Exhibitors②
NEUTRINO TOKYO INC.
NEUTRINO TOKYO INC.
Cambridge Univ Pr, Elsevier, Springer, Taylor & Francis, Wiley, Geological Society of London などの地球科学関連洋書を紹介・販売いたします。通常よりもお得な学会特別価格でご提供いたします。
割引適用期間：2021年5月28日（金）～2021年7月9日（金）まで
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◆JpGU 2021: Online 最大20％引にて販売！！
学術洋書販売のニュートリノ東京です。今回もオンライン開催となってしまい残念ですが、今回も地球科学関連洋書を割引価格で販売いたします。通常の価格から、10～20%OFFで販売いたしますので、大変お買い求め安くなっております。また、合計4,500円以上のお買い上げで送料無料となります。
◆展示リスト・注文書
展示リスト（PDF）展示リストデータ（Excel）
注文書（PDF）
注文書（Word）
注文用メールフォーム
※自由にダウンロードしてご利用いただいて構いませんが、
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◆注目の新刊・おすすめ書籍 随時更新!!
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この他にも多数の書籍を割引価格で販売いたしております。
展示リスト・分野別リンクからご確認ください。
◆分野別ページへのリンク
・Earth and Planetary Science, Textbook・Atmospheric Science, Climate Change
・Geology, Geomorphology, Geography
・Geophysics, Seismology, Numerical Analysis
・Geochemistry, Mineralogy, Petrology, Volcanology
・Environmental Science, Groundwater, Soil Science, Hydrology
◆ご購入・お支払い方法について
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・その他ご不明な点があれば、お気軽にお問い合わせください。
| Address | 182-0024 Takahashi Bldg., 1-44-3 Fuda, Chofu-shi, Tokyo 182-0024 Japan |
|---|---|
| TEL | 042-484-5550 |
| FAX | 042-484-5556 |
| Web site, SNS | https://neutrino.shop-pro.jp/ |
DARTS: Space Science Data Archive (ISAS/JAXA)
DARTS: Space Science Data Archive (ISAS/JAXA)
What is DARTS?
DARTS(Data ARchives and Transmission System) primarily archives high-level data products obtained by JAXA's space science missions in lunar and planetary science, solar-terrestrial physics, solar physics, and astrophysics. In addition, we provide data services to facilitate use of these data.
What kind of data is published in DARTS?
DARTS publishes data on more than 30 space science missions, as shown in the figure below.
【Lunar and planetary science】
Observation data of Hayabusa2, Hayabusa, Kaguya(SELENE), Akatsuki, etc are available on DARTS. In addition, the planetary seismic data from Apollo and Viking2 can also be obtained.
Image taken by SELENE (KAGUYA) High Definition Television (HDTV).
【Solar-terrestrial physics】
At DARTS, you can download observation data from Arase, JEM-GLIMS, SMILES, Reimei, Geotail, Akebono, etc. are released.
The time history of the splite image taken by JEM-GLIMS.
【Solar physics】
Solar observational data by Hinode, Yohkoh, and Hinotori are available. From June 2020, the "Yohkoh Legacy Data Archive", which was prepared at the University of Montana, has also been released.
A series of soft X-ray images of the sun from 1991 to 1999 obtaind by Yohkoh. You can see the sun changes its appearance from the maximum to the minimum and vice versa.
Let's use DARTS application tools!
DARTS provides various application tools. Please try it.(For reference) List of our web apps.
FLOW on the Web
Users can view simulated field of view image of exploration satellites such as Hayabusa or Akatsuki with our "FLOW on the Web".
Simulation result by FieLd Of View Visualizer (FLOW). The figure on the left shows the simulation results of Kaguya HDTV, and the figure on the right shows the results of ROSETTA OSIRIS.
JUDO2
By using JUDO2 (JAXA Universe Data Oriented Gen2) web tool, you can compare various sky-images in various wavelengthes including constellation lines or images.
Let's talk with DARTS members.
If you have any questions about DARTS,Please access CHAT and/or the zoom below.
List of Core Times:
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| Web site, SNS | https://darts.isas.jaxa.jp/index.html.en |
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European Geosciences Union (EGU)
European Geosciences Union (EGU)
The European Geosciences Union (EGU) is the leading organisation for Earth, planetary and space science research in Europe. EGU publishes a number of diverse scientific journals and its annual General Assembly is the largest European geosciences event.
Download the material
E-mail: info@egu.eu
| Address | 81677 Munich, Germany |
|---|---|
| TEL | +49-89-2050 76300 |
| FAX | +49-89-2050 76399 |
| Web site, SNS | https://www.egu.eu/ |
NAOJ TMT Project
NAOJ TMT Project
Contents
Thirty Meter TelescopeIn Search for Life on Extrasolar Planets
Our Solar System
Science Teams
Maunakea and TMT
Thirty Meter Telescope
TMT is an ambitious project with plans to construct on Hawaiʻi an extremely large telescope with an aperture of 30m with the cooperation of five countries including Japan. The major goals of TMT include search for signatures of life on extrasolar planets and the history of our solar system.◆TMT Overview
・Aperture：30 meters / 492 segment mirrors
・Wavelength range：0.31-28μｍ
・Diffraction limit：8miliarcsec （at 1μｍ）
・Sensitivity：More than 100 times better than conventional telescopes
(when observing a point light source with adaptive optics)
English Brochure (PDF, 2MB)
In Search for Life on Extrasolar Planets
◆Direct observations of Earth-like planetsMany planetary systems around stars other than our Sun are being discovered today, and we are learning that there exist planets with various sizes and orbits. Recently, planets similar in size as Earth have been discovered, indicating that there are planetary systems much like our own Solar Sytem. Today, infrared observation has advanced to a point of being able to actually capture images of these planets.
Three Jupiter-like planets around HR8799 discovered by the Subaru Telescope (in red circle). TMT will attempt to directly capture even smaller Earth-like planets. (Credit: CHARIS Team of Princeton University, and NAOJ)
◆Are we alone?
Are there extrasolar planets with existence of life? This is a question common to all humanity. TMT aims to discover signs of life on these planets.
TMT will be able to study the composition of the atmosphere of extrasolar planets through spectroscopic observation. Discovery of oxygen molecules and organic substances could be a signature of existence of extra-terrestrial life.
Exoplanets with TMT (TIO website)
Our Solar System
The advent of TMT will enable us to tackle long-standing questions concerning the formation of the solar system, the origin of planetary volatiles, the physics of the ice and gas giants, and the unraveling of the complex dynamical history recorded in the Kuiper belt.
The view of Jupiter's moon Io when observed using adaptive optics. The image on the left is a simulation of a conventional telescope with an aperture of 8 to 10 meters, and the image in the center is a simulation of TMT. The image on the right is the actual image taken by the Galileo spacecraft (Credit: T. Do/UCLA/IRIS)
Simulation of Pluto and its satellite Charon observed with TMT using adaptive optics (Credit: IRIS/TMT/G. Walth)
Our Solar System with TMT (TIO website)
Science Teams
The TMT International Science Development Teams (ISDTs) are groups of researchers who work together to provide scientific guidance and feedback to the TMT project, to stimulate planning for future TMT observing programs, and to build connections between the TMT and the international astronomical communities. The ISDTs foster scientific collaboration across the TMT partnership and beyond, into the broader astronomical community. Prospective applicants are encouraged to contact the conveners to learn more about the ISDTs and their activities.ISDTs (TIO website)
Maunakea and TMT
TMT is planned to be built on Maunakea, Hawaiʻi. Maunakea is a 4000-m mountain with gently inclined slopes, isolated in the mid-Pacific Ocean from any other land mass, which makes the mountain one of the exceptionally well-endowed sites for astronomical observations in the world. Maunakea is also a sacred place for the people of Hawaiʻi, connecting them to their kūpuna (ancestors) and akua (gods). It represents a symbol of the Hawaiʻi culture deeply rooted in nature. We are committed to the TMT Project without impeding traditional and customary cultural practices of Hawaiʻi.
| Address | 181-8588 2-21-1 Osawa, Mitaka, Tokyo 181-8588, JAPAN |
|---|---|
| Web site, SNS | https://www.nao.ac.jp/en/research/project/tmt.html |
Oxford Instruments KK
Oxford Instruments KK
◆Providing leading-edge tools
Oxford Instruments NanoAnalysis provides leading-edge tools that enable materials characterisation and sample manipulation at the nanometre scale. Used on electron microscopes (SEM and TEM) and ion-beam systems (FIB), our tools are used for R&D across a wide range of academic and industrial applications including semiconductor, renewable energy, mining, metallurgy and forensics.◆Exhibitors' Seminar 2021 4th June Fri. 11:30-12:15 JST Ch.17
Quantitative EDS Explained ‐ For reliable quantitative analysis
Energy dispersive X-ray spectrometry (EDS) provides elemental information in seconds. In this talk, the EDS spectral processing and quantification method will be explained based on AZtecLive system. Upgrade your EDS operating skills and knowledge to the "Master Class".
◆Products
◆ AZtecLive Energy Dispersive Spectroscopy(EDS)
AZtecLive is a revolutionary new approach to EDS analysis that enables a radical change in the way users perform sample investigation in the SEM. It combines a live electron image with live X-ray chemical imaging to give an intuitive new way of interacting with your samples.See More
◆ AZtecWave Wavelength Dispersive Spectroscopy(WDS)
AZtecWave combines the unique power of WDS to resolve X-ray peaks and quantify minor and trace elements with the speed and flexibility of EDS. EDS and WDS Wave Spectrometer operation is fully integrated into the AZtec software, guaranteeing maximum accessibility to users with all levels of expertise and Tru-Q® processing technology for the most accurate results. When microanalysis is at its most challenging, AZtecWave provides accurate answers, fast.See More
◆ AZtecHKL Electron Backscatter Diffraction(EBSD)
The most powerful EBSD software available, AZtecHKL combines speed and accuracy of results for routine analysis, with the flexibility and power required for applications that push the frontiers of EBSD. See More
◆What's New 
The powerful, automated, Mineral Liberation Analysis solution. It enables ore characterisation, provides vital data on metal recovery and enables process yield characterisation using multipurpose SEMs. It is also a valuable tool for the characterisation of rocks in research environments, enabling the automation of otherwise laborious optical analyses. Exploiting the performance of up to 4 of Oxford Instruments’ large area SDDs (Ultim Max), it provides accurate classification of minerals at speeds comparable to dedicated systems – but with the flexibility to perform other investigations as required. See More
・Application Note
Fast Characterisation of Minerals with Similar Crystal Structures
◆Applications
Application Library
To find application notes in geology, click here
Blogs
Scientific blogs to educate and entertain. Enjoy Oxford Instruments blogs here
◆Contact Us
On Line①31st May Mon.13:00-14:00 JST
②4th June Fri.14:00-15:00 JST
Join online meeting（MicrosoftTeams(R) will start）
Send mail
◆About Us
| Address | 140-0002 IS Building, 3-32-42, Higashishinagawa, Shinagawa-ku, Tokyo 140-0002 |
|---|---|
| TEL | 03-6732-8967 |
| FAX | 03-6732-8939 |
| Web site, SNS | https://nano.oxinst.com/ |
HARADA CORPORATION
HARADA CORPORATION
◆見出し①
発展し続ける通信インフラの現場作業効率化のパートナーとして、各種測定器や海底ケーブルの防護システムを取り扱っています。また、次世代高速無線通信「5G」関連商材の開発にも積極的に取り組んでいます。
今回は、海底ケーブル上の地震観測用DAS装置を出展させて頂きます。
◆見出し②
内容
資料を表示する
◆見出し③
◆見出し④
DAS装置のご購入を検討される際には、是非ご連絡ください。
また、DAS装置のレンタル相談にもお気軽にお問い合わせください。
| Address | 1000005 2-1, Marunouchi 1-chome, Chiyoda-ku, Tokyo |
|---|---|
| TEL | 0332128391 |
| FAX | 0333138399 |
| Web site, SNS | https://www.haradacorp.co.jp/en/ |
ISEE, Nagoya University
ISEE, Nagoya University
What is the Institute for Space-Earth Environmental Research (ISEE)?
The mission of ISEE is to clarify the mechanisms and relationships between the Earth, the Sun, and cosmic space, treating them as a seamless system, and to contribute to solving issues related to the global environment and human society spreading in space. In addition, ISEE plays a role as the only joint usage/research center linking space science and earth science, and promotes various collaborative research projects.Our environment comprises various interacting elements and evolves with time. In particular, the dynamics of solar activity sometimes have a great influence on the global environment and human society. A huge solar flare explosion occurring on the solar surface severely disturbs the Earth's magnetic field, the atmosphere, and the radiation environment, and it may cause serious impacts on satellites, electric power, communications, aviation, and other infrastructure. Long-term variation in sunspot activity may also affect the global climate. Cosmic rays arriving from far away in the universe are also an element of our environment, and the cosmogenic isotopes in tree rings provide us with valuable information to explore past environments. On the other hand, it is important to understand the mechanisms of climate change and extreme weather phenomena, both of which may cause disasters. For this purpose, it is necessary to clarify not only the greenhouse effect but also the hydrological circulation, in which aerosols, clouds, and precipitation interact, as well as the interaction between meteorological dynamics and the land–ocean ecosystem with solar influence.
In order to explore the space–earth environment, interdisciplinary research across different fields is necessary. ISEE aims to play a role in promoting domestic and international research collaboration between researchers, and to develop a new discipline of space–earth environmental research. We look forward to your continued support and cooperation.
Education at ISEE
ISEE offers primarily graduate programs (Graduate School of Science, Graduate School of Engineering, and Graduate School of Environmental Studies in Nagoya University), but also provides opportunities for both undergraduate and postdoctoral study.link to Education page at ISEE HP
Outreach activities at ISEE
For purposes of science education, ISEE publishes booklets on many topics in space science. These publications include comic books written by the popular cartoonist "Hayanon," featuring humorous characters and explaining scientific themes in a friendly way. The booklets are suitable for the general public as well as for school children. ISEE publishes these booklets in collaboration with SCOSTEP. These booklets can be downloaded at the following site.link to Outreach page at ISEE HP
ISEE Introduction Movie with English Subtitles
| Address | 464-8601 Furo-cho, Chikusa-ku, Nagoya, Aichi |
|---|---|
| Web site, SNS | https://www.isee.nagoya-u.ac.jp/en/index.html |
OYO Corporation
OYO Corporation
We, OYO Corporation, are a group of experts with extensive knowledge and abundant experiences in overall earth sciences such as geology, geophysics,soil mechanics, civil engineering, hydraulics, environmental engineering, ecology.
Making full use of our expertise knowledges and technologies related to earth science, we investigate the actual conditions of natural phenomena and disasters and the characteristics of the earth and underground water,
predict and evaluate the impact on business and society, and make optimal proposals for solving various challenges related to earth science.
◆Instruments and Technologies of OYO Corporation◆
We introduce our Instruments and Technologies for the purpose of visualizing geological structure in 3D model. Instruments
McOHM Profiler-8i McSEIS-AT UtilityScan 
Resistivity Image Passive wave survey Compct GPR System
Profiling
Product
details Product
details Product
details
3D Technology
Product3D Exploration Center
Contribute to the development of 3D exploration technology for underground.
Title: [HTT17-08] Towing Electrical Exploration using “Plate Electrode Capacitively Coupled Resistivity Survey
◆Session◆
Name: [HTT17] New Challenge with shallow geophysical exploration.Title: [HTT17-08] Towing Electrical Exploration using “Plate Electrode Capacitively Coupled Resistivity Survey
◆
| Address | 101-8486 7 Kanda-Mitoshiro-cho, Chiyoda-ku, Tokyo 101-8486, Japan |
|---|---|
| TEL | 03-5577-4501 |
| Web site, SNS | https://www.oyo.co.jp/english/ |
Paleo Labo co.,ltd.
Paleo Labo co.,ltd.
Business details
Paleo Lab conducts scientific analysis of artifacts and sediment samples obtained from archaeological sites. Our company handles everything from boring core drilling and sampling to analyses including radiocarbon dating, microfossil analysis (pollen, phytolith and diatom), plant macrofossil analysis, wood identification, faunal analysis, tephra identification, etc. 
Company Brochure
Download Company Brochure 30秒CM
Radiocarbon dating for small-scale samples
Small scale samples (~0.1mg) can also be dated using radiocarbon dating. Please contact us for more information.
Radiocarbon Dating Academic Price
Discount is available for universities, research institutes, or other academic research groups (students included). Please download the pamphlet below for details.Download Pamphlet
Research grant for young researchers
1. Support detailsa. ¥300,000 research grant
b. 10 radiocarbon dating samples for free
Acceptable period: September 1, 2021 to October 31, 2021 and April 1, 2022 to August 31, 2022
2. Submission deadline
July 31, 2021 (must arrive)
Please contact us for further information: jyosei@paleolabo.jp
Remote consultation on Zoom
a. June 3 13:00-17:00b. June 4 13:00-17:00
c. June 5 13:00-17:00
Remote consultation on Zoom
| Address | 335-0016 1-13-22, Shimomae, Toda, Saitama, 335-0016, Japan |
|---|---|
| TEL | 048-446-2345 |
| FAX | 048-444-7756 |
| Web site, SNS | https://www.paleolabo.jp/English_site/e-toppage.html |
ZEISS
ZEISS
Introduction of ZEISS Microscopy
ZEISS is proud to celebrate its heritage of the longest history in geoscience imaging of any company. From micropaleontology to mineralogical studies, technologies such as X-ray microanalysis and cathodoluminescence along with advances in scanning electron microscopy are extending your research capabilities today and tomorrow.
We will be participating in the Quiz Rally, come join us to win amazing prizes!
We will be participating in the Quiz Rally, come join us to win amazing prizes!
Solutions
1. Discover the new possibilities of automated petrography with ZEISS Axioscan 7 Digitize your thin sections with Axioscan 7 – the reliable, reproducible way to create high quality, digitized petrography data in transmitted and reflected light
2. Automate Your Mineralogy to Increase Productivity with Mineralogic
ZEISS Mineralogic is the ideal solution for exacting geological interrogation of your samples, from in-depth petrological investigations to high throughput mineral liberation workflows
3. Diffraction Contrast Tomography Module for X-Ray Microscopy
Laboratory Diffraction Contrast Tomography (LabDCT) is a unique grain imaginganalytical technology, enabling thenon-destructive mapping of orientation and microstructure in 3D. It is the first-ever laboratory-based diffraction contrast tomography imaging module, obtaining 3D crystallographic information from polycrystalline samples.
4. Discover the Unknown with Ultimate Imaging and Effortless Analytics with ZEISS GeminiSEM
ZEISS GeminiSEM stands for effortless imaging with sub-nanometer resolution. Take sub-nanometer images below 1 kV without an immersion lens. Explore, how the GeminiSEM family answers all your imaging and analytical needs.
ZEISS Seminar Talk: “Digital Petrology”: How automation and digitalization is revolutionizing microscopy based petrographic studies
Timing of Session: 3rd June 2021, 10:45-11:30 Abstract
In 1851, Henry Sorby (Sheffield, England) laid the foundations of microscopy-based petrography. The innovation was the use of two Nicol-prisms to be able to study a slice of rock with polarized light. The second level of foundations of microscopy-based petrography occurred sometime after the 1965 introduction of commercial Scanning Electron Microscopy (SEM) by Sir Charles Oatley (Cambridge, England). Since these innovations established the “foundations of petrography”, there has been little technological innovation to address some of the challenges in microscopy-based petrography. These challenges can be summarized as the following:
1. Sampling bias and sample heterogeneity
2. Resolutions vs Field of View (FoV)
3. Unable to quantify and therefore a subjective technique
In this presentation innovations and the development of “Digital Petrography” technology can:
1. Automated data acquisition of 10’s – 100’s of thin sections in Light and Electron Microscopy. This enables high resolution and large area digitization to solve the “resolution vs FoV” challenge and understanding heterogenous samples.
2. Classification of the mineralogy and quantification to product modal mineralogy (etc.) and thus removing subjectivity.
The innovations that are allowing Geologists to address these challenges will be discussed to understand the technological developments and their applications through multiple case studies.
Talk to a ZEISS Specialist
Join us at the popup session and talk to a ZEISS Specialist to answer all your questions! Time: 4th June 2021, 13:45 - 15:15
Book a meeting at your convenience via Teams call
Date and Time (JST):
6月1日（火）●11:00- ●12:00- ●15:00- ●16:00-
6月2日（水）●11:00- ●12:00- ●15:00- ●16:00-
6月3日（木）●11:00- ●12:00- ●15:00- ●16:00-
6月4日（金）●11:00- ●12:00- ●15:00- ●16:00-
Book A Session with Our Specialists Here
If you have further inquiries, please email us at marketing.microscopy@zeiss.com
Dont miss the latest geoscience information, sign up for our newsletter to receive regular updates! Sign up here!
| Address | 102-0083 2-10-9 Kojimachi, Chiyoda-ku, Tokyo 102-0083 Japan |
|---|---|
| TEL | 0570-02-1310 |
Sairisha
Sairisha
Crochet Radiolaria
Radiolaria, a kind of plankton, have been living in the ocean from the Paleozoic era to the present. They are unicellular organisms with hard skeletons of various shapes. A major group of radiolaria (Polycystina) makes siliceous skeleton, which is stable in geologic time and often found from marine sediment. Their rapid change and variety in skeleton shapes make them good index fossils. They are about 0.1 - 0.5 mm in size.Radiolarian skeletons look like beautiful glassworks under microscope. I am making crocheted daily goods with cotton yarn expressing the shape and luster of radiolarians.
Works
catalogue (click to enlarge)
example of use
trial product
Online Shop
Online Shop Service (in Japanese)
Creator Profile
Keiko Mizugaki, Doctor of Science1984 - 1985: study on Mesozoic radiolaria at Nagoya University
1986 - 2018: study on geothermal geology at the Geological Survey of Japan
Related papers*
1) Mizugaki, K. (1985) Radiolarian Fossils from the Chichibu System, Northwest of Hamana Lake, Central Japan. Bulletin of the Mizunami Fossil Museum, 12, 171-182. (in Japanese with English abstract)
2) Mizugaki, K. (1987) Mesozoic radiolarians in conglomerate of the Shimanto Supergroup in the Sazara-ura Area, eastern Kii Peninsula, Central Japan. Bulletin of the Nagoya University Museum, 3, 19-69. (in Japanese with English abstract)
*Please contact me via Twitter (open DM) or the contact form for PDF files.
| Web site, SNS | http://sairisha.net/ |
|---|
SANYO-TRADING / PICARRO
SANYO-TRADING / PICARRO
◆New! Express & Survey Mode is now available for FREE! (Until December 31, 2021)
Normally, 27 samplings could be performed a day in Standard Mode,Picarro has released new Express Mode and Survey Mode!
Expresse Mode: 50 samplings per day
Survey Mode: 900 samplings can be executed per day
Now you can get two modes for free.
Click the image below for details.
* Limited to customers who have newly purchased L2130-i.
◆Exhibit contents
We will exhibit a gas analyzer and stable isotope ratio analyzer.It is a device that can measure the concentration of environmental gases such as carbon dioxide and methane with high accuracy over a long period of time.
With this device, the gas concentration can be calculated directly, so there is no need to calibrate frequently.
PICARRO's equipment uses a high-precision laser wavelength monitor to achieve highly stable and highly accurate measurements.
More than 2000 products are used in 60 countries and are measured in a wide variety of locations, in harsh environments such as automobiles, ships, aircraft, deserts and polar regions, volcanoes, forests and lakes.
◆ Stable isotope ratio analysis of oxygen and hydrogen (δ18O, δ17O, δD)
→ Oxygen hydrogen stable isotope ratio analyzer L2130-i, L2140-i
◆ Stable isotope ratio analysis of carbon nitrogen
→ Stable isotope ratio analyzer G2210-i, G2201-i, G2101-i
→ Nitrogen stable isotope ratio analyzer G5131-i
◆ Greenhouse gas analyzer
→ Portable gas analyzer G4301, G4302
→ Multi-gas analyzer G2301, G2308, G2401, G5310
◆ Soil science gas analyzer
→ Ammonia gas analyzer G2103
→ Portable gas analyzer G4301, G4302
→ Multi-gas analyzer G2301, G2308, G2401, G5310
◆About the device / Catalog and latest news
Oxygen hydrogen stable isotope ratio analyzer L2140-i-Easy operation by cavity ringdown spectroscopy (CRDS)
・ Measurement of 17O-excess, δ17O, δ18O, δD of liquid, gas, and solid is possible.
・ Can be used in the laboratory or outdoors
Carbon stable isotope ratio analyzer G2210-i
・ Cavity ring-down spectroscopy (CRDS)
・ Measure carbon stable isotope ratio (δ13C), methane (CH4) concentration, and ethane (C2H6) concentration of methane (CH4) in real time.
Portable gas analyzer G4302
・ Methane gas (CH4), ethane gas (C2H6)
・ Simultaneous measurement of ppb level is possible
・ Cavity ring-down spectroscopy (CRDS)
・ Portable gas analyzer that can be carried
Please see the following URL for details.
◆Information on online seminars
Title「Latest Application Developments from Picarro」
Topics:
①Picarro introduction
②New Express and Survey modes for isotopic water analyzers – highest throughput solution
③New OC/EC solution for isotopic carbon analyzers – tracing air pollution
④Open access book on GHG measurement techniques – versatile CRDS deployment methods for GHG studies
Speakers:
Dr. Zhiwei Lin（Principal Application Scientist）
Thomas Gottschalk（Director of Sales, Asia Pacific）
| Address | 101-0054 2-11, Kanda Nishiki-cho, Chiyoda-ku Tokyo, 101-0054 Japan |
|---|---|
| TEL | 0335181196 |
| FAX | 0335181237 |
| Web site, SNS | https://www.sanyo-si.com/products/maker/picarro/ |