Comparative analysis of GOCI ocean color products

by on 22 August 2016in Earth Science and Remote Sensing No comment

The Geostationary Ocean Color Imager (GOCI) is the first geostationary ocean color sensor in orbit that provides bio-optical properties from coastal and open waters around the Korean Peninsula at unprecedented temporal resolution. In this study, we compare the normalized water-leaving radiance (nLw) products generated by the Naval Research Laboratory Automated Processing System (APS) with those produced by the stand-alone software package, the GOCI Data Processing System (GDPS), developed by the Korean Ocean Research & Development Institute (KORDI). Both results are then compared to the nLw measured by the above water radiometer at the Ieodo site. This above-water radiometer is part of the Aerosol Robotic NETwork (AeroNET). The results indicate that the APS and GDPS processed correlates well within the same image slot where the coefficient of determination (r(2)) is higher than 0.84 for all the bands from 412 nm to 745 nm. The agreement between APS and the AeroNET data is higher when compared to the GDPS results. The Root-Mean-Squared-Error (RMSE) between AeroNET and APS data ranges from 0.24 [mW/(cm(2)srmum)] at 555 nm to 0.52 [mW/(cm(2)srmum)] at 412 nm while RMSE between AeroNET and GDPS data ranges from 0.47 [mW/(cm(2)srmum)] at 443 nm to 0.69 [mW/(cm(2)srmum)] at 490 nm.

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http://www.ncbi.nlm.nih.gov/pubmed/26473861

Occurrence and Spatial Extent of HABs on the West Florida Shelf 2002 – Present

by on 22 August 2016in Earth Science and Remote Sensing No comment

Harmful algal blooms (HABs) can lead to severe economic and ecological impacts in coastal areas and can threaten marine life and human health. About three quarters of these toxic blooms are caused by dinoflagellate species. One dinoflagellate species, i.e., Karenia brevis, blooms nearly every year in the Gulf of Mexico, particularly on the West Florida Shelf (WFS), where these blooms cause millions of dollars in socioeconomic damage. In this letter, we use the red band difference (RBD) bloom detection tech- nique for detection of low backscattering phytoplankton blooms, such as K. brevis, and conduct time-series analyses of the spatial extent of these blooms using Moderate Resolution Imaging Spec- troradiometer (MODIS) monthly mean data spanning July 2002 (sensor inception) to September 2014. The time-series results show that the RBD successfully detects the documented HABs in the region, illustrating the seasonal and interannual variability, in- cluding the extensive blooms of 2005 and 2014.

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http://ieeexplore.ieee.org/xpl/articleDetails.jsp?reload=true&arnumber=7160674

Hourly turbidity monitoring using Geostationary Ocean Color Imager fluorescence bands

by on 22 August 2016in Earth Science and Remote Sensing No comment

TheGeostationaryOceanColorimager(GOCI)isthefirstgeostationaryoceancolor satellite sensor that collects hourly images eight times per day during daylight. This high fre- quency image acquisition makes it possible to study more detailed dynamics of red tide blooms, sediment plumes, and colored dissolved organic matter plumes, and can aid in the prediction of biophysical phenomena. We apply the red band difference and the fluorescence line height algo- rithms to GOCI imagery to separate waters with high algal and nonalgal particles and validate the results with the MODIS imagery. We also track optical features using hourly GOCI imagery and assess their movement through comparisons with predicted ocean currents derived from the navy coastal ocean model and tidal data.

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http://remotesensing.spiedigitallibrary.org/article.aspx?articleid=2424313

Preservation of Biomarkers from Cyanobacteria Mixed with Mars-Like Regolith Under Simulated Martian Atmosphere and UV Flux

by on 22 August 2016in Biology & Biotechnology, Earth Science and Remote Sensing No comment

The space mission EXPOSE-R2 launched on the 24th of July 2014 to the International Space Station is carrying the BIOMEX (BIOlogy and Mars EXperiment) experiment aimed at investigating the endurance of extremophiles and stability of biomolecules under space and Mars-like conditions. In order to prepare the analyses of the returned samples, ground-based simulations were carried out in Planetary and Space Simulation facilities. During the ground-based simulations, Chroococcidiopsis cells mixed with two Martian mineral analogues (phyllosilicatic and sulfatic Mars regolith simulants) were exposed to a Martian simulated atmosphere combined or not with UV irradiation corresponding to the dose received during a 1-year-exposure in low Earth orbit (or half a Martian year on Mars). Cell survival and preservation of potential biomarkers such as photosynthetic and photoprotective pigments or DNA were assessed by colony forming ability assays, confocal laser scanning microscopy, Raman spectroscopy and PCR-based assays. DNA and photoprotective pigments (carotenoids) were detectable after simulations of the space mission (570 MJ/m(2) of UV 200-400 nm irradiation and Martian simulated atmosphere), even though signals were attenuated by the treatment. The fluorescence signal from photosynthetic pigments was differently preserved after UV irradiation, depending on the thickness of the samples. UV irradiation caused a high background fluorescence of the Martian mineral analogues, as revealed by Raman spectroscopy. Further investigation will be needed to ensure unambiguous identification and operations of future Mars missions. However, a 3-month exposure to a Martian simulated atmosphere showed no significant damaging effect on the tested cyanobacterial biosignatures, pointing out the relevance of the latter for future investigations after the EXPOSE-R2 mission. Data gathered during the ground-based simulations will contribute to interpret results from space experiments and guide our search for life on Mars.

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http://www.ncbi.nlm.nih.gov/pubmed/26530341

Combined Spectral and Timing Analysis of the Black Hole Candidate MAXI J1659−152, Discovered by MAXI and Swift

by on 9 June 2015in Earth Science and Remote Sensing No comment

We report on X-ray spectral and timing results of a new black hole candidate (BHC), MAXI J1659−152, with an orbital period of 2.41 hr (shortest among BHCs) in a 2010 outburst from 65 Rossi X-ray Timing Explorer (RXTE) observations and 8 simultaneous Swift and RXTE observations. According to the definitions of the spectral states in Remillard and McClintock (2006, ARA&A, 44, 49), most of the observations have been classified into the intermediate state. All of the X-ray broadband spectra can be modeled by a multi-color disk plus a power-law with an exponential cutoff or a multi-color disk plus a Comptonization component. During the initial phase of the outburst, a high-energy cutoff was visible at 30–40 keV. The innermost radius of the disk gradually decreased by a factor of more than 3 from the onset of the outburst, and reached a constant value of 35 d10cos i−1/2 km, where d10 is the distance in units of 10 kpc and i is the inclination. The type-C quasi-periodic oscillation (QPO) frequency varied from 1.6 Hz to 7.3 Hz in association with a change of the innermost radius, while the innermost radius remained constant during the type-B QPO detections at 1.6–4.1 Hz. Hence, we suggest that the origin of the type-B QPOs is different from that of type-C QPOs, the latter of which would originate from the disk truncation radius. Assuming the constant innermost radius in the latter phase of the outburst as the innermost stable circular orbit, the black hole mass in MAXI J1659−152 is estimated to be 3.6–8.0 M⊙ for a distance of 5.3–8.6 kpc and an inclination angle of 60∘–75∘.

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http://pasj.oxfordjournals.org/content/64/2/32.abstract

Imaging Observation of the Earth's Plasmasphere and Ionosphere by EUVI of ISS-IMAP on the International Space Station

by on 9 June 2015in Earth Science and Remote Sensing No comment

At the end of previous century, we succeeded to image the Earth's plasmasphere from the space by EUV spectral range. Then, spacecraft missions were carried out to image the terrestrial EUV emissions. The extreme ultraviolet imagers (EUVIs) on the international space station (ISS) will be launched in 2012. At the altitude of approximately 400 km, two telescopes direct toward the Earth's limb to look the ionosphere and plasmasphere from the inside-out. One telescope detects the terrestrial EUV emission at O+ (83.4 nm), and the other is He+ (30.4 nm). These two EUV emissions are solar-scattered by ionized oxygen and helium, respectively. The maximum spatial and time resolutions are 0.1 degree and 1 minute, respectively. Our observation methods will become standard to probe the Earth's upper atmosphere.

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Verification of pointing and antenna pattern knowledge of Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES)

by on 9 June 2015in Earth Science and Remote Sensing No comment

The Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) observes 03 and other minor chemical species in the stratosphere and mesosphere. Limb observation of SMILES is sensitive to the quality of the tangent altitude retrieval. To obtain better retrieval result, knowledge of initial tangent height and antenna pattern should be as precise and accurate as possible. It was concluded that initial tangent height is calculated by using ISS attitude and mirror pointing angle, and ISS position. Antenna pattern assuming 6 points moving average was applied to the retrieval and showed reasonable results.

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The spectral reflectance of ship wakes between 400 and 900 nanometers

by on 9 June 2015in Earth Science and Remote Sensing No comment

This technical note describes the use of an airborne hyperspectral imaging sensor (HICO – Hyperspectral Imager of the Coastal Ocean) to record the spectral reflectance characteristics of centerline ship wakes in the 400 to 900 nm wavelength region. Data were collected for a target of known provenance (the United States Coast Guard Cutter Kittiwake) off the Wai'anae coast of O'ahu, Hawai'i, on 8 April 2010. HICO acquired data in 60 spectral bands by flying along the long axis of the wake while the vessel travelled at three speeds (~3.6 m s<sup>-1</sup> or 7 knots; ~7.2 m s<sup>-1</sup> or 14 knots; and ~11.2 m s<sup>-1</sup> or 21 knots). A flying altitude of ~1500 m yielded a spatial resolution of ~1.5 m. Spectral profiles along and across the wake axes are presented which show how the spectral reflectance of the centerline wake varies spatially and temporally as a function of vessel speed. Length (and to a lesser extent, width) vary in proportion to speed. In common with previous studies and model predictions, the wakes show a pronounced greening of the wake (i.e. enhanced reflectance at ~550 nm), with evidence for elevated reflectance at 750-800 nm. Resampling the data from its raw 1.5 m spatial resolution yields insights into how the turbulent wake becomes spectrally inseparable from the background water as spatial resolution decreases (i.e. becomes increasingly coarse). Using a simple statistical test, the wake becomes spectrally similar to the background ocean as the resolution approaches 60 m.

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Gas Slit Camera (GSC) onboard MAXI on ISS

by on 9 June 2015in Earth Science and Remote Sensing No comment

The Gas Slit Camera (GSC) is an X-ray instrument on the MAXI (Monitor of All-sky X-ray Image) mission on the International Space Station. It is designed to scan the entire sky every 92-minute orbital period in the 2–30 keV band and to achieve the highest sensitivity among the X-ray all-sky monitors ever flown so far. The GSC employs large-area position-sensitive proportional counters with the total detector area of 5350 cm$^2$. The on-board data processor has functions to format telemetry data as well as to control the high voltage of the proportional counters to protect them from the particle irradiation. The paper describes the instruments, on-board data processing, telemetry data formats, and performance specifications expected from the ground calibration tests.

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Discovery of a Cyclotron Resonance Feature in the X-ray Spectrum of GX 304-1 with RXTE and Suzaku during Outbursts Detected by MAXI in 2010

by on 9 June 2015in Earth Science and Remote Sensing No comment

We report the discovery of a cyclotron resonance scattering feature (CRSF) in the X-ray spectrum of GX 304-1, obtained by RXTE and Suzaku during major outbursts detected by MAXI in 2010. The peak intensity in August reached 600 mCrab in the 2-20 keV band, which is the highest ever observed from this source. The RXTE observations on more than twenty occasions and one Suzaku observation revealed a spectral absorption feature at around 54 keV, which is the first CRSF detection from this source. The estimated strength of surface magnetic field, 4.7×1012 G, is one of the highest among binary X-ray pulsars from which CRSFs have ever been detected. The RXTE spectra taken during the August outburst also suggest that the CRSF energy changed over 50-54 keV, possibly in a positive correlation with the X-ray flux. The behavior is qualitatively similar to that observed from Her X-1 on long time scales, or from A 0535+26, but different from the negative correlation observed from 4U 0115+63 and X 0331+53.

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