Daily Variation of Cosmogenic Nuclide Be-7 Concentrations in High Altitude Atmosphere at Mt. Chacaltaya in the solar minimum from 2009 Hirohisa Sakurai.

Slides:



Advertisements
Similar presentations
SBUV/2 Observations of Atmospheric Response to Solar Variations Matthew DeLand Science Systems and Applications, Inc. (SSAI) Background -SBUV/2 instruments.
Advertisements

COSMIC RAY PHYSICS IN BOLIVIA 4TH School on Cosmic Rays and Astrophysics UFABC-Santo André-SP-Brasil August 2010 Alfonso Velarde Cosmic Ray Laboratory.
Quantifying uncertainties of OMI NO 2 data Implications for air quality applications Bryan Duncan, Yasuko Yoshida, Lok Lamsal, NASA OMI Retrieval Team.
Bastille Day 2000 Solar Energetic Particles Event: Ulysses observations at high heliographic latitudes M. Zhang Florida Institute of Technology.
Cosmic rays in solar system By: Tiva Sharifi. Cosmic ray The earth atmosphere is bombarded with the energetic particles originating from the outer space.
The Pierre Auger Project By Megan Edwards Bancroft-Rosalie.
1 Trends and Anomalies in Southern Hemisphere OH Inferred from 12 Years of 14 CO Data Martin Manning, Dave Lowe, Rowena Moss, Gordon Brailsford National.
CLIMATOLOGICAL ANALYSIS OF OZONE AND METEOROLOGICAL PARAMETERS A BACKGROUND SITE: CERRO TOLOLO 30ºS,70ºW, 2200 m.a.s.l. Ana Maria Cordova CMM.
Solar Activities and Halloween Storms Ahmed Hady Astronomy Department Cairo University, Egypt.
Search for solar neutrons associated with proton flares in solar cycle 23 Yutaka Matsubara (presenter) Solar-Terrestrial Environment Laboratory, Nagoya.
Chapter 2 Solar Energy, Seasons, and the Atmosphere
Chapter 2 Solar Energy, Seasons, and the Atmosphere Elemental Geosystems 5e Robert W. Christopherson Charles E. Thomsen.
Solar Energetic Particles -acceleration and observations- (Two approaches at the highest energy) Takashi SAKO Solar-Terrestrial Environment Laboratory,
IACETH Institute for Atmospheric and Climate Science Representation of Middle Range Energy Electrons in the Chemistry-Climate Model SOCOL Pavle Arsenovic.
Warm Up 3/4/08 True or False: The seasons are caused by changes in Earth’s distance from the sun. False Does land or water heat more rapidly? Land heats.
Belle Tamir, Sharet High School Nitzan Atia, Tchernichovsky High School Netanya, Israel.
Atmospheric temperature
Jae H. Kim 1, Sunmi Na 1, and Mike Newchurch 2 1; Department of Atmospheric Science, Pusan Nat’l University 2; Department of Atmospheric Science, University.
THE ATMOSPHERE OF THE EARTH
Introduction A new methodology is developed for integrating complementary ground-based data sources to provide consistent ozone vertical distribution time.
Radiation in Your Environment. Radiation Around You Nature –Cosmic (direct and cosmic-produced radioactivity –Terrestrial (including radon) Medical Consumer.
Radiation conditions during the GAMMA-400 observations:
Cosmogenic Dating.  A group of isotopic methods of age determination based on accumulation of certain nuclides, which are produced only in the top few.
TRENDS IN ATMOSPHERIC OZONE FROM A LONG-TERM OZONE CLIMATOLOGY Jane Liu 1,2, D. W. Tarasick 3, V. E. Fioletov 3, C. McLinden 3, J. H. Y. Jung 1, T. Zhao.
Lesson 01 Atmospheric Structure n Composition, Extent & Vertical Division.
222Rn daughters influence on scaler mode of ARGO-YBJ detector Irene Bolognino, University of Pavia and INFN E. Giroletti,C. Cattaneo,G. Liguori,P. Salvini,P.
The PLANETOCOSMICS Geant4 application L. Desorgher Physikalisches Institut, University of Bern.
Cosmic-Ray Induced Neutrons: Recent Results from the Atmospheric Ionizing Radiation Measurements Aboard an ER-2 Airplane P. Goldhagen 1, J.M. Clem 2, J.W.
By Dr. A. Mahrous Helwan University - EGYPT By Dr. A. Mahrous Helwan University - EGYPT.
Research Activities in Japan and other Asian Countries 1. Ground-based observation - AGAGE monitoring stations: China, Korea, and Japan - NDACC stations:
NMDB - the European neutron monitor database Karl-Ludwig Klein, for the NMDB consortium.
Kelvin Waves as Observed by the SABER Instrument on the TIMED Spacecraft Jeffrey M. Forbes, Xiaoli Zhang, Saburo Miyahara, Scott E. Palo, James Russell,
The Atmosphere Composition, Structure and Temperature.
Stellenbosch University
Atmosphere: Structure and Temperature Bell Ringers:  How does weather differ from climate?  Why do the seasons occur?  What would happen if carbon.
 Gasses make up the air around us  Primary gasses are Nitrogen and Oxygen  Small amounts of many other gasses are present.
Recent Results of Individual Asian Dust Particle Analysis Daizhou Zhang Prefectural University of Kumamoto, Japan Yasunobu Iwasaka, et al. Nagoya University,
Air-showers, bursts and high-energy families detected by hybrid experiment at Mt.Chacaltaya M.Tamada Kinki University M.Tamada ICRC2011, Beijing, 15 Aug.
Radiation Storms in the Near Space Environment Mikhail Panasyuk, Skobeltsyn Institute of Nuclear Physics of Lomonosov Moscow State University.
Reconstruction of the solar activity in 7th-11th centuries by the carbon 14 content in tree-rings F USA M IYAKE 1, K ENTARO N AGAYA 1, K IMIAKI M ASUDA.
東京工業大学 理工学研究科 基礎物理学専攻 寺澤研究室 修士2年 樋口千夏
The Atmosphere.
The Atmosphere Aim: How are the layers of the atmosphere organized?
Stratospheric Ozone Brent Greenhalgh and Carrie Welker Reviews in Earth Science Oct. 4, 2011 September 17, 1979 October 1, 2010 (NASA, )
Atmosphere. What makes up our atmosphere?  Nitrogen  Oxygen  Argon.
Ion Acceleration in Solar Flares Determined by Solar Neutron Observations 2013 AGU Meeting of the Cancun, Mexico 2013/05/15 Kyoko Watanabe ISAS/JAXA,
Earth’s Atmosphere.
17 Chapter 17 The Atmosphere: Structure and Temperature.
A New Solar Neutron Telescope working at the International Space Station K. Koga, T. Goka (PI), H. Matsumoto, T. Obara, O. Okudaira (JAXA) Y. Muraki (Nagoya)
10/20/11SESAPS111 Correlation study of atmospheric weather and cosmic ray flux variation Kanishka Dayananda Georgia State University.
Periodic Variations in Muon Flux at Project GRAND Thomas A. Catanach, John Poirier ICRC August 2011.
Temporal Variations of 7Be and its AMAD over “Demokritos” GAW station
Cosmogenic Muon Background
ENERGETIC NEUTRONS FROM PARTICLE ACCELERATION
Disciplines of Science, ch. 16
Observation of cosmogenic nuclide Be-7 concentrations in the air at Bangkok and trajectory analysis of global air-mass motion S. Suzuki , H. Sakurai ,
Search for Cosmic Ray Anisotropy with the Alpha Magnetic Spectrometer on the International Space Station G. LA VACCA University of Milano-Bicocca.
Seasonal dependence of the nighttime traveling ionospheric disturbances in the mid-latitude ionosphere A.Saito1,2, M.C. Kelley1, T. Tsugawa2, J.J. Makela1,
Earth’s Atmosphere.
Charles Lin1, Jia-Ting Lin1, Loren Chang2, Yang-Yi Sun2
32nd International Cosmic Ray Conference, Beijing
本田 建 (山梨大学) Knee 領域のEnergy Spectrum
Detection of Solar Neutrons and Protons by the ground level detectors
Forbush and GCRDs First rigorous experimental observation of Cosmic Ray Flux Decrease was obtained by S. E. Forbush in , after deep statisitcal.
Simulation of 14C production rates for the troposphere and stratosphere in weak geomagnetic intensity at 26,000 yr BP 1 Graduate School of Science and.
NMDB - the European neutron monitor database
Unit: Water and the Atmosphere Lesson 3: Layers of the Atmosphere
The Layered Atmosphere:
Analysis of Solar gamma-rays and Solar-neutrons detected on  March 7th and September 25th of 2011 by the ground level    Neutron Telescopes, SEDA-FIB.
The Atmosphere.
Presentation transcript:

Daily Variation of Cosmogenic Nuclide Be-7 Concentrations in High Altitude Atmosphere at Mt. Chacaltaya in the solar minimum from 2009 Hirohisa Sakurai

H. Sakurai 1, T. Sato 1, T. Oe 1, S. Kikuchi 1, Y. Takahashi 1, S. Namai K. Masuda 2, Y. Matsubara 2, H. Miyahara 3, H. Ohashi 4, W. Tavera 5, J. Salinas 5 1. Department of Physics, Yamagata University, Kojirakawa,Yamagata , Japan 2. STEL, Nagoya University, Furocho chikusa-ku, Nagoya , Japan 3. ICRC, The University of Tokyo, Kashiwanoha Kashiwa- city, , Japan 4. Tokyo University of Marine Science and Technology, Kounan Minato-ku, Tokyo, Japan 5. IIF, Universidad Mayor De San Andres, Calle 27 Cota Cota s/n Campus Universitario, La Paz, Bolivia

The cosmogenic nuclides, which are radioisotopes produced in the Earth by cosmic rays, show the solar variations?

Stratosphere Geomagnetic fields Solar magnetic fields Cosmic rays 22 Na 14 C 10 Be 7 Be Troposphere 12 km Radioisotopes produced by cosmic rays in the Earth

Daily Sampling and Measurement of Be-7 in the atmosphere from 2000 High Volume Air Sampler (HV-100F) Sampling time: 23 hours/day Intake rate: 1000 L/min. Collected filter ・ Glass fiber filter collection efficiency : 99.99% (  m particle ) ・ Glass fiber filter collection efficiency : 99.99% (  m particle ) HPGe detector Measurement time : 6 hours detection efficiency 2.68% resolution @ 1.33MeV 1.69keV Sampling site Altitude: 153 m Latitude: Longitude:140.3

Yearly profile of Be-7 concentrations

Daily profile of Be-7 Japan

Daily sampling of Be-7 in atmosphere at high altitude Expecting observation of short term variations such as 27-day, GLE, Fourbush decrease, CME, etc. Chacaltaya Altitude: 5600 m (16.34° S, 68.12° W)

Sampling at Chacaltaya HV-500F

Rn-222 Pb-210 Be-7 Stratosphere Troposphere Cosmic Ray origin and Earth origin Rn-222 Pb day Attempting to remove the environmental effects of the Earth

Monthly profiles of Be-7 and Pb-210 Chacaltaya The profiles show a seasonal variation, including different variability.

Daily profiles of Be-7 and Pb-210 Chacaltaya Sharp peaks of Be-7 is visible compared to Pb-210

Periodic components of Be-7 and Pb-210 concentrations Be-7 Pb-210 For the days from100 to 200, the periodicity around 27-day are different for the Be-7 and the Pb-210.

Correlation between daily concentrations of Be-7 and Pb-210

Be-7 concentrations subtracting the correlation components between Be-7 and Pb-210 Be-7s show up sharp peaks with a periodic component around 27-day.

Summary In addition to the observation of daily Be-7 concentrations in the atmosphere at middle latitude from 2000, we started daily observation of Be-7 concentrations at Chacaltaya in the altitude of 5600 m from September Using correlation with Pb-210, we tried to extract the variation of Be-7 connecting to short term solar variability for one year data.