to correct for instrumental drift and ensure brightness temperature accuracy within 1–2 K across channels.[10] The noise equivalent temperature difference ranged from 0.3 K at lower frequencies to 1.8 K at 50.3 GHz, maintaining reliable sensitivity for weak microwave signals.[12]Global Imager (GLI)
The Global Imager (GLI) was a sophisticated optical instrument aboard the ADEOS II satellite, designed as a 36-channel multispectral pushbroom scanner for high-resolution Earth observations across visible, near-infrared, shortwave infrared, and thermal infrared wavelengths ranging from 0.38 to 12.0 μm. Developed by Japan's National Space Development Agency (NASDA, now part of JAXA), it featured an off-axis Gregorian telescope with a 300 mm aperture to collect incoming radiation, coupled with linear detector arrays—typically comprising silicon detectors for visible/near-infrared bands, indium gallium arsenide for shortwave infrared, and mercury cadmium telluride for thermal bands—that enabled simultaneous imaging along the flight track while a scanning mirror provided cross-track coverage.[1][4] GLI's core capabilities centered on deriving key environmental parameters through its spectral channels, including the normalized difference vegetation index (NDVI) for assessing global vegetation health and biomass, aerosol optical depth for monitoring atmospheric pollution and clarity (with target accuracy of 0.05 or 10%), cloud top height and optical thickness for weather and climate studies, and snow/ice extent and albedo for cryosphere analysis. The instrument's design prioritized frequent global coverage to support carbon cycle monitoring, ocean productivity estimation, and land surface process studies, building on the legacy of prior sensors like the Ocean Color and Temperature Scanner.[4][10][15] With a swath width of 1600 km at nadir, GLI achieved spatial resolutions of 250 m for six high-priority visible and shortwave infrared channels dedicated to detailed terrestrial and oceanic features, while the remaining 30 channels operated at 1 km resolution for broader thermal infrared coverage, enabling efficient mapping of heterogeneous landscapes without excessive data volume. Operational modes included nadir viewing for standard global surveys, as well as tilted configurations (±20° along-track) facilitated by the adjustable scanning mirror, which allowed for stereoscopic imaging, along-track angle observations to mitigate sun glint over oceans, and enhanced temporal sampling in targeted regions. These modes, combined with continuous thermal infrared acquisition during both day and night, supported a 4-day recurrent orbit cycle for near-global revisit times.[1][4][10]Improved Limb Atmospheric Spectrometer 2 (ILAS-2)
The Improved Limb Atmospheric Spectrometer-II (ILAS-II), developed by Japan's Ministry of the Environment (MOE) and National Institute for Environmental Studies (NIES), was a solar occultation instrument designed for measuring vertical profiles of stratospheric trace gases and aerosols, primarily in polar regions, as part of ADEOS-II's contribution to atmospheric research.[4] It featured four spectrometers: three infrared Fourier transform spectrometers and one visible grating spectrometer, utilizing a 13 cm Cassegrain telescope, beam splitters, a two-axis gimbal mirror for sun-tracking, a sun-edge sensor, and signal processing units.[1] The infrared channels covered wavelengths from 3.0–5.7 µm (22 channels), 6.21–11.76 µm (44 channels), and 12.78–12.85 µm (22 channels), while the visible channel spanned 753–784 nm (1024 channels).[1] Cryogenic cooling was provided by a Stirling-cycle mechanical cooler to maintain detector temperatures around 77 K, ensuring low noise for infrared detection.[4] The instrument was mounted on the ADEOS-II spacecraft's mission module, oriented nadir-pointing in a sun-synchronous orbit to enable sunset and sunrise occultation observations.[4] ILAS-II's capabilities centered on retrieving vertical profiles of key atmospheric constituents, including ozone (O₃), nitric acid (HNO₃), nitrogen dioxide (NO₂), nitrous oxide (N₂O), methane (CH₄), water vapor (H₂O), chlorine nitrate (ClONO₂), chlorofluorocarbons (CFC-11 and CFC-12), and aerosol extinction coefficients, along with temperature and pressure data up to 60 km altitude.[1] It also detected polar stratospheric clouds (PSCs) and provided insights into aerosol distributions relevant to ozone chemistry.[4] Operations focused on high latitudes, covering 57–73°N and 64–88°S, with approximately 100 occultation events per day—derived from 14 orbits daily, each yielding multiple measurement points—to support studies of ozone depletion and stratospheric dynamics.[4] These profiles contributed to broader mission objectives for monitoring global atmospheric composition changes, such as those driven by human activities.[1] The instrument achieved a vertical resolution of approximately 1–1.5 km and a horizontal tangent resolution of 1.5–2 km in the visible channel, with infrared fields of view ranging from 13–21.7 km horizontally.[1] This resolution enabled detailed profiling of thin stratospheric layers, surpassing the coarser capabilities of prior systems.[4] ILAS-II represented an upgrade from the ILAS instrument on ADEOS-I, incorporating enhanced detector stability through improved cooling and signal-to-noise ratios, as well as additional infrared channels for better coverage of species like ClONO₂.[1] These advancements addressed limitations in the original ILAS, such as spectral gaps and reduced precision in polar observations, allowing for more reliable data during ADEOS-II's operational period from April to October 2003.[16]| Parameter | Specification |
|---|---|
| Infrared Channels | 3.0–5.7 µm (22 ch.), 6.21–11.76 µm (44 ch.), 12.78–12.85 µm (22 ch.) |
| Visible Channel | 753–784 nm (1024 ch.) |
| Vertical Profiles | O₃, HNO₃, NO₂, N₂O, CH₄, H₂O, ClONO₂, CFC-11, CFC-12, aerosols, temperature, pressure |
| Altitude Range | 10–60 km |
| Daily Occultations | ~100 events (high latitudes) |
| Vertical Resolution | 1–1.5 km |
| Horizontal Resolution | 1.5–21.7 km (channel-dependent) |