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1. The CRISM investigation in Mars orbit: Overview, history, and delivered data products

Author

Seelos, Frank P., Seelos, Kimberly D., Murchie, Scott L., Novak, M. Alexandra Matiella, Hash, Christopher D., Morgan, M. Frank, Arvidson, Raymond E., Aiello, John, Bibring, Jean-Pierre, Bishop, Janice L., Boldt, John D., Boyd, Ariana R., Buczkowski, Debra L., Chen, Patrick Y., Clancy, R. Todd, Ehlmann, Bethany L., Frizzell, Katelyn, Hancock, Katie M., Hayes, John R., Heffernan, Kevin J., Humm, David C., Itoh, Yuki, Ju, Maggie, Kochte, Mark C., Malaret, Erick, McGovern, J. Andrew, McGuire, Patrick, Mehta, Nishant L., Moreland, Eleanor L., Mustard, John F., Nair, A. Hari, Núñez, Jorge I., O'Sullivan, Joseph A., Packer, Liam L., Poffenbarger, Ryan T., Poulet, Francois, Romeo, Giuseppe, Santo, Andrew G., Smith, Michael D., Stephens, David C., Toigo, Anthony D., Viviano, Christina E., and Wolff, Michael J.

Published
2024
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2. Satellite sensor requirements for monitoring essential biodiversity variables of coastal ecosystems.

Author

Siegel, David, Miller, Robert, Humm, David, Izenberg, Noam, Keller, Mary, Morgan, Frank, Frouin, Robert, Dekker, Arnold, Gardner, Royal, Goodman, James, Schaeffer, Blake, Franz, Bryan, Pahlevan, Nima, Mannino, Antonio, Concha, Javier, Ackleson, Steven, Cavanaugh, Kyle, Romanou, Anastasia, Tzortziou, Maria, Boss, Emmanuel, Pavlick, Ryan, Freeman, Anthony, Rousseaux, Cecile, Dunne, John, Long, Matthew, Klein, Eduardo, McKinley, Galen, Goes, Joachim, Letelier, Ricardo, Kavanaugh, Maria, Roffer, Mitchell, Bracher, Astrid, Arrigo, Kevin, Dierssen, Heidi, Zhang, Xiaodong, Muller-Karger, Frank, Best, Ben, Guralnick, Robert, Moisan, John, Sosik, Heidi, Mouw, Colleen, Barnard, Andrew, Palacios, Sherry, Roesler, Collin, Drakou, Evangelia, Appeltans, Ward, Jetz, Walter, Ade, Christiana, Turpie, Kevin, Davis, Frank, Roberts, Dar, Kudela, Raphe|Raphael, and Hestir, Erin

Subjects
H4 imaging, aquatic, coastal zone, ecology, essential biodiversity variables, hyperspectral, remote sensing, vegetation, wetland, Biodiversity, Oceans and Seas, Phytoplankton, Remote Sensing Technology
Abstract

The biodiversity and high productivity of coastal terrestrial and aquatic habitats are the foundation for important benefits to human societies around the world. These globally distributed habitats need frequent and broad systematic assessments, but field surveys only cover a small fraction of these areas. Satellite-based sensors can repeatedly record the visible and near-infrared reflectance spectra that contain the absorption, scattering, and fluorescence signatures of functional phytoplankton groups, colored dissolved matter, and particulate matter near the surface ocean, and of biologically structured habitats (floating and emergent vegetation, benthic habitats like coral, seagrass, and algae). These measures can be incorporated into Essential Biodiversity Variables (EBVs), including the distribution, abundance, and traits of groups of species populations, and used to evaluate habitat fragmentation. However, current and planned satellites are not designed to observe the EBVs that change rapidly with extreme tides, salinity, temperatures, storms, pollution, or physical habitat destruction over scales relevant to human activity. Making these observations requires a new generation of satellite sensors able to sample with these combined characteristics: (1) spatial resolution on the order of 30 to 100-m pixels or smaller; (2) spectral resolution on the order of 5 nm in the visible and 10 nm in the short-wave infrared spectrum (or at least two or more bands at 1,030, 1,240, 1,630, 2,125, and/or 2,260 nm) for atmospheric correction and aquatic and vegetation assessments; (3) radiometric quality with signal to noise ratios (SNR) above 800 (relative to signal levels typical of the open ocean), 14-bit digitization, absolute radiometric calibration

Published
2018

3. Satellite sensor requirements for monitoring essential biodiversity variables of coastal ecosystems

Author

Muller-Karger, Frank E, Hestir, Erin, Ade, Christiana, Turpie, Kevin, Roberts, Dar A, Siegel, David, Miller, Robert J, Humm, David, Izenberg, Noam, Keller, Mary, Morgan, Frank, Frouin, Robert, Dekker, Arnold G, Gardner, Royal, Goodman, James, Schaeffer, Blake, Franz, Bryan A, Pahlevan, Nima, Mannino, Antonio G, Concha, Javier A, Ackleson, Steven G, Cavanaugh, Kyle C, Romanou, Anastasia, Tzortziou, Maria, Boss, Emmanuel S, Pavlick, Ryan, Freeman, Anthony, Rousseaux, Cecile S, Dunne, John, Long, Matthew C, Klein, Eduardo, McKinley, Galen A, Goes, Joachim, Letelier, Ricardo, Kavanaugh, Maria, Roffer, Mitchell, Bracher, Astrid, Arrigo, Kevin R, Dierssen, Heidi, Zhang, Xiaodong, Davis, Frank W, Best, Ben, Guralnick, Robert, Moisan, John, Sosik, Heidi M, Kudela, Raphael, Mouw, Colleen B, Barnard, Andrew H, Palacios, Sherry, Roesler, Collin, Drakou, Evangelia G, Appeltans, Ward, and Jetz, Walter

Subjects
Life Below Water, Life on Land, Biodiversity, Oceans and Seas, Phytoplankton, Remote Sensing Technology, aquatic, coastal zone, ecology, essential biodiversity variables, H4 imaging, hyperspectral, remote sensing, vegetation, wetland, Environmental Sciences, Biological Sciences, Agricultural and Veterinary Sciences, Ecology
Abstract

The biodiversity and high productivity of coastal terrestrial and aquatic habitats are the foundation for important benefits to human societies around the world. These globally distributed habitats need frequent and broad systematic assessments, but field surveys only cover a small fraction of these areas. Satellite-based sensors can repeatedly record the visible and near-infrared reflectance spectra that contain the absorption, scattering, and fluorescence signatures of functional phytoplankton groups, colored dissolved matter, and particulate matter near the surface ocean, and of biologically structured habitats (floating and emergent vegetation, benthic habitats like coral, seagrass, and algae). These measures can be incorporated into Essential Biodiversity Variables (EBVs), including the distribution, abundance, and traits of groups of species populations, and used to evaluate habitat fragmentation. However, current and planned satellites are not designed to observe the EBVs that change rapidly with extreme tides, salinity, temperatures, storms, pollution, or physical habitat destruction over scales relevant to human activity. Making these observations requires a new generation of satellite sensors able to sample with these combined characteristics: (1) spatial resolution on the order of 30 to 100-m pixels or smaller; (2) spectral resolution on the order of 5 nm in the visible and 10 nm in the short-wave infrared spectrum (or at least two or more bands at 1,030, 1,240, 1,630, 2,125, and/or 2,260 nm) for atmospheric correction and aquatic and vegetation assessments; (3) radiometric quality with signal to noise ratios (SNR) above 800 (relative to signal levels typical of the open ocean), 14-bit digitization, absolute radiometric calibration

Published
2018

4. Calibration of ShadowCam

Author

Humm, David Carl, primary, Kinczyk, Mallory Janet, additional, Brylow, Scott Michael, additional, Wagner, Robert Vernon, additional, Speyerer, Emerson Jacob, additional, Estes, Nicholas Michael, additional, Mahanti, Prasun, additional, Boyd, Aaron Kyle, additional, and Robinson, Mark Southwick, additional

Published
2023
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6. ShadowCam Instrument and Investigation Overview

Author

Robinson, Mark Southwick, primary, Brylow, Scott Michael, additional, Caplinger, Michael Alan, additional, Carter, Lynn Marie, additional, Clark, Mattew John, additional, Denevi, Brett Wilcox, additional, Estes, Nicholas Michael, additional, Humm, David Carl, additional, Mahanti, Prasun, additional, Peckham, Douglas Arden, additional, Ravine, Michael Andrew, additional, Schaffner, Jacob Andrieu, additional, Speyerer, Emerson Jacob, additional, and Wagner, Robert Vernon, additional

Published
2023
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7. The CRISM investigation in Mars orbit: Overview, history, and delivered data products

Author

Seelos, Frank P., primary, Seelos, Kimberly D., additional, Murchie, Scott L., additional, Novak, M. Alexandra Matiella, additional, Hash, Christopher D., additional, Morgan, M. Frank, additional, Arvidson, Raymond E., additional, Aiello, John, additional, Bibring, Jean-Pierre, additional, Bishop, Janice L., additional, Boldt, John D., additional, Boyd, Ariana R., additional, Buczkowski, Debra L., additional, Chen, Patrick Y., additional, Clancy, R. Todd, additional, Ehlmann, Bethany L., additional, Frizzell, Katelyn, additional, Hancock, Katie M., additional, Hayes, John R., additional, Heffernan, Kevin J., additional, Humm, David C., additional, Itoh, Yuki, additional, Ju, Maggie, additional, Kochte, Mark C., additional, Malaret, Erick, additional, McGovern, J. Andrew, additional, McGuire, Patrick, additional, Mehta, Nishant L., additional, Moreland, Eleanor L., additional, Mustard, John F., additional, Nair, A. Hari, additional, Núñez, Jorge I., additional, O'Sullivan, Joseph A., additional, Packer, Liam L., additional, Poffenbarger, Ryan T., additional, Poulet, Francois, additional, Romeo, Giuseppe, additional, Santo, Andrew G., additional, Smith, Michael D., additional, Stephens, David C., additional, Toigo, Anthony D., additional, Viviano, Christina E., additional, and Wolff, Michael J., additional

Published
2023
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9. MRO/CRISM retrieval of surface Lambert albedos for multispectral mapping of Mars with DISORT-based radiative transfer modeling: phase 1--using historical climatology for temperatures, aerosol optical depths, and atmospheric pressures

Author

McGuire, Patrick C., Wolff, Michael J., Smith, Michael D., Arvidson, Raymond E., Murchie, Scott L., Clancy, R. Todd, Roush, Ted L., Cull, Selby C., Lichtenberg, Kim A., Wiseman, Sandra M., Green, Robert O., Martin, Terry Z., Milliken, Ralph E., Cavender, Peter J., Humm, David C., Seelos, Frank P., Seelos, Kim D., Taylor, Howard W., Ehlmann, Bethany L., Mustard, John F., Pelkey, Shannon M., Titus, Timothy N., Hash, Christopher D., and Malaret, Erick R.

Subjects
Astrogeology -- Models, Astrogeology -- Analysis, Remote sensing -- Usage, Remote sensing -- Analysis, Albedo -- Analysis, Paleoclimatology -- Models, Paleoclimatology -- Analysis, Mars (Planet) -- Atmosphere, Mars (Planet) -- Observations, Mars (Planet) -- Models, Mars (Planet) -- Analysis, Business, Earth sciences, Electronics and electrical industries
Abstract

We discuss the DISORT-based radiative transfer pipeline ('CRISM_LambertAlb') for atmospheric and thermal correction of MRO/CRISM data acquired in multispectral mapping mode (~200 m/pixel, 72 spectral channels). Currently, in this phase-one version of the system, we use aerosol optical depths, surface temperatures, and lower atmospheric temperatures, all from climatology derived from Mars Global Surveyor Thermal Emission Spectrometer (MGS-TES) data and from surface altimetry derived from MGS Mars Orbiter Laser Altimeter (MOLA). The DISORT-based model takes the dust and ice aerosol optical depths (scaled to the CRISM wavelength range), the surface pressures (computed from MOLA altimetry, MGS-TES lower atmospheric thermometry, and Viking-based pressure climatology), the surface temperatures, the reconstructed instrumental photometric angles, and the measured I/F spectrum as inputs, and then a Lambertian albedo spectrum is computed as the output. The Lambertian albedo spectrum is valuable geologically because it allows the mineralogical composition to be estimated. Here, I/F is defined as the ratio of the radiance measured by CRISM to the solar irradiance at Mars divided by [pi]; if there was no martian atmosphere, I/F divided by the cosine of the incidence angle would be equal to the Lambert albedo for a Lambertian surface. After discussing the capabilities and limitations of the pipeline software system, we demonstrate its application on several multispectral data cubes--particularly, the outer reaches of the northern ice cap of Mars, the Tyrrhena Terra area that is northeast of the Hellas basin, and an area near the landing site for the Phoenix mission in the northern plains. For the icy spectra near the northern polar cap, aerosols need to be included in order to properly correct for the C[O.sub.2] absorption in the [H.sub.2]O ice bands at wavelengths near 2.0 [micro]m. In future phases of software development, we intend to use CRISM data directly in order to retrieve the spatiotemporal maps of aerosol optical depths, surface pressure, and surface temperature. This will allow a second level of refinement in the atmospheric and thermal correction of CRISM multispectral data. Index Terms--Atmospheric propagation, infrared spectroscopy, remote sensing, software verification and validation.

Published
2008

10. Extensive MRO CRISM Observations of 1.27 micron O2 Airglow in Mars Polar Night and Their Comparison to MRO MCS Temperature Profiles and LMD GCM Simulations

Author

Clancy, R. Todd, Sandor, Brad J, Wolff, Michael J, Smith, Michael Doyle, Lefevre, Franck, Madeleine, Jean-Baptiste, Forget, Francois, Murchie, Scott L, Seelos, Frank P, Seelos, Kim D, Nair, Hari A, Toigo, Anthony D, Humm, David, Kass, David M, Kleinbahl, Armin, and Heavens, Nicholas

Subjects
Lunar And Planetary Science And Exploration
Abstract

The Martian polar night distribution of 1.27 micron (0-0) band emission from O2 singlet delta [O2(1Delta(sub g))] is determined from an extensive set of Mars Reconnaissance Orbiter (MRO) Compact Reconnaissance Imaging Spectral Mapping (CRISM) limb scans observed over a wide range of Mars seasons, high latitudes, local times, and longitudes between 2009 and 2011. This polar nightglow reflects meridional transport and winter polar descent of atomic oxygen produced from CO2 photodissociation. A distinct peak in 1.27 micron nightglow appears prominently over 70-90NS latitudes at 40-60 km altitudes, as retrieved for over 100 vertical profiles of O2(1Delta(sub g)) 1.27 micron volume emission rates (VER). We also present the first detection of much (x80+/-20) weaker 1.58 micron (0-1) band emission from Mars O2(1Delta(sub g)). Co-located polar night CRISM O2(1Delta(sub g)) and Mars Climate Sounder (MCS) (McCleese et al., 2008) temperature profiles are compared to the same profiles as simulated by the Laboratoire de Météorologie Dynamique (LMD) general circulation/photochemical model (e.g., Lefèvre et al., 2004). Both standard and interactive aerosol LMD simulations (Madeleine et al., 2011a) underproduce CRISM O2(1Delta(sub g)) total emission rates by 40%, due to inadequate transport of atomic oxygen to the winter polar emission regions. Incorporation of interactive cloud radiative forcing on the global circulation leads to distinct but insufficient improvements in modeled polar O2(1Delta(sub g)) and temperatures. The observed and modeled anti-correlations between temperatures and 1.27 mm band VER reflect the temperature dependence of the rate coefficient for O2(1Delta(sub g)) formation, as provided in Roble (1995).

Published
2012
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11. Satellite sensor requirements for monitoring essential biodiversity variables of coastal ecosystems

Author

Muller-Karger, Frank E., Hestir, Erin, Ade, Christiana, Turpie, Kevin, Roberts, Dar A., Siegel, David A., Miller, Robert J., Humm, David, Izenberg, Noam, Keller, Mary, Morgan, Frank, Frouin, Robert, Dekker, Arnold G., Gardner, Royal, Goodman, James, Schaeffer, Blake, Franz, Bryan A., Pahlevan, Nima, Mannino, Antonio, Concha, Javier A., Ackleson, Steven G., Cavanaugh, Kyle C., Romanou, Anastasia, Tzortziou, Maria, Boss, Emmanuel S., Pavlick, Ryan, Freeman, Anthony, Rousseaux, Cecile S., Dunne, John P., Long, Matthew C., Salas, Eduardo Klein, McKinley, Galen A., Goes, Joachim I., Letelier, Ricardo M., Kavanaugh, Maria T., Roffer, Mitchell, Bracher, Astrid, Arrigo, Kevin R., Dierssen, Heidi M., Zhang, Xiaodong, Davis, Frank W., Best, Benjamin D., Guralnick, Robert P., Moisan, John R., Sosik, Heidi M., Kudela, Raphael M., Mouw, Colleen B., Barnard, Andrew H., Palacios, Sherry, Roesler, Collin S., Drakou, Evangelia G., Appeltans, Ward, Jetz, Walter, Muller-Karger, Frank E., Hestir, Erin, Ade, Christiana, Turpie, Kevin, Roberts, Dar A., Siegel, David A., Miller, Robert J., Humm, David, Izenberg, Noam, Keller, Mary, Morgan, Frank, Frouin, Robert, Dekker, Arnold G., Gardner, Royal, Goodman, James, Schaeffer, Blake, Franz, Bryan A., Pahlevan, Nima, Mannino, Antonio, Concha, Javier A., Ackleson, Steven G., Cavanaugh, Kyle C., Romanou, Anastasia, Tzortziou, Maria, Boss, Emmanuel S., Pavlick, Ryan, Freeman, Anthony, Rousseaux, Cecile S., Dunne, John P., Long, Matthew C., Salas, Eduardo Klein, McKinley, Galen A., Goes, Joachim I., Letelier, Ricardo M., Kavanaugh, Maria T., Roffer, Mitchell, Bracher, Astrid, Arrigo, Kevin R., Dierssen, Heidi M., Zhang, Xiaodong, Davis, Frank W., Best, Benjamin D., Guralnick, Robert P., Moisan, John R., Sosik, Heidi M., Kudela, Raphael M., Mouw, Colleen B., Barnard, Andrew H., Palacios, Sherry, Roesler, Collin S., Drakou, Evangelia G., Appeltans, Ward, and Jetz, Walter

Abstract

© The Author(s), 2018. This article is distributed under the terms of the Creative Commons Attribution License. The definitive version was published in Ecological Applications 28 (2018): 749-760, doi: 10.1002/eap.1682., The biodiversity and high productivity of coastal terrestrial and aquatic habitats are the foundation for important benefits to human societies around the world. These globally distributed habitats need frequent and broad systematic assessments, but field surveys only cover a small fraction of these areas. Satellite‐based sensors can repeatedly record the visible and near‐infrared reflectance spectra that contain the absorption, scattering, and fluorescence signatures of functional phytoplankton groups, colored dissolved matter, and particulate matter near the surface ocean, and of biologically structured habitats (floating and emergent vegetation, benthic habitats like coral, seagrass, and algae). These measures can be incorporated into Essential Biodiversity Variables (EBVs), including the distribution, abundance, and traits of groups of species populations, and used to evaluate habitat fragmentation. However, current and planned satellites are not designed to observe the EBVs that change rapidly with extreme tides, salinity, temperatures, storms, pollution, or physical habitat destruction over scales relevant to human activity. Making these observations requires a new generation of satellite sensors able to sample with these combined characteristics: (1) spatial resolution on the order of 30 to 100‐m pixels or smaller; (2) spectral resolution on the order of 5 nm in the visible and 10 nm in the short‐wave infrared spectrum (or at least two or more bands at 1,030, 1,240, 1,630, 2,125, and/or 2,260 nm) for atmospheric correction and aquatic and vegetation assessments; (3) radiometric quality with signal to noise ratios (SNR) above 800 (relative to signal levels typical of the open ocean), 14‐bit digitization, absolute radiometric calibration <2%, relative calibration of 0.2%, polarization sensitivity <1%, high radiometric stability and linearity, and operations designed to minimize sunglint; and (4) temporal resolution of hours to days. We refer to these combined s, National Center for Ecological Analysis and Synthesis (NCEAS); National Aeronautics and Space Administration (NASA) Grant Numbers: NNX16AQ34G, NNX14AR62A; National Ocean Partnership Program; NOAA US Integrated Ocean Observing System/IOOS Program Office; Bureau of Ocean and Energy Management Ecosystem Studies program (BOEM) Grant Number: MC15AC00006

Published
2018

13. A spaceborne visible-NIR hyperspectral imager for coastal phenology

Author

Osterman, Steven N., additional, Muller-Karger, Frank E., additional, Humm, David C., additional, Noble, Matthew W., additional, Begley, Shawn M., additional, Hersman, Christopher B., additional, Hestir, Erin L., additional, Izenberg, Noam, additional, Keller, Mary R., additional, Lees, Jeff, additional, Magruder, Adam S., additional, Morgan, Frank, additional, Seifert, Helmut, additional, and Strohbehn, Kim, additional

Published
2016
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14. Correction to 'Extensive MRO CRISM observations of 1.27 µm O2 airglow in Mars polar night and their comparison to MRO MCS temperature profiles and LMD GCM simulations'

Author

Clancy, R. Todd, Sandor, Brad J., Wolff, Michael J., Smith, Michael D., Lefèvre, Franck, Madeleine, Jean-Baptiste, Forget, François, Murchie, Scott L., Seelos, Frank, Seelos, Kim D., Nair, Hari A., Toigo, Anthony D., Humm, David, Kass, David M., Kleinböhl, Armin, Heavens, Nicholas, Space Science Institute [Boulder] (SSI), NASA Goddard Space Flight Center (GSFC), PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut Pierre-Simon-Laplace (IPSL), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Météorologie Dynamique (UMR 8539) (LMD), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-École des Ponts ParisTech (ENPC)-Centre National de la Recherche Scientifique (CNRS)-Département des Géosciences - ENS Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Université Pierre et Marie Curie - Paris 6 (UPMC), Johns Hopkins University Applied Physics Laboratory [Laurel, MD] (APL), Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), École normale supérieure - Paris (ENS Paris), Département des Géosciences - ENS Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS Paris), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École des Ponts ParisTech (ENPC)-École polytechnique (X)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)

Subjects
[PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2013
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15. Extensive MRO CRISM observations of 1.27 μm O2 airglow in Mars polar night and their comparison to MRO MCS temperature profiles and LMD GCM simulations

Author

Clancy, R. Todd, Sandor, Brad J., Wolff, Michael J., Smith, Michael D., Lefèvre, Franck, Madeleine, Jean-Baptiste, Forget, François, Murchie, Scott L., Seelos, Frank, Seelos, Kim D., Nair, Hari A., Toigo, Anthony D., Humm, David, Kass, David M., Kleinböhl, Armin, Heavens, Nicholas, Space Science Institute [Boulder] (SSI), NASA Goddard Space Flight Center (GSFC), PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut Pierre-Simon-Laplace (IPSL), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Météorologie Dynamique (UMR 8539) (LMD), Département des Géosciences - ENS Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École des Ponts ParisTech (ENPC)-École polytechnique (X)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Université Pierre et Marie Curie - Paris 6 (UPMC), Johns Hopkins University Applied Physics Laboratory [Laurel, MD] (APL), Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), École normale supérieure - Paris (ENS-PSL), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-École des Ponts ParisTech (ENPC)-Centre National de la Recherche Scientifique (CNRS)-Département des Géosciences - ENS Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS-PSL), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)

Subjects
Singlet delta, O2, Photochemistry, Atmosphere, [PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], Mars, Polar
Abstract

International audience; The Martian polar night distribution of 1.27 μm (0-0) band emission from O2 singlet delta [O2(1Δg)] is determined from an extensive set of Mars Reconnaissance Orbiter (MRO) Compact Reconnaissance Imaging Spectral Mapping (CRISM) limb scans observed over a wide range of Mars seasons, high latitudes, local times, and longitudes between 2009 and 2011. This polar nightglow reflects meridional transport and winter polar descent of atomic oxygen produced from CO2 photodissociation. A distinct peak in 1.27 μm nightglow appears prominently over 70-90NS latitudes at 40-60 km altitudes, as retrieved for over 100 vertical profiles of O2(1Δg) 1.27 μm volume emission rates (VER). We also present the first detection of much (x80±20) weaker 1.58 μm (0-1) band emission from Mars O2(1Δg). Co-located polar night CRISM O2(1Δg) and Mars Climate Sounder (MCS, McCleese et al, 2007) temperature profiles are compared to the same profiles as simulated by the Laboratoire de Meteorologie Dynamique (LMD) general circulation/photochemical model (e.g., Lefevre et al, 2004). Both standard and interactive aerosol LMD simulations (Madeleine et al, 2011) underproduce CRISM O2(1Δg) total emission rates by 40%, due to inadequate transport of atomic oxygen to the winter polar emission regions. Incorporation of interactive cloud radiative forcing on the global circulation leads to distinct but insufficient improvements in modeled polar O2(1Δg) and temperatures. The observed and modeled anti-correlations between temperatures and 1.27 μm band VER reflect the temperature dependence of the rate coefficient for O2(1Δg) formation, as provided in Roble (1995).

Published
2012
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17. Extensive MRO CRISM observations of 1.27 μm O2 airglow in Mars polar night and their comparison to MRO MCS temperature profiles and LMD GCM simulations

Author

Clancy, R. Todd, primary, Sandor, Brad J., additional, Wolff, Michael J., additional, Smith, Michael D., additional, Lefèvre, Franck, additional, Madeleine, Jean‐Baptiste, additional, Forget, Francois, additional, Murchie, Scott L., additional, Seelos, Frank P., additional, Seelos, Kim D., additional, Nair, Hari A., additional, Toigo, Anthony D., additional, Humm, David, additional, Kass, David M., additional, Kleinböhl, Armin, additional, and Heavens, Nicholas, additional

Published
2012
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18. Compact Reconnaissance Imaging Spectrometer for Mars investigation and data set from the Mars Reconnaissance Orbiter's primary science phase

Author

Murchie, Scott L., primary, Seelos, Frank P., additional, Hash, Christopher D., additional, Humm, David C., additional, Malaret, Erick, additional, McGovern, J. Andrew, additional, Choo, Teck H., additional, Seelos, Kimberly D., additional, Buczkowski, Debra L., additional, Morgan, M. Frank, additional, Barnouin-Jha, Olivier S., additional, Nair, Hari, additional, Taylor, Howard W., additional, Patterson, Gerald W., additional, Harvel, Christopher A., additional, Mustard, John F., additional, Arvidson, Raymond E., additional, McGuire, Patrick, additional, Smith, Michael D., additional, Wolff, Michael J., additional, Titus, Timothy N., additional, Bibring, Jean-Pierre, additional, and Poulet, Francois, additional

Published
2009
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20. GUVI: a hyperspectral imager for geospace

Author

Paxton, Larry J., primary, Christensen, Andrew B., additional, Morrison, Daniel, additional, Wolven, Brian, additional, Kil, Hyosub, additional, Zhang, Yongliang, additional, Ogorzalek, Bernard S., additional, Humm, David C., additional, Goldsten, John O., additional, DeMajistre, Robert, additional, and Meng, Ching-I., additional

Published
2004
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21. CRISM (Compact Reconnaissance Imaging Spectrometer for Mars) on MRO (Mars Reconnaissance Orbiter)

Author

Murchie, Scott L., primary, Arvidson, Raymond E., additional, Bedini, Peter, additional, Beisser, K., additional, Bibring, Jean-Pierre, additional, Bishop, J., additional, Boldt, John D., additional, Choo, Tech H., additional, Clancy, R. Todd, additional, Darlington, Edward H., additional, Des Marais, D., additional, Espiritu, R., additional, Fasold, Melissa J., additional, Fort, Dennis, additional, Green, Richard N., additional, Guinness, E., additional, Hayes, John R., additional, Hash, C., additional, Heffernan, Kevin J., additional, Hemmler, J., additional, Heyler, Gene A., additional, Humm, David C., additional, Hutchison, J., additional, Izenberg, Noam R., additional, Lee, Robert E., additional, Lees, Jeffrey J., additional, Lohr, David A., additional, Malaret, Erick R., additional, Martin, T., additional, Morris, Richard V., additional, Mustard, John F., additional, Rhodes, Edgar A., additional, Robinson, Mark S., additional, Roush, Ted L., additional, Schaefer, Edward D., additional, Seagrave, Gordon G., additional, Silverglate, Peter R., additional, Slavney, S., additional, Smith, Mark F., additional, Strohbehn, Kim, additional, Taylor, Howard W., additional, Thompson, Patrick L., additional, and Tossman, Barry E., additional

Published
2004
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22. STARS: STellar Absorption and Refraction Sensor

Author

Lloyd, Steven, primary, Yee, Jeng-Hwa, additional, Humm, David, additional, Murphy, Graham, additional, Morrison, Daniel, additional, Vervack, Ronald, additional, Carbary, James, additional, Paxton, Larry, additional, and Silverglate, Peter, additional

Published
2004
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23. The CONTOUR remote imager and spectrometer (CRISP)

Author

Warren, Jeffery W., primary, Heffernan, Kevin J., additional, Conard, Steven J., additional, Bell, James F., additional, Cochran, Anita L., additional, Boldt, John D., additional, Bowman, Alice F., additional, Darlington, E. H., additional, Deluzio, Anthony, additional, Fiore, Daniel, additional, Fort, Dennis E., additional, Garcia, David, additional, Grey, Matthew P., additional, Gotwols, Bruce L., additional, Harch, Ann P., additional, Hayes, John R., additional, Heyler, Gene A., additional, Howser, Linda M., additional, Humm, David C., additional, Izenberg, Noam R., additional, Kosakowski, Kris E., additional, Lees, W. J., additional, Lohr, D. A., additional, Luther, Holger M., additional, Mehoke, Douglas S., additional, Murchie, Scott L., additional, Reiter, R. Alan, additional, Rider, Brian, additional, Rogers, G. D., additional, Sampath, Deepak, additional, Schaefer, Edward D., additional, Spisz, Thomas S., additional, Strohbehn, Kim, additional, Svenson, Scott, additional, Taylor, Howard W., additional, Thompson, Patrick L., additional, Veverka, Joseph, additional, Williams, Robert L., additional, and Wilson, Paul, additional

Published
2004
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24. CONTOUR forward imager on the Comet Nucleus Tour mission

Author

Conard, Steven J., primary, Warren, Jeffery W., additional, Barnuoin-Jha, Olivier S., additional, Bell, James F., additional, Boldt, John D., additional, Bowman, Alice F., additional, Cochran, Anita L., additional, Darlington, E. H., additional, Deluzio, Anthony, additional, Fiore, Daniel, additional, Garcia, David, additional, Gotwols, Bruce L., additional, Grey, Matthew P., additional, Harch, Ann P., additional, Hayes, John R., additional, Heffernan, Kevin J., additional, Humm, David C., additional, Izenberg, Noam R., additional, Kosakowski, Kris E., additional, Luther, Holger M., additional, Mehoke, Douglas S., additional, Murchie, Scott L., additional, Prockter, Louise M., additional, Rider, Brian, additional, Sampath, Deepak, additional, Schaefer, Edward D., additional, Svenson, Scott, additional, Taylor, Howard W., additional, Thompson, Patrick L., additional, Veverka, Joseph, additional, Williams, Robert L., additional, and Wilson, Paul, additional

Published
2004
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25. Advanced time-of-flight system-on-a-chip for remote sensing instruments

Author

Paschalidis, Nicholas P., primary, Stamatopoulos, Nick, additional, Karadamoglou, Kosta, additional, Kottaras, George, additional, Paschalidis, Vasilis, additional, Sarris, Emmanuel, additional, Mitchell, Donald G., additional, Humm, David C., additional, Paxton, Larry J., additional, and McNutt, Jr., Ralph L., additional

Published
2003
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27. STARS: the Stellar Absorption and Refraction Sensor

Author

Yee, Jeng-Hwa, primary, Morrison, Daniel, additional, Murphy, Graham A., additional, Morgan III, M. F., additional, Humm, David C., additional, Silverglate, Peter R., additional, Vervack, Ronald, additional, and Paxton, Larry J., additional

Published
2002
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30. CONTOUR forward imager on the Comet Nucleus Tour mission.

Author

Conard, Steven J., Warren, Jeffery W., Barnuoin-Jha, Olivier S., Bell, James F., Boldt, John D., Bowman, Alice F., Cochran, Anita L., Darlington, E. H., Deluzio, Anthony, Fiore, Daniel, Garcia, David, Gotwols, Bruce L., Grey, Matthew P., Harch, Ann P., Hayes, John R., Heffernan, Kevin J., Humm, David C., Izenberg, Noam R., Kosakowski, Kris E., and Luther, Holger M.

Published
2004
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31. The CONTOUR remote imager and spectrometer (CRISP).

Author

Warren, Jeffery W., Heffernan, Kevin J., Conard, Steven J., Bell, James F., Cochran, Anita L., Boldt, John D., Bowman, Alice F., Darlington, E. H., Deluzio, Anthony, Fiore, Daniel, Fort, Dennis E., Garcia, David, Grey, Matthew P., Gotwols, Bruce L., Harch, Ann P., Hayes, John R., Heyler, Gene A., Howser, Linda M., Humm, David C., and Izenberg, Noam R.

Published
2004
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32. Compact reconnaissance imaging spectrometer for Mars (CRISM): characterization results for instrument and focal plane subsystems.

Author

Silverglate, Peter R., Heffernan, Kevin J., Bedini, Peter D., Boldt, John D., Cavender, Peter J., Choo, Tech H., Darlington, Edward H., Donald, Erik T., Fasold, Melissa J., Fort, Dennis E., Gurnee, Reid S., Hayes, Allen T., Hayes, John R., Hemler, James B., Humm, David C., Izenberg, Noam R., Lee, Robert E., Lees, William J., Lohr, David A., and Murchie, Scott L.

Published
2004
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35. A spaceborne visible-NIR hyperspectral imager for coastal phenology

Author

Meynart, Roland, Neeck, Steven P., Kimura, Toshiyoshi, Shimoda, Haruhisa, Osterman, Steven N., Muller-Karger, Frank E., Humm, David C., Noble, Matthew W., Begley, Shawn M., Hersman, Christopher B., Hestir, Erin L., Izenberg, Noam, Keller, Mary R., Lees, Jeff, Magruder, Adam S., Morgan, Frank, Seifert, Helmut, and Strohbehn, Kim

Published
2016
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37. SCHOONERS: absorption and refraction of starlight from space for atmospheric profiles

Author

Humm, David C., primary, Murphy, Graham A., additional, Yee, Jeng-Hwa, additional, Morrison, Daniel, additional, Morgan III, M. F., additional, Heyler, Gene A., additional, Shapiro, H. S., additional, Wilson, D. S., additional, Peacock, Keith, additional, Lees, W. J., additional, Persons, David F., additional, Heffernan, Kevin J., additional, and Pardoe, C. T., additional

Published
2000
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39. Global ultraviolet imager (GUVI): measuring composition and energy inputs for the NASA Thermosphere Ionosphere Mesosphere Energetics and Dynamics (TIMED) mission

Author

Paxton, Larry J., primary, Christensen, Andrew B., additional, Humm, David C., additional, Ogorzalek, Bernard S., additional, Pardoe, C. T., additional, Morrison, Daniel, additional, Weiss, Michele B., additional, Crain, W., additional, Lew, Patricia H., additional, Mabry, Dan J., additional, Goldsten, John O., additional, Gary, Stephen A., additional, Persons, David F., additional, Harold, Mark J., additional, Alvarez, E. Brian, additional, Ercol, Carl J., additional, Strickland, Douglas J., additional, and Meng, Ching-I., additional

Published
1999
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41. Total Photoabsorption Cross Section of Molecular Nitrogen Near 83.4 nm

Author

Naval Postgraduate School (U.S.), Physics, Morgan, Harry D., Seyoum, Hailemichael M., Fortna, J.D.E., Humm, David C., Asfaw, Araya, Cleary, David D., Naval Postgraduate School (U.S.), Physics, Morgan, Harry D., Seyoum, Hailemichael M., Fortna, J.D.E., Humm, David C., Asfaw, Araya, and Cleary, David D.

Abstract

The photoabsorption cross section of molecular nitrogen near 83.4 nm has been measured at room temperature. The cross sections at the wavelengths of the 2s2p 4 4p•, 4P3/2, and 4P 1/2 (all - 2s22p3 4S0 3/2) O* emission lines are measured to be 10.1 + 1.6 Mb, 0.29 _+ 0.02 Mb, and 0.049 _+ 0.008 Mb respectively. These measurements were made with an O'emission discharge source, and repeated using a synchrotron radiation source. Both measurements were made with the 0.008-nm resolution 6.65-m spectrometer at the SURF lI storage ring of the National Institute for Standards and Technology.

Published
1993

42. Design and performance of the Global Ultraviolet Imager (GUVI)

Author

Humm, David C., primary, Paxton, Larry J., additional, Christensen, Andrew B., additional, Ogorzalek, Bernard S., additional, Pardoe, C. T., additional, Meng, Ching-I., additional, Morrison, Daniel, additional, Strickland, Douglas J., additional, Evans, J. S., additional, Weiss, Michele B., additional, Crain, W., additional, Lew, Patricia H., additional, Mabry, Dan J., additional, Goldsten, John O., additional, Gary, Stephen A., additional, Peacock, Keith, additional, Persons, David F., additional, Harold, Mark J., additional, Alvarez, E. Brian, additional, and Ercol, Carl J., additional

Published
1998
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49. Design and performance of the Global Ultraviolet Imager (GUVI).

Author

Humm, David C., Paxton, Larry J., Christensen, Andrew B., Ogorzalek, Bernard S., Pardoe, C. T., Meng, Ching-I., Morrison, Daniel, Strickland, Douglas J., Evans, J. S., Weiss, Michele B., Crain, W., Lew, Patricia H., Mabry, Dan J., Goldsten, John O., Gary, Stephen A., Peacock, Keith, Persons, David F., Harold, Mark J., Alvarez, E. Brian, and Ercol, Carl J.

Published
1998
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