ACE/EPAM (ELECTRON, PROTON, AND APLPHA MONITOR) INTERCALIBRATION WITH STEREO/SEPT SEP EVENT OBSERVATIONS Olga Malandraki Institute of Astronomy and Astrophysics,

Slides:



Advertisements
Similar presentations
W.J. Merline, Southwest Research Institute, Boulder P.M. Tamblyn, Southwest Research Instutute, Boulder W.M. Owen, Jet Propulsion Lab, Pasadena C. Neyman,
Advertisements

BELGISCH INSTITUUT VOOR RUIMTE-AERONOMIE INSTITUT D’AERONOMIE SPATIALE DE BELGIQUE BELGIAN INSTITUTE FOR SPACE AERONOMY BELGISCH INSTITUUT VOOR RUIMTE-AERONOMIE.
Xin LiuMOP The growth of plasma convection in Saturn’s inner magnetosphere X. Liu; T. W. Hill; R. A. Wolf; Y. Chen Physics & Astronomy Department,
On the link between the solar energetic particles and eruptive coronal phenomena On the link between the solar energetic particles and eruptive coronal.
ASTROSAT Prospects for a Hard X-ray Survey  ASTROSAT Overview  LAXPC Details  Science Prospects  Hard X-ray Survey Prospects  Beyond ASTROSAT Biswajit.
M1.0 flare of 22 Oct 2002 RHESSI observations of the M 1.0 solar flare on 22 October 2002 A. Berlicki 1,2, B. Schmieder 1, N. Vilmer 1, G. Aulanier 1 1)
1/03/09 De 89 à 98. 1/03/09 De 89 à 98 1/03/09 De 89 à 98.
Estimated SOFT X-ray Spectrum and Ionization of Molecular Hydrogen in the Central Molecular Zone of the Galactic Center Masahiro Notani and Takeshi Oka.
Ionization of H 2 by X-rays in the Central Molecular Zone of the Galactic Center Masahiro Notani and Takeshi Oka Department of Astronomy and Astrophysics,
Cross-calibration of SOHO/ERNE proton and heavy ion measurements with other particle instruments at L1 E. Valtonen, M. Paassilta, R. Vainio, O. Raukunen,
24 Oct 2001 A Cool, Dense Flare T. S. Bastian 1, G. Fleishman 1,2, D. E. Gary 3 1 National Radio Astronomy Observatory 2 Ioffe Institute for Physics and.
Terrestrial Gamma-ray Flashes. Gamma Ray Astronomy Beginning started as a small budget research program in 1959 monitoring compliance with the 1963 Partial.
Benjamin McCall and Takeshi Oka University of Chicago Kenneth H. Hinkle National Optical Astronomy Observatories Thomas R. Geballe Joint Astronomy Centre.
APh161 - Lecture 2: The Rate of Things Rob Phillips California Institute of Technology.
Global Climate Change: The Heart of the Matter. What we can see (observations) What is causing it (causes and evidence) What can happen (projections)
Impacts of Climate Change on Physical Systems PPT
STEREO IMPACT Critical Design Review 2002 November 20,21,22 1 LET Performance Requirements Presenter: Richard Mewaldt
New Operational Algorithms for Charged Particle Data from Low-Altitude Polar-Orbiting Satellites J. L. Machol 1,2 *, J.C. Green 1, J.V. Rodriguez 3,4,
Paper Plate Model of Carbon
Credit: Michael Owen, John Blondin Black hole pudding – on the quest for the ultimate accretion disk cooking recipe – Chefs de cuisine Dominikus Heinzeller.
IHY Workshop A PERSONAL VIEW OF SOLAR DRIVERS for Solar Wind Coronal Mass Ejections Solar Energetic Particles Solar Flares.
Decay Phase of Proton and Electron SEP Events E.I. Daibog 1, K. Kecskeméty 2, Yu.I. Logachev 1 1 Skobeltsyn Inst. of Nuclear Physics, Moscow State Univ.,
Where is Coronal Plasma Heated? James A. Klimchuk NASA Goddard Space Flight Center, USA Stephen J. Bradshaw Rice University, USA Spiros Patsourakos University.
Mark DierckxsensSpace Weather and Solar Energetic Particles1 M. Dierckxsens 1, K. Tziotziou 2, S. Dalla 3, I. Patsou 2, M. Marsh 3, N. Crosby 1, O. Malandraki.
Negative Ions in IEC Devices David R. Boris 2009 US-Japan IEC Workshop 12 th October, 2009 This work performed at The University of Wisconsin Fusion Technology.
Comparative data quality assessment for ACE SIS, ACE EPAM, WIND 3DP, SOHO/ERNE, and SOHO EPHIN during selected solar energetic particle events B. Heber.
Elemental Abundance variations of the Suprathermal Heavy Ion Population over solar cycle 23 M. Al Dayeh, J.R. Dwyer, H.K. Rassoul Florida Institute of.
Find the geometric mean between: 1.4 and and and and 20 Geometric Mean x is the geometric mean between a and b. a x x b = Similarity.
1 PEBS Prototype PERDaix was launched in October 2010 from Kiruna, Sweden.
DYNAMIC OF ELECTROMAGNETIC EMISSION DURING THE PERIOD OF SOLAR EXTREME EVENTS M.S.Durasova, V.M.Fridman, T.S.Podstrigach, O.A.Sheiner, S.D.Snegirev, Yu.V.Tikhomirov.
The acceleration and radiation in the internal shock of the gamma-ray bursts ~ Smoothing Effect on the High-Energy Cutoff by Multiple Shocks ~ Junichi.
Mauna Kea University of Hawaii 2.2-m telescope Toruń Centre for Astronomy 0.6-m telescope Jena Astrophysical Institute 0.9/0.6-m telescope Calar Alto Astronomical.
Prof. Steven Boggs UCB Space Sciences Laboratory SPI Instrument Team Activities Prof. Steven Boggs (PI) Dr. Cornelia Wunderer (SPI CoI) Dr. Emrah Kalemci.
VIIth Bulgarian-Serbian Astronomical Conference, 1- 4 June 2010, Chepelare, Bulgaria The INASAN Zvenigorod observatory plate collection Sergei V. Vereshchagin,
High Energy cosmic-Radiation Detection (HERD) Facility onboard China’s Space Station Shuang-Nan Zhang ( 张双南 ) Center for Particle Astrophysics.
Remembering Jack Tueller
THREE-DIMENSIONAL ANISOTROPIC TRANSPORT SIMULATIONS: A PARAMETER STUDY FOR THE INTERPRETATION OF MULTI-SPACECRAFT SOLAR ENERGETIC PARTICLE OBSERVATIONS.
Multi-spacecraft observations of solar energetic electron events during the rising phase of solar cycle 24 W. Droege 1, R. Gomez-Herrero 2, J. Kartavykh.
The large scale convection electric field, ring current energization, and plasmasphere erosion in the June 1, 2013 storm Scott Thaller Van Allen Probes.
Ulysses HISCALE Data Production and Archiving Status Report Report to Final Investigation Team Meeting Belmont Conference Center September 30, 2009 Thomas.
1 SEP Timing Studies: An Excruciatingly Brief Review Allan J. Tylka US Naval Research Laboratory, Washington DC SHINE 2006 Where was the CME when the SEPs.
This is a sentence made using 10 point font. This is a sentence made using 12 point font. This is a sentence made using 14 point font. This is a sentence.
From Heritage of Astronomy to Space Technological Heritage: A Perspective By Dr. Olga Dluzhnevskaya, Director of the Centre for the Astronomical Data,
。 33 投资环境 3 开阔视野 提升竞争力 。 3 嘉峪关市概况 。 3 。 3 嘉峪关是一座新兴的工业旅游城市,因关得名,因企设市,是长城文化与丝路文化交 汇点,是全国唯一一座以长城关隘命名的城市。嘉峪关关城位于祁连山、黑山之间。 1965 年建市,下辖雄关区、镜铁区、长城区, 全市总面积 2935.
Chemistry: Inside the Atom Chapter 3 Part 2. How Atoms Differ Atoms differ in the number of protons they have. – Oxygen has 8 Protons, Fluorine 9 Protons,
Contact: Dr. Johannes Labrenz Extraterrestrische Physik Institut für Experimentelle und Angewandte Physik Christian Albrechts-Universität.
EGU General Assembly 2016 Contact: Dr. Johannes Labrenz
Chandrayaan-2 Large Area Soft X-ray Spectrometer (CLASS)
EGU General Assembly 2016 Contact: Dr. Johannes Labrenz
Elemental Abundance variations of the Suprathermal Heavy Ion Population over solar cycle 23 M. Al Dayeh, J.R. Dwyer, H.K. Rassoul Florida Institute of.
LET Performance Requirements Presenter: Richard Mewaldt
@iphigenia_k A service for the continuous, real-time monitoring of the urban thermal environment and development of applications Iphigenia Keramitsoglou,
EGU General Assembly 2016 Contact: Dr. Johannes Labrenz
GIADA Grain Impact Analyser and Dust Accumulator
© The Author(s) Published by Science and Education Publishing.
Karl-Ludwig Klein & Rositsa Miteva
Indian Institute of Astrophysics
SOLAR FLARE OPTICAL SPECTROPOLARIMETRY
Tips Need to Consider When Organizing a College Event
HI !.
GLAST Workshop April 13, 2007 Argonne National Lab
Present-day irrigation mitigates heat extremes
کشف اولین سیاره‌ی فراخورشیدی خاکی
EVENT of 20 JANUARY 2005 INJECTION TIME of IONS, PROTONS and ELECTRONS
ماجستير إدارة المعارض من بريطانيا
Yue Chen (Los Alamos National Laboratory)
Picture 1 10 protons 10 neutrons = an electron.
Solar Energetic Electrons and Radio Emission Signatures
Max-Planck-Institut für extraterrestrische Physik
Presentation transcript:

ACE/EPAM (ELECTRON, PROTON, AND APLPHA MONITOR) INTERCALIBRATION WITH STEREO/SEPT SEP EVENT OBSERVATIONS Olga Malandraki Institute of Astronomy and Astrophysics, National Observatory of Athens SEPT meeting 26-27 July 2010, Kiel

EPAM (Gold et al., 1998) adapted from the flight-spare of HI-SCALE (Lanzerotti et al. 1992)

Deflected electrons, CA60, ACE/EPAM Geometrical factor = 0.103 cm2 sr DE1: 38-53 keV DE2: 53-103 keV DE3: 103-175 keV DE4: 175-315 keV LEFS60 ACE/EPAM Geometrical factor: 0.397 cm2 sr E’1: 45-62 keV E’2: 62-102 keV E’3: 102-175 keV E’4: 175-290 keV

DEs LEFS60

LEFS60

Malandraki et al. 2005, JGR LEMS30

LEFS150