Photonics engineers involved in designing and operating Fourier transform spectrometers (FTS) often rely on Maxwell’s
wave equations and time-frequency (distance-wavenumber) Fourier theory as models to understand and predict the
conversion of optical energy to electrical signals in their instruments. Dr. Chandrasekhar Roychoudhuri and his
colleagues, at last year’s conference, presented three significant concepts that might completely change the way we
comprehend the interaction of light and matter and the way interference information is generated.
The first concept is his non-interaction of waves (NIW) formulation, which puts in place an optical wave description that
more accurately describe the properties of the finite time and spatial signals of an optical system. The second is a new
description for the cosmic EM environment that recognizes that space is really filled with the ether of classical
electromagnetics. The third concept is a new metaphysics or metaphotonics that compares the photon as a particle in a
void against the photon as a wave in a medium to see which best explain the twelve different aspects of light. Dr. Henry
Lindner presents a compelling case that photons are waves in a medium and particles (electrons, protons, atoms) are
wave-structures embedded in the new ether. Discussion of the three new principles is intended to increase the curiosity
of photonics engineers to investigate these changes in the nature of light and matter.
Recent discoveries from analysis of measurements made by the Sounding of the Atmosphere
using Broadband Emission Radiometry (SABER) instrument on the Thermosphere-Ionosphere-
Mesosphere Energetics and Dynamics (TIMED) satellite have shown that NO(v) 5.3 um
emission is the primary mechanism of dissipating solar-geomagnetic storm energy in the
thermosphere. Further insight into the ionosphere-thermosphere (IT) storm-time response
emerged from observations and analysis of the SABER 4.3 um channel radiances, which showed
that nighttime 4.3 um emission is dominated by NO+(v) during geomagnetically disturbed
conditions. Analysis of SABER NO+(v) 4.3 um emission led to major advances in the
understanding of E-region ion-neutral chemistry and kinetics, such as the identification of a new
source of auroral 4.3 um emission, which also provides a new context for understanding auroral
infrared emission from O2(a1▵g). Surprisingly, NO+(v) 4.3 um emission is the second largest
contribution to solar-geomagnetic infrared radiative response and provides a non-negligible
contribution to the "natural thermostat" thought to be solely due to NO(v) 5.3 um emission.
Despite these major advances, a fully physics-based understanding of the two largest sources of
storm-time energy dissipation in the IT system from NO(v) and NO+(v) is lacking because of the
limited information content contained in SABER's broadband infrared channel measurements.
On the other hand, detailed information on the chemical-radiative excitation and loss processes
for NO(v), NO+(v), and O2(a1▵g) emission is encoded in the infrared spectrum, of which SABER
only provides an integral constraint. Consequently, a prototype infrared field-wide Michelson
interferometer (FWMI) is currently under development to advance the understanding of IT
storm-time energetics beyond the current state of knowledge. It is anticipated that progress in the
developments of the FWMI technology, along with advancements in a physics-based
understanding of the fundamental chemical-radiative mechanisms responsible for IT infrared
emission, will play an integral role in the future planning of a rocket-borne and satellite-based Eregion
science missions. In this paper, a survey of recent SABER discoveries in IT ion-neutral
coupling will be given, open questions in a physics-based understanding of chemical-radiative
vibration-rotation excitation and loss from important IT infrared emitters will be identified, and
the FWMI instrument requirements necessary to address these open science questions will be
presented.
Recent broadband observations by the SABER sensor aboard the TIMED satellite hint at intriguing new vibrationrotation
excitation and loss processes that occur in the energy dissipation of the ionosphere-thermosphere as it
responds to solar storms. To address the questions exposed by the SABER data, SDL's field-widened interferometer
has been brought back after three decades to again fly into or above aurorally disturbed atmosphere to gain the data
needed to better understand the different processes of ionosphere-thermosphere energetics. The paper discusses the
evaluation and design phases (laboratory evaluation, a rocket flight, and a satellite flight) needed to prepare this
elegant and unique interferometer to reach its goal of making high resolution (0.5 cm-1) and wide bandwidth (1300-
8000 cm-1) measurements of the ionosphere-thermosphere world-wide. Design details of interferometer will be
presented along with comparisons between a standard Michelson interferometer and the field-widened sensor to
illustrate just how the Bounchareine and Connes field-widened form provides the enhanced performance needed for
the new missions. The paper also describes how the improved Inferometer design will leverage advances in modern
electronics, detectors, bearing design and software to gain significant improvements in the performance of the
upgraded field-widened interferometer-spectrometer when compared to the heritage instrument.
The radiative balance of the troposphere, and hence global climate, is dominated by the infrared absorption and emission of water vapor, particularly at far-infrared (far-IR) wavelengths from 15-50 μm. Current and planned satellites observe the infrared region to about 15.4 μm, ignoring spectral measurement of the far-IR region from 15 to 100μm. The far-infrared spectroscopy of the troposphere (FIRST) project, flown in June 2005, provided a balloon-based demonstration of the two key technologies required for a space-based far-IR spectral sensor. We discuss the FIRST Fourier transform spectrometer system (0.6 cm-1 unapodized resolution), its radiometric calibration in the spectral range from 10 to 100 μm, and its performance and science data from the flight. Two primary and two secondary goals are given and data presented to show the goals were achieved by the FIRST flight.
The radiative balance of the troposphere, and hence global climate, is dominated by the infrared absorption and emission of water vapor, particularly at far-infrared (far-IR) wavelengths from 15-50 μm. Water vapor is the principal absorber and emitter in this region. The distribution of water vapor and associated far-IR radiative forcings and feedbacks are widely recognized as major uncertainties in our understanding of current and the prediction of future climate. Cirrus clouds modulate the outgoing longwave radiation (OLR) in the far-IR. Up to half of the OLR from the Earth occurs beyond 15.4 μm (650 cm-1). Current and planned operational and research satellites observe the midinfrared to only about 15.4 μm, leaving space or airborne spectral measurement of the far-IR region unsupported. NASA has now developed the sensor required to make regular far-IR measurements of the Earth's atmosphere possible. Far InfraRed Spectroscopy of the Troposphere (FIRST) was developed for NASA's Instrument Incubator Program under the direction of the Langley Research Center. The objective of FIRST is to provide a balloon-based demonstration of the key technologies required for a space-based sensor. The FIRST payload will also be proposed for science flights in support of validation of the various experiments on the Earth Observing System (EOS). We discuss the FIRST Fourier transform spectrometer system (0.6 cm-1 unapodized resolution), along with its radiometric calibration in the spectral range from 10 to 100 µm (1000 to 100 cm-1). FIRST incorporates a broad bandpass beamsplitter, a cooled (~180 K) high throughput optical system, and an image type detector system. We also discuss the actual performance of the FIRST instrument relative to its performance goal of a NE(delta)T of 0.2 K from 10 to 100 μm.
The radiative balance of the troposphere, and hence global climate, is dominated by the infrared absorption and emission of water vapor, particularly at far-infrared (far-IR) wavelengths from 15-50 μm. Water vapor is the principle absorber and emitter in this region. The distribution of water vapor and associated far-IR radiative forcings and feedbacks are widely recognized as major uncertainties in our understanding of current and the prediction of future climate. Cirrus clouds modulate the outgoing longwave radiation (OLR) in the far-IR, and up to half of the OLR from the Earth occurs beyond 15.4 μm (650 cm-1). Current and planned operational and research satellites observe the mid-infrared to only about 15.4 μm, leaving space or airborne spectral measurement of the far-IR region unsupported. NASA is now developing the technology required to make regular far-IR measurements of the Earth’s atmosphere possible. Far InfraRed Spectroscopy of the Troposphere (FIRST) is being developed for NASA’s Instrument Incubator Program under the direction of the Langley Research Center. The objective of FIRST is to provide a balloon-based demonstration of the key technologies required for a space-based sensor. We discuss the FIRST Fourier transform spectrometer system (0.6 cm-1 unapodized resolution), along with radiometric calibration techniques in the spectral range from 10 to 100 μm (1000 to 100 cm-1). FIRST will incorporate a broad bandpass beamsplitter, a cooled (~180 K) high throughput optical system, and an image type detector system. The FIRST performance goal is a NEΔT of 0.2 K from 10 to 100 μm.
FIRST (a NASA Instrument Incubator Program) is a balloon-based demonstration of a space-based sensor to measure the Earth’s thermal infrared at high spatial and spectral resolution. The radiative balance of the troposphere, and hence climate, is dominated by the infrared absorption and emission of water vapor, particularly at far-infrared (far-IR) wavelengths longer than 15 µm (650 cm-1), the distribution of water vapor and its far-IR radiative forcings and feedbacks are major uncertainties in understanding and predicting future climate. However, far-IR emission (spectra of band-integrated) has rarely been directly measured from space platforms. FIRST will be a Fourier Transform Spectrometer (FTS) with radiometric calibration in the spectral range from 10 to 100 µm (1000 to 100 cm-1) at 0.6 cm-1 unapodized resolution. It will incorporate a broad bandpass beamsplitters and a high-throughput optical and detector system. FIRST has a NEΔT performance goal of 0.2K from 10 to 100 µm. The spectral resolution will allow simultaneous retrievals of temperature and water vapor profiles. A 10 × 10 array of 10 km IFOVs is desired isolate clear and cloudy fields of view, while providing daily global coverage capability.
A helium-cooled interferometer was flown aboard shuttle flight STS-39. This interferometer, along with its sister radiometer, set new benchmarks for the quantity and quality of data collected. The interferometer generated approximately 150,000 interferograms during the course of the flight. Data was collected at tangent heights from the earth's surface to celestial targets. The interferograms encoded spectral data from aurora, earth limb, and earth terminator scenes. The interferometer collected data at resolutions of 8, 4, and 1 wavenumbers over a spectral range of 2 to 25 micrometers. The interferometer's optics, detectors and preamps, laser reference system, realignment system, and eight-position optical filter wheel are described as they performed on-orbit.
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