The new information about UV radiation of the Earth's atmosphere according to the «Universitetskij-Tatiana-2» data D.V.Skobeltsyn Institute of Nuclear.

Slides:



Advertisements
Similar presentations
Earth’s Weather Patterns
Advertisements

Lightning Imager and its Level 2 products Jochen Grandell Remote Sensing and Products Division.
Stacking up the Atmosphere ELF Activity: Atmosphere 5A.
Lecture 12 Content LIDAR 4/15/2017 GEM 3366.
FCFM-BUAP VIII Latin American Symposium of High Energy Physics, 6-12 December 2010, Valparaiso, Chile Study of UV atmospheric background for UHECR detection.
 Intracloud  Cloud-to-Cloud  Anvil Crawlers  Cloud-to-Air  Sprites and Jets.
MSU Space Project «Lomonosov». MSU Space Project «Lomonosov» Participants of the experiment (preliminary list): M.V. Lomonosov Moscow State University.
Ultraviolet Radiation Detector of the MSU Research Educational Micro satellite UNIVERSITETSKIY-TAT’YANA Garipov G.K., Panasyuk M.I., Tulupov V.I., Khrenov.
RESEARCH RESULTS ON ATMOSPHERIC ELECTRIC FIELD AT OBSERVATORY PARATUNKA IN KAMCHATKA. V.V. Kuznetsov, N.V. Cherneva, G.I. Druzhin, I.Y. Babahanov. Institute.
TROPOSPHERE The troposphere is the lowest layer of Earth's atmosphere. The troposphere starts at Earth's surface and goes up to a height of 7 to 20 km.
Stratosphere Troposphere
the Ionosphere as a Plasma
Chapter 4.1- Earth’s Atmosphere Pages Earth’s Atmosphere Atmosphere- a thin protective layer of air that surrounds the Earth and makes life possible.
Meteorology \ Dr. Mazin sherzad
Sponge: List the six layers of the Earth.. Atmosphere A mixture of gases: N 2 78% O 2 21% Ar0.9% CO %
The Atmosphere Essential Question: What is the significance of the atmosphere to the existence of life on earth? pp
The Atmosphere.
Interrelation between Cosmic Rays, Magnetosphere particles and the Earth Atmospheric Phenomena- Prospects of Experimental Study from Satellites M.I. Panasyuk.
RELEC project (Relativistic ELECtrons). Unified platform “Karat” for small spacecraft 2 MICROSATELLITE KARAT FOR PLANETARY MISSIONS, ASTROPHYSICAL AND.
UV data of the “Universitetsky-Tatiana-1” satellite and plans for the Tatiana-2. A.V. Dmitriev, G.K. Garipov, O.R. Grigoryan, B.A. Khrenov, P.A. Klimov,
TUS/KLYPVE Program for Observation of Extreme Energy Cosmic Rays from Space B.A. Khrenov DV Skobeltsyn Institute of Nuclear Physics of MV Lomonosov Moscow.
International research project GALA: Monitoring of high energy gamma-ray astrophysical sources.
RELEC project (Relativistic ELECtrons). Satellites Low altitudes Geostationary Balloons Arctic Antarctic Ionosphere Atmosphere particles Space and balloon.
Workshop on Coupling of Thunderstorms and Lightning Discharges to Near-Earth Space June 2008, University of Corsica, Corte in Corsica, France (weekends.
The Atmosphere.
G.K. Garipov 1, B.A. Khrenov 1, P.A. Klimov 1, V.S. Morozenko 1, M.I. Panasyuk 1, V.I. Tulupov 1, V.M. Shahparonov 1, S.A. Sharakin 1, S.I. Svertilov 1,
NCKU UCB Tohoku ISUAL / ROCSAT-2 August 2001 Sprites observation by ISUAL on the ROCSAT-2 satellite J. L. Chern, R. R. Hsu, H. T. Su, A. B. Chen, and L.
Stacking up the Atmosphere ELF Activity: Atmosphere 5A.
On the Role of Electric Field Changes when Calculating Thunderstorm Currents Yu.V. Shlugaev, V.V. Klimenko, E.A. Mareev Institute of Applied Physics RAS,
REMOTE SENSING IN EARTH & SPACE SCIENCE
An introduction to our active ionosphere begin
Transient Luminous Effects as observed onboard "Tatiana-1” and "Tatiana-2" satellites Mikhail Panasyuk Skobeltsyn Institute of Nuclear Physics of Lomonosov.
 Ranges from 0 km to 12 km  Lowest layer of the atmosphere  Where we live  Where almost all of the Earth’s weather occurs  “Tropo” means turning.
Atmosphere.
UV And Red-IR Radiation Flashes Energy Characteristics Measured by UV&IR Detector On-Board “Universitetsky-Tatiana-2” Satellite. G.K. Garipov 1, B.A. Khrenov.
Layers of the Atmosphere
Bellwork March 1, 2007 Define the following words: Page 434 Define the following words: Page 434 –Atmosphere –Troposphere –Ionosphere –Ultraviolet Radiation.
SPRITE OBSERVATIONS DURING MEIDEX Yoav Yair, Colin Price, Zev Levin and Adam Devir Department of Geophysics and Planetary Sciences, Tel Aviv University,
Astronomy 1010 Planetary Astronomy Fall_2015 Day-23.
Monday, January 30th Key Question: How do the layers of the atmosphere affect us? HW: Read Chapter 15, Section 2, take notes and answer Self Check questions.
Some results of observation of ultraviolet and infrared emission from lightning discharges at Aragats Cosmic Station LEAD workshop Armenia, NOR AMBERD.
LPCE:CETP: CESR: LONG DURATION FLIGHTS OF BALLOONS FOR THE STUDY OF STRATOSPHERIC CHEMISTRY IN THE FRAME OF THE TARANIS PROJECT LPCE:Gwenaël BERTHET CETP:
ISUAL Design Concept S. Mende. SDR 7 Jun NCKU UCB Tohoku ISUAL Design Concept S. Mende Sprite Example Sprite Image obtained by Berkeley/NCKU 1999.
The Atmosphere The atmosphere is the layer of gases that surrounds the Earth. Earth’s atmosphere is a mixture of nitrogen, oxygen, water vapor, and many.
Simulation of Terrestrial Gamma Ray and Neutron Flashes (Small variations of thundercloud dipole moment) L.P. Babich, Е.N. Donskoĭ, A.Y. Kudryavtsev, M.L.
Layers of the Atmosphere
Exosphere  Uppermost layer  Beyond this lies space.
The Atmosphere Layers. What’s the atmosphere made of? Nitrogen % Oxygen % Argon -.934% CO % Neon % Helium % Methane.
The Atmosphere.
The Atmosphere.
Sponge: List the six layers of the Earth.
for Lomonosov-GRB collaboration
Exploring Earth’s Atmosphere
By: Armani Haynes, and Noelle Nguyen,Mariana Nunez
E. Ponce2-1, G. Garipov2, B. Khrenov2, P. Klimov2, H. Salazar1
Layers of the Atmosphere
The Atmosphere.
Electromagnetic Spectrum
A mixture of gases that surrounds a planet
Layers of the Atmosphere
R. Bucˇık , K. Kudela and S. N. Kuznetsov
V. M. Lipunov, E. S. Gorbovskoy
The Atmosphere.
Why is it so important to life on earth?
Chapter 11 Section 2 What are the layers of the atmosphere?
Electromagnetic Waves
Atmospheric Layers.
The Layered Atmosphere:
The Structure of the Atmosphere
Unit: Weather and Climate
Presentation transcript:

The new information about UV radiation of the Earth's atmosphere according to the «Universitetskij-Tatiana-2» data D.V.Skobeltsyn Institute of Nuclear Physics, Moscow State University, Vorobjevy Gory 1, Moscow , Russia.

OBJECTIVE OF THE EXPERIMENT Simulataneous research of the transient events by means of optic and charged particles detectors. The studies of the connections between the transient events and the processes in the near-Earth space and atmospheric processes in the electrically-active zones of the Earth. Detectors onboard «Tatiana-2» satellite: Charged particles detector with total area of 400 cm 2 (FZK) UV ( nm) and red ( nm) radiation detector (DUFIK)

MSU VNIIEM EWHA Woman's University, Seoul, Korea University of Puebla (BUAP), Puebla, Mexico. Carrier rocket: “Soyuz-2” Upper-stage rocket “Fregat” Operating orbit: Polar Sun synchronous Altitude: 800 – 850km Inclination Mass: 100kg Power: 100W Contribution from:

«Tatiana-2» launching

«Tatiana-2» satellite's orbit

DUFIK and FZK detectors' block diagram Digital oscilloscope: Oscillogram width — 128 мс Integral action time for trigger output — 1 ms Fixation of the most powerful event during the minute Automatic arrangement of photomultiplier amplification High voltage changes depending on UV background

Research of the Transient Luminous Events (TLE): blue jets, sprites, gigantic jets, elves.

UV flashes registration examples

Geographical distribution of the flashes measured by «Tatiana-2» detector in October-November 2009

One day transient flashes distribution on the Global clouds map 16 of November 2009

Typical distribution of the lightnings above the clouds during the hours of the maximum thunderstorm activitey (by

Oscillogram example. Simultaneous measurements of ultraviolet, infrared and charged particles density.

Town UV light at night measured by “Tatyana-2”

Global charged particles distribution measured by “Tatyana-2” November 2009

UV flashes global distribution on the map of total column water vapor

Conclusion 1.The global distribution of the transient flashes (over 1000 events) is obtained 1.Portion of flashes is observed in the cloudless regions 1.It is proved that the transient discharges are produced not only by lightnings as it was considered by now but also by other reasons which are still unknown 1.The flashes are not detected by the Global network of lightning registration by means of radio signals within the range of ultra-long waves. It indicates that the flashes are located higher than the lower boundary of the ionosphere. 1.The flashes are not observed above Sahara desert. Probably, it indicates the important role of the water vapor in the production of the Earth's electric field not only in the troposphere, but also in the ionosphere. Data processing is in progress.