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.
Auroral infrared emission observed from the TIMED/SABER broadband 4.3 um channel is used
to develop an empirical geomagnetic storm correction to the International Reference Ionosphere
(IRI) E-region electron densities. The observation-based proxy used to develop the storm model
is SABER-derived NO+(v) 4.3 um volume emission rates (VER). A correction factor is defined
as the ratio of storm-time NO+(v) 4.3 um VER to a quiet-time climatological averaged NO+(v)
4.3 um VER, which is linearly fit to available geomagnetic activity indices. The initial version of
the E-region storm model, called STORM-E, is most applicable within the auroral oval region.
The STORM-E predictions of E-region electron densities are compared to incoherent scatter
radar electron density measurements during the Halloween 2003 storm events. Future STORM-E
updates will extend the model outside the auroral oval.
The response of the ionospheric E-region to solar-geomagnetic storms can be characterized using observations of infrared 4.3 um emission. In particular, we utilize nighttime TIMED/SABER measurements of broadband 4.3 um limb emission and derive a new data product, the NO+(v) volume emission rate, which is our primary observationbased
quantity for developing an empirical storm-time correction the IRI E-region electron density. In this paper we describe our E-region proxy and outline our strategy for developing the empirical storm model. In our initial studies, we analyzed a six day storm
period during the Halloween 2003 event. The results of this analysis are promising and suggest that the ap-index is a viable candidate to use as a magnetic driver for our model.
The SABER radiometer on the TIMED spacecraft scans the earthlimb continuously in ten channels spanning the spectrum from 1.27 to 15 μm. The signature of the diurnal tide in the equatorial region is apparent throughout the mesosphere in TIMED/SABER data, especially in the CO2 15-μm radiance profiles. In addition, layer structures are apparent in a large fraction of the both the radiance profiles and the kinetic temperature profiles derived from them. We present results showing tidal and layer features in the variation with local time and latitude of 15-μm radiance and temperature. Temperature inversion layers (TILs) are regions of extreme perturbations in the retrieved temperature profile where the temperature increases rapidly over 3-10 km range by tens of degrees K, sometimes approaching increases of 100 K, and are not represented in any existing atmospheric climatologies. Theories that have been proposed connect them with the amplitude and phase of atmospheric tides, as well as with the interactions and dissipation of atmospheric gravity waves and planetary waves. The radiance local maxima, or "knees," are more mysterious. Their occurrence is rather unpredictable and not well explained by models, although it is known that they are due to vibrational excitation of CO2 by atomic oxygen and they may have tidal connections. While they may be associated with strong TILs, the most important class occurring at tangent heights in the lower thermosphere between 100 and 115 km appear not to be simply related to local inversion layers. SABER data offers the opportunity to do the first global survey of MLT TILs, determine their spatial extent and persistence time, and develop a global climatology of their occurrence and properties.
KEYWORDS: Temperature metrology, Satellites, Data processing, Environmental sensing, Data centers, Stratosphere, Meteorology, Data analysis, Earth observing sensors, Mesosphere
MIPAS on ENVISAT measures vertical profiles of atmospheric temperature, ozone, and other species with nearly global coverage and
high accuracy/precision. The standard observation mode covers the altitude region between 6 and 68 km. The atmospheric state parameters
retrieved from MIPAS measurements using the IMK data analysis processor are compared with a number of other satellite observations. Our comparisons in this paper will focus on temperatures measured by MIPAS, HALOE, SABER, and UKMO Stratospheric Assimilated Data. Both individual profiles and zonal means measured by MIPAS and other
instruments at different seasons and geolocations show reasonable agreement, though some differences exist due to characteristics of the
individual instruments and observation scenarios. The MIPAS measurements during the stratospheric major sudden warming during the southern hemisphere winter of 2002 are also presented to show the
features of this unusual event. The analysis indicates the reliability of MIPAS-IMK data products and their capability for providing valuable scientific information.
The Sounding of the Atmosphere using Broadband Emission Radiometry
(SABER) experiment was launched onboard the TIMED satellite in
December, 2001. SABER is designed to provide measurements of temperature, constituents, and the key radiative and chemical sources and sinks of energy in the mesosphere and lower thermosphere (MLT). SABER measures Earth limb emission in 10 broadband radiometer channels ranging from 1.27 μm to 17 μm. Measurements are made both day and night over the latitude range from 52°S to 83°N with alternating hemisphere coverage every 60 days. In this paper we
concentrate on retrieved profiles of kinetic temperature (Tk) and CO2 volume mixing ratio (vmr), inferred from observed 15 μm and 4.3 μm limb emissions. SABER-measured limb radiances are in non-local thermodynamic
equilibrium (non-LTE) in the MLT region. The complexity of non-LTE
radiation transfer combined with the large volume of data measured
by SABER requires new retrieval approaches and radiative transfer
techniques to accurately and efficiently retrieve the data
products. In this paper we present the salient features of the
coupled non-LTE Tk/CO2 retrieval algorithm, along with preliminary results.
The radiative balance of the troposphere, and hence climate, is influenced strongly by radiative cooling associated with emission of infrared radiation by water vapor, particularly at far-infrared (far-IR) wavelengths greater than 15 micrometers and extending out beyond 50micrometers . Water vapor absorption and emission is principally due to the pure rotation band, which includes both line and continuum absorption. The distribution of water vapor and associated far-IR radiative forcings and feedbacks are well-recognized as major uncertainties in understanding and predicting future climate. Up to half of the outgoing longwave radiation (OLR) from the Earth occurs beyond 15.4 micrometers (650 cm-1_ depending on atmospheric and surface conditions. Cirrus clouds also modulate the outgoing longwave radiation in the far-IR. However, despite this fundamental importance, far-IR emission (spectra of band- integrated) has rarely been directly measured from space, airborne, or ground-based platforms. Current and planned operational and research satellites typically observe the mid-infrared only to about 15.4 micrometers . In this talk we will review the role of the far-IR radiation in climate and will discuss the scientific and technical requirements for far-IR measurements of the Earth's atmosphere.
Since the early 1970's, infrared remote sensing of water vapor has been based exclusively on observations of mid-infrared (mid-ir) emission from the strong 6.3 micrometers vibration-rotation band. However, the outgoing longwave radiation from Earth is dominated by emission in the far-infrared (far-ir) at wavelengths greater than 15 micrometers . The source of this far-ir radiation is upper tropospheric water vapor. Furthermore, there are a growing number of novel instrument concepts that propose measuring the thermal far-ir spectrum for the purpose of radiation budget sensing and climate fingerprinting. As a result, we investigate the feasibility of retrieving upper tropospheric water vapor from nadir-viewing observations of far-ir spectral emission. We find that it is possible to retrieve upper tropospheric water vapor from measurements of the far-ir spectral radiation, and that the vertical resolution can be significantly improved by combining measurements from the far-ir and mid-ir spectrum.
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